{"as_of":"2026-08-10T01:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b9d2342392b98ffae09d752c850b0bc27ced081248d4feb7f05a1f780e329ef0","coverage":[{"denominator":114,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T23:10:51.469444Z","state":"measured"},{"denominator":103,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":103,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T16:36:20.025090Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"cited_work":{"arxiv_id":"2506.19166","doi":"10.48550/arxiv.2506.19166","metadata_source":"arxiv_reference","pith_arxiv_id":"2506.19166","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025 (Preprint 2506.19166)","venue":"ArXiv.org","work_id":"619dc44c-ebfb-43de-8baf-880056afca19","year":2025},"citing_paper":{"arxiv_id":"2508.16399","last_updated":"2026-05-06T16:25:25Z","snapshot_observed_at":"2026-08-07T07:38:52.963691Z","submitted_at":"2025-08-22T14:00:58Z","title":"Constraints on the extreme mass-ratio inspiral population from LISA data","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-18T21:45:55.600867Z"},"links":{"cited_paper":"/paper/2506.19166","citing_paper":"/paper/2508.16399"},"observation_digest":"sha256:250896692051811dd197b080b49162345e8825c588fe2fd8dc1f8814144b3ac0","observation_id":"cded2a44-d77e-4cc3-a0df-002f6aaf44f7","resolution":{"observed_at":"2026-05-18T21:46:51.657341Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"cited_work":{"arxiv_id":"2506.19166","doi":"10.48550/arxiv.2506.19166","metadata_source":"arxiv_reference","pith_arxiv_id":"2506.19166","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025 (Preprint 2506.19166)","venue":"ArXiv.org","work_id":"619dc44c-ebfb-43de-8baf-880056afca19","year":2025},"citing_paper":{"arxiv_id":"2604.21405","last_updated":"2026-07-08T08:18:54Z","snapshot_observed_at":"2026-07-12T18:39:55.261528Z","submitted_at":"2026-04-23T08:20:42Z","title":"Supermassive Black Hole Winds in X-rays: SUBWAYS IV. Tracing Radio Emission and Unveiling the Role of Winds","version":1},"reference_index":140,"source":"arxiv_source","source_observed_at":"2026-05-09T21:20:55.807127Z"},"links":{"cited_paper":"/paper/2506.19166","citing_paper":"/paper/2604.21405"},"observation_digest":"sha256:a7e0489c6499972b94aa808d338bf60afa68d83f0f90045a355837d8b3a7d44e","observation_id":"7e09ae67-2d61-441c-9663-244722581931","resolution":{"observed_at":"2026-05-09T21:23:25.307174Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.19166","snapshot_observed_at":"2026-08-08T16:36:20.025090Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05267","last_updated":"2026-08-05T18:00:00Z","snapshot_observed_at":"2026-08-09T23:10:27.019154Z","submitted_at":"2026-08-05T18:00:00Z","title":"Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-08T16:36:20.025090Z"},"links":{"cited_paper":"/paper/2506.19166","citing_paper":"/paper/2608.05267"},"observation_digest":"sha256:17d67bc437d29cddfac895fba2a914f690e8bd16f3719917992685ee078feb5e","observation_id":"00b488ea-6e37-42d0-92b9-99aa227c1fb3","resolution":{"observed_at":"2026-08-08T16:36:20.025090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2506.19166/citation-record","integrity":"/paper/2506.19166/integrity","json":"/paper/2506.19166/citation-record.json","paper":"/paper/2506.19166"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1805.01467","last_updated":"2018-05-03T18:00:00Z","snapshot_observed_at":"2026-07-06T06:37:16.373053Z","submitted_at":"2018-05-03T18:00:00Z","title":"A Population of Bona Fide Intermediate Mass Black Holes Identified as Low Luminosity Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.01467","snapshot_observed_at":"2026-08-06T23:10:42.378979Z","title":"Choi, E., Ostriker, J.P., Naab, T., Johansson, P.H., 2012","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.378979Z"},"links":{"cited_paper":"/paper/1805.01467","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c68656fff0a772115f546896a78302d20804632cb429142c327c5ab00d37b0f5","observation_id":"336b9a93-12b1-4cb2-9e97-3eb4b046653d","resolution":{"observed_at":"2026-08-06T23:10:42.378979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12432","last_updated":"2022-07-25T18:00:09Z","snapshot_observed_at":"2026-07-06T13:35:06.611122Z","submitted_at":"2022-07-25T18:00:09Z","title":"BASS XXII: The BASS DR2 AGN Catalog and Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.12432","snapshot_observed_at":"2026-08-06T23:10:45.564962Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.564962Z"},"links":{"cited_paper":"/paper/2207.12432","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a4570039407c5694109545dc0fd363f35fb702d820a602f2e54978ae6d334a26","observation_id":"cc52a82c-b2c3-4064-836e-25db646720ae","resolution":{"observed_at":"2026-08-06T23:10:45.564962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:10:47.561022Z","title":"doi: 10.1111/j.1365-2966.2011.19675.x, arXiv:1106.4284","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.561022Z"},"links":{"citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:406c26207d2f63e4a35affd84f7db0eaa9a4033e469e899c7f1374c19d46e71b","observation_id":"91acc9d0-c9c5-42bf-9204-3cf8762798d4","resolution":{"observed_at":"2026-08-06T23:10:47.561022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.07320","last_updated":"2023-06-12T18:00:01Z","snapshot_observed_at":"2026-07-06T15:41:43.459371Z","submitted_at":"2023-06-12T18:00:01Z","title":"UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.07320","snapshot_observed_at":"2026-08-06T23:10:45.988154Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.988154Z"},"links":{"cited_paper":"/paper/2306.07320","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a0fa76525d839a5b187519db075878dee780c531c4e758efd6002459efc6fe0d","observation_id":"c2a622fd-248b-4c4a-97b1-7bfd3a512919","resolution":{"observed_at":"2026-08-06T23:10:45.988154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.02317","last_updated":"2017-06-07T18:01:01Z","snapshot_observed_at":"2026-07-06T05:45:59.048278Z","submitted_at":"2017-06-07T18:01:01Z","title":"The primordial environment of supermassive black holes (II): deep Y and J band images around the z=6.3 quasar SDSS J1030+0524","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.02317","snapshot_observed_at":"2026-08-06T23:10:41.580952Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.580952Z"},"links":{"cited_paper":"/paper/1706.02317","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:b4e41ea990f67ee0011c72524d6d03405cd1577804ec42d22ee9fd8679b9f4ed","observation_id":"2ff7934c-1d42-4ce3-a656-3e90474a34be","resolution":{"observed_at":"2026-08-06T23:10:41.580952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.10395","last_updated":"2020-06-02T07:48:04Z","snapshot_observed_at":"2026-08-04T08:10:50.354039Z","submitted_at":"2019-10-23T07:53:11Z","title":"Spectral properties of quasars from Sloan Digital Sky Survey data release 14: The catalog","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.10395","snapshot_observed_at":"2026-08-06T23:10:48.447453Z","title":null,"venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.447453Z"},"links":{"cited_paper":"/paper/1910.10395","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:52a2c248a6245e8aebbac2020d5f325ea89475723ecd3e7aaf30ecfc3e33b6c8","observation_id":"fb584383-5a90-41f3-b23f-97f717560162","resolution":{"observed_at":"2026-08-06T23:10:48.447453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14490","last_updated":"2024-04-22T18:00:04Z","snapshot_observed_at":"2026-08-09T01:41:11.290967Z","submitted_at":"2024-04-22T18:00:04Z","title":"An Excess of AGNs Triggered by Galaxy Mergers in MaNGA Galaxies of Stellar Mass $\\sim10^{11}$ $M_{\\odot}$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.14490","snapshot_observed_at":"2026-08-06T23:10:42.553709Z","title":"ApJ 963, 53","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.553709Z"},"links":{"cited_paper":"/paper/2404.14490","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c11be7eee66e0fbf328156f56f3cf6dd8f639532c51c0aebba2c5b664a5b8997","observation_id":"69158930-d98f-4d8b-8719-da4ed30f280a","resolution":{"observed_at":"2026-08-06T23:10:42.553709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.10572","last_updated":"2021-06-19T21:07:24Z","snapshot_observed_at":"2026-07-06T11:20:59.954618Z","submitted_at":"2021-06-19T21:07:24Z","title":"The XMM-SERVS survey: XMM-Newton point-source catalogs for the W-CDF-S and ELAIS-S1 fields","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.10572","snapshot_observed_at":"2026-08-06T23:10:47.845230Z","title":"Ni, Q., Brandt, W.N., Luo, B., Garmire, G.P., Hall, P.B., Plotkin, R.M., Shemmer, O., Timlin, J.D., Vito, F., Wu, J., Yi, W., 2022a","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.845230Z"},"links":{"cited_paper":"/paper/2106.10572","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:d2db58b86b3204430caad1fdcc351a53e3ad0b61fa1364c017d3c79e83f5e787","observation_id":"01726e21-565e-405b-a5e7-0d583d0eea0a","resolution":{"observed_at":"2026-08-06T23:10:47.845230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.11242","last_updated":"2025-02-21T09:08:55Z","snapshot_observed_at":"2026-08-10T00:42:30.335418Z","submitted_at":"2024-01-20T14:50:22Z","title":"UNCOVERing the contribution of black holes to reionization in the JWST era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.11242","snapshot_observed_at":"2026-08-06T23:10:42.825254Z","title":"arXiv e-prints , arXiv:2401.11242doi:10.48550/arXiv.2401","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.825254Z"},"links":{"cited_paper":"/paper/2401.11242","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:7f54de25caaaf0505fa4ed8e113dd219372334a678b563ebf3cd453c85f932a8","observation_id":"13b55191-d7ff-49cb-9c71-7f2eeb4cb4a7","resolution":{"observed_at":"2026-08-06T23:10:42.825254Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08380","last_updated":"2015-07-30T05:19:46Z","snapshot_observed_at":"2026-07-06T04:25:18.071224Z","submitted_at":"2015-07-30T05:19:46Z","title":"Clustering of intermediate redshift quasars using the final SDSS III-BOSS sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.08380","snapshot_observed_at":"2026-08-06T23:10:43.194074Z","title":"MNRAS 453, 2779–2798","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.194074Z"},"links":{"cited_paper":"/paper/1507.08380","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a99064b2cd7b4955374d94757b03dca2ec1148755f1b95c0c0daf27de9c71e45","observation_id":"9474ee9d-971f-407d-893a-717b304afc9f","resolution":{"observed_at":"2026-08-06T23:10:43.194074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.1092","last_updated":"2015-02-19T20:04:35Z","snapshot_observed_at":"2026-07-06T03:50:59.029723Z","submitted_at":"2014-08-05T20:00:08Z","title":"Half of the Most Luminous Quasars May Be Obscured: Investigating the Nature of WISE-Selected Hot, Dust-Obscured Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.1092","snapshot_observed_at":"2026-08-06T23:10:41.254525Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.254525Z"},"links":{"cited_paper":"/paper/1408.1092","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:7e668b5228b6547475e5c152f7557eacae5680bd0ae0ea01b5595b2a30ce12f9","observation_id":"60a7d7ad-08b5-41f8-a16b-117054a8319f","resolution":{"observed_at":"2026-08-06T23:10:41.254525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.06357","last_updated":"2024-12-20T21:18:11Z","snapshot_observed_at":"2026-07-06T19:30:00.101083Z","submitted_at":"2024-10-08T20:48:56Z","title":"Galaxy evolution in the post-merger regime. II -- Post-merger quenching peaks within 500 Myr of coalescence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.06357","snapshot_observed_at":"2026-08-06T23:10:43.293091Z","title":"II – Post-merger quench- ing peaks within 500 Myr of coalescence","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.293091Z"},"links":{"cited_paper":"/paper/2410.06357","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:fc70efc9cb4b44376f0e947368d71c374f215468bf40f86dbbd9b430b390b5c3","observation_id":"17175e67-7b41-4c9d-ba56-000634569123","resolution":{"observed_at":"2026-08-06T23:10:43.293091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.06096","last_updated":"2017-09-18T18:00:06Z","snapshot_observed_at":"2026-08-07T18:22:34.530323Z","submitted_at":"2017-09-18T18:00:06Z","title":"Mapping the Lyman-Alpha Emission Around a z~6.6 QSO with MUSE: Extended Emission and a Companion at Close Separation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.06096","snapshot_observed_at":"2026-08-06T23:10:43.381473Z","title":"ApJ 848, 78","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.381473Z"},"links":{"cited_paper":"/paper/1709.06096","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:338a09a454a02089d2b81c26de736da29657b207c2de8c9cd71ea0375bd939ce","observation_id":"3e4dc2b2-74cc-4a20-a8c2-1d6ae37c4a0e","resolution":{"observed_at":"2026-08-06T23:10:43.381473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.04507","last_updated":"2017-02-15T09:00:10Z","snapshot_observed_at":"2026-08-06T09:31:01.506267Z","submitted_at":"2017-02-15T09:00:10Z","title":"AGN wind scaling relations and the co-evolution of black holes and galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.04507","snapshot_observed_at":"2026-08-06T23:10:43.482361Z","title":"A&A 601, A143","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.482361Z"},"links":{"cited_paper":"/paper/1702.04507","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c08ca3e64217ba239a8948b616870bb36af783f692629803dfe1dac10f2cf03b","observation_id":"8e275b1f-80fd-4377-9b9d-44016b336c23","resolution":{"observed_at":"2026-08-06T23:10:43.482361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.06806","last_updated":"2020-12-12T12:45:24Z","snapshot_observed_at":"2026-08-09T04:56:52.596969Z","submitted_at":"2020-12-12T12:45:24Z","title":"Mid-InfraRed Outburst in Nearby Galaxies (MIRONG) I: Sample Selection and Characterization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.06806","snapshot_observed_at":"2026-08-06T23:10:45.146733Z","title":"Jiang, Y .F., Stone, J.M., Davis, S.W., 2019","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.146733Z"},"links":{"cited_paper":"/paper/2012.06806","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:37386c34e0d2ad7b8afabf4a394fa51301ad1cc9f04b560795101163f2e83766","observation_id":"4dac0fcf-f84f-48cc-b875-14051f940193","resolution":{"observed_at":"2026-08-06T23:10:45.146733Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01252","last_updated":"2024-03-01T22:27:18Z","snapshot_observed_at":"2026-08-10T01:39:16.603920Z","submitted_at":"2023-07-03T18:00:01Z","title":"ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052","version":2},"cited_work":{"arxiv_id":"2307.01252","doi":null,"metadata_source":"pith","pith_arxiv_id":"2307.01252","snapshot_observed_at":"2026-08-06T23:10:53.373771Z","title":"ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052","venue":"astro-ph.GA","work_id":"3b1adbdb-2555-4f89-9a29-2a83f64bd846","year":2023},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.141455Z"},"links":{"cited_paper":"/paper/2307.01252","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a1b203cc30e9a0ca790f47525ee0dc2cb7969e8d2b10a3c0405be2e54fc31648","observation_id":"bf0ca4f4-bc87-40da-a31a-bd08d1976575","resolution":{"observed_at":"2026-08-06T23:10:53.379029Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.09888","last_updated":"2022-06-14T18:00:00Z","snapshot_observed_at":"2026-08-04T11:43:47.269954Z","submitted_at":"2022-01-24T19:00:00Z","title":"The black hole population in low-mass galaxies in large-scale cosmological simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.09888","snapshot_observed_at":"2026-08-06T23:10:44.612804Z","title":"MNRAS 514, 4912–4931","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.612804Z"},"links":{"cited_paper":"/paper/2201.09888","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:193e6de0fb9ce1a2c4235777a062e0c93a7bf5629543f162c730c1cbaef97d2a","observation_id":"b2a5bfaf-96d3-40ca-950a-2edb1b8e971c","resolution":{"observed_at":"2026-08-06T23:10:44.612804Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.16943","last_updated":"2024-02-26T19:00:01Z","snapshot_observed_at":"2026-08-06T02:06:39.150137Z","submitted_at":"2024-02-26T19:00:01Z","title":"The LOFAR-eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.16943","snapshot_observed_at":"2026-08-06T23:10:44.902024Z","title":"A&A 686, A43","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.902024Z"},"links":{"cited_paper":"/paper/2402.16943","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:58ba85a654e0c4f2b8d8d1250122bf71c8c5c33ab7f5cb7a17175d9ccd5760de","observation_id":"fa6d8025-96ec-4237-9200-197f5c413c52","resolution":{"observed_at":"2026-08-06T23:10:44.902024Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.2420","last_updated":"2012-09-11T20:00:06Z","snapshot_observed_at":"2026-07-06T02:55:24.800852Z","submitted_at":"2012-09-11T20:00:06Z","title":"Occupation of X-ray selected galaxy groups by X-ray AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.2420","snapshot_observed_at":"2026-08-06T23:10:40.903003Z","title":"Almaini, O., Wild, V ., Maltby, D., Taylor, E., Rowlands, K., de Lisle, T., Alat- alo, K., Harrold, J., Hewitt, G., Patil, P., Skarbinski, M., 2025","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:40.903003Z"},"links":{"cited_paper":"/paper/1209.2420","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:03c60a26cbfa5793a968ff27214794f7da4f3f5d2972d73818e1f113fb9a06b6","observation_id":"15a9fc1b-9612-45dc-8a2b-942387fca4ba","resolution":{"observed_at":"2026-08-06T23:10:40.903003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.03981","last_updated":"2023-10-31T23:16:30Z","snapshot_observed_at":"2026-08-03T02:22:14.735658Z","submitted_at":"2022-12-07T22:31:20Z","title":"The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.03981","snapshot_observed_at":"2026-08-06T23:10:45.286033Z","title":"MNRAS 530, 2688–2730","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.286033Z"},"links":{"cited_paper":"/paper/2212.03981","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:722751a0216eb425b7a295fe7864b836404506e9de5d3f132580ffc789e87280","observation_id":"b27c178b-7604-44c0-b0ce-b52a2c78f027","resolution":{"observed_at":"2026-08-06T23:10:45.286033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2112.08380","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:10:53.136736Z","title":"ApJ 925, 203","venue":null,"work_id":"a680672d-55b1-42d6-af4a-8eaf3467b1f8","year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.400215Z"},"links":{"citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:1adc6d03a6ec046f8f0c3270380f222b73efb1b9c73373a9ffc2e92591145768","observation_id":"b4923733-7d79-4fad-80af-b470920e3538","resolution":{"observed_at":"2026-08-06T23:10:53.144568Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.14745","last_updated":"2024-03-21T18:00:00Z","snapshot_observed_at":"2026-08-05T08:38:30.853368Z","submitted_at":"2024-03-21T18:00:00Z","title":"A candidate supermassive black hole in a gravitationally-lensed galaxy at $z\\approx10$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.14745","snapshot_observed_at":"2026-08-06T23:10:45.655605Z","title":"ApJ 965, L21","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.655605Z"},"links":{"cited_paper":"/paper/2403.14745","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c2952864ef4dff79900a716543e57c8efe2dbc3f468f6b6038af5a22e7e3fd18","observation_id":"3e70a280-30b7-4363-860b-4f793368c02d","resolution":{"observed_at":"2026-08-06T23:10:45.655605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.01261","last_updated":"2015-12-14T18:16:14Z","snapshot_observed_at":"2026-07-06T04:28:44.949920Z","submitted_at":"2015-09-03T20:04:55Z","title":"The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos","version":2},"cited_work":{"arxiv_id":"1509.01261","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.01261","snapshot_observed_at":"2026-08-06T23:10:53.008150Z","title":"The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos","venue":"astro-ph.GA","work_id":"ea45659a-e10e-49cd-b161-7bff3dbfb811","year":2015},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.734072Z"},"links":{"cited_paper":"/paper/1509.01261","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:e9e1a7d91d4d140c8530d2aed9998d71988a3cb9acfff730e4eeac94bea9d6a8","observation_id":"d0ad298e-3936-4644-971e-ca231d6c64dc","resolution":{"observed_at":"2026-08-06T23:10:53.013003Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:10:45.867579Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.867579Z"},"links":{"citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:ed83a4a1f183d8343e0d35eea83d682ceed98cc00e0b9c0520e05ff33334bdd4","observation_id":"bb9ca538-dae7-4982-b0ec-4fa9fbe5d8f3","resolution":{"observed_at":"2026-08-06T23:10:45.867579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12446","last_updated":"2022-12-31T09:05:06Z","snapshot_observed_at":"2026-08-10T00:43:51.239507Z","submitted_at":"2022-07-25T18:01:43Z","title":"A population of red candidate massive galaxies ~600 Myr after the Big Bang","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.12446","snapshot_observed_at":"2026-08-06T23:10:46.090377Z","title":"Nature 616, 266–269","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.090377Z"},"links":{"cited_paper":"/paper/2207.12446","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:9ab240643e6c4d4a45b4d8081b9eacbb6de899c8af29acdc3e563ea62bc401a5","observation_id":"a27ffb49-0d41-4ba9-b674-214a5621f702","resolution":{"observed_at":"2026-08-06T23:10:46.090377Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07109","last_updated":"2024-10-08T06:38:01Z","snapshot_observed_at":"2026-08-04T07:33:07.851362Z","submitted_at":"2024-03-11T19:00:03Z","title":"Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07109","snapshot_observed_at":"2026-08-06T23:10:46.283437Z","title":"Changing Look","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.283437Z"},"links":{"cited_paper":"/paper/2403.07109","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:39a0d983de27d90e9770f89204e4253fe5a1f972b6a4d43c6efb0de8f2318534","observation_id":"30fb20b9-1328-46df-8e7f-310442e3d23b","resolution":{"observed_at":"2026-08-06T23:10:46.283437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.08918","last_updated":"2023-08-29T19:36:47Z","snapshot_observed_at":"2026-08-07T09:12:12.390053Z","submitted_at":"2023-03-15T20:22:38Z","title":"A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.08918","snapshot_observed_at":"2026-08-06T23:10:46.443696Z","title":"arXiv e-prints , arXiv:2303.08918doi: 10.48550/arXiv.2303","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.443696Z"},"links":{"cited_paper":"/paper/2303.08918","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:3d741b6f74e6f9854ff7b5044474db58bb45b093bc6fc439bea1d2a0e052b7db","observation_id":"4ba93e99-af50-4099-82cf-64639bace2e0","resolution":{"observed_at":"2026-08-06T23:10:46.443696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.5058","last_updated":"2008-09-29T20:12:13Z","snapshot_observed_at":"2026-08-04T11:26:57.031645Z","submitted_at":"2008-09-29T20:12:13Z","title":"The Chandra Deep Protocluster Survey: Evidence for an Enhancement in the AGN Activity in the SSA22 Protocluster at z = 3.09","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.5058","snapshot_observed_at":"2026-08-06T23:10:46.701775Z","title":"ApJ 691, 687–695","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.701775Z"},"links":{"cited_paper":"/paper/0809.5058","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c52d091d02e77617651f94fb89a5ed0503b2d9caf97d1303d75d7932f3ccc5da","observation_id":"95b4d849-ccb8-45f8-b361-071b920574b7","resolution":{"observed_at":"2026-08-06T23:10:46.701775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.02441","last_updated":"2018-08-07T16:11:17Z","snapshot_observed_at":"2026-08-06T06:59:24.151674Z","submitted_at":"2018-08-07T16:11:17Z","title":"The z=0.54 LoBAL Quasar SDSS J085053.12+445122.5: I. Spectral Synthesis Analysis Reveals a Massive Outflow","version":1},"cited_work":{"arxiv_id":"1808.02441","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.02441","snapshot_observed_at":"2026-08-06T23:10:52.898945Z","title":"The z=0.54 LoBAL Quasar SDSS J085053.12+445122.5: I. Spectral Synthesis Analysis Reveals a Massive Outflow","venue":"astro-ph.GA","work_id":"6a9ddfc6-df8d-4e57-b5a5-fc5d397462e1","year":2018},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.783114Z"},"links":{"cited_paper":"/paper/1808.02441","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:8034bf4b8effe818e0d5547418b16398705c6f8409d94383f11d5d0d125d85cb","observation_id":"2c1c4f39-b337-4b60-bff2-805e03946661","resolution":{"observed_at":"2026-08-06T23:10:52.905008Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.12330","last_updated":"2024-04-16T23:21:54Z","snapshot_observed_at":"2026-07-06T16:35:19.728025Z","submitted_at":"2023-10-18T21:15:26Z","title":"AGN Selection and Demographics: A New Age with JWST/MIRI","version":2},"cited_work":{"arxiv_id":"2310.12330","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.12330","snapshot_observed_at":"2026-08-06T23:10:52.875146Z","title":"AGN Selection and Demographics: A New Age with JWST/MIRI","venue":"astro-ph.GA","work_id":"56ee0e57-08ce-4b08-8a18-dd9738b50ecb","year":2023},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.852051Z"},"links":{"cited_paper":"/paper/2310.12330","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:5432952b43118307cd0eddaba9ba51284b561a8ee702f5800da57d7212c3c1a0","observation_id":"6d796b67-78f9-4ca2-91f3-cf43b92b2600","resolution":{"observed_at":"2026-08-06T23:10:52.880562Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:10:46.959862Z","title":"Astronomy and Computing 48, 100835","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.959862Z"},"links":{"citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:b6fd3353716b57276be6f687dae418bded9b7d7057e60ef0e03b6e97c26fe1e1","observation_id":"7b504d32-ba44-45f2-a282-ad736eea43f5","resolution":{"observed_at":"2026-08-06T23:10:46.959862Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:10:47.115303Z","title":"Frontiers in Astronomy and Space Sciences 5, 6","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.115303Z"},"links":{"citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a405368fc6032f315844e8733c0b8b37dd3a87519f8d145dcb8cd3876cb64b89","observation_id":"8690bb80-f3f7-4013-900c-8afea7e5d855","resolution":{"observed_at":"2026-08-06T23:10:47.115303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.01567","last_updated":"2018-05-02T08:48:22Z","snapshot_observed_at":"2026-08-05T09:07:31.200297Z","submitted_at":"2018-02-05T18:59:59Z","title":"Intermediate-mass black holes in dwarf galaxies out to redshift $\\sim$ 2.4 in the Chandra COSMOS Legacy Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.01567","snapshot_observed_at":"2026-08-06T23:10:47.393721Z","title":"MNRAS 478, 2576–2591","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.393721Z"},"links":{"cited_paper":"/paper/1802.01567","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:643ea0e96fb32cf5232f958513142e2462bab5edfa35e55fd4441a28d052cf81","observation_id":"741f716c-c6aa-486d-a9a7-0dac27016eff","resolution":{"observed_at":"2026-08-06T23:10:47.393721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.08912","last_updated":"2018-03-02T14:05:43Z","snapshot_observed_at":"2026-07-06T06:25:11.708379Z","submitted_at":"2018-02-24T21:10:35Z","title":"Large Scale Environment of a $z=6.61$ Luminous Quasar Probed by Ly$\\alpha$ Emitters and Lyman Break Galaxies","version":2},"cited_work":{"arxiv_id":"1802.08912","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.08912","snapshot_observed_at":"2026-08-06T23:10:52.395042Z","title":"Large Scale Environment of a $z=6.61$ Luminous Quasar Probed by Ly$\\alpha$ Emitters and Lyman Break Galaxies","venue":"astro-ph.GA","work_id":"d25a1b62-6e0a-4657-aa46-a16bcdb7caac","year":2018},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.967966Z"},"links":{"cited_paper":"/paper/1802.08912","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:04138f87cb07d4b49d0144bf7c10450b0d15ba322dcb037b97f7fe417c8dbb66","observation_id":"4b1a875a-711d-49fa-b922-fc80437ab62f","resolution":{"observed_at":"2026-08-06T23:10:52.400068Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:10:48.034553Z","title":"ApJ 944,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.034553Z"},"links":{"citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:604dd89874e60e945f0bae18568cc66a7427bd4d2f7cc354da6ff363abce7988","observation_id":"14206fd8-8f3a-4ee8-aec0-681fb22ddbea","resolution":{"observed_at":"2026-08-06T23:10:48.034553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.01915","last_updated":"2022-12-04T20:27:33Z","snapshot_observed_at":"2026-07-06T14:26:40.492700Z","submitted_at":"2022-12-04T20:27:33Z","title":"The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques","version":1},"cited_work":{"arxiv_id":"2212.01915","doi":null,"metadata_source":"pith","pith_arxiv_id":"2212.01915","snapshot_observed_at":"2026-08-06T23:10:52.366925Z","title":"The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques","venue":"astro-ph.GA","work_id":"f9dc736f-98bb-49a4-82aa-2005abc995de","year":2022},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.092673Z"},"links":{"cited_paper":"/paper/2212.01915","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:f27c080f0ed2888f4cf0462347ab0cdfae0787364821bc8a2c7341c243b234dd","observation_id":"7a7343de-8188-427b-9450-f9714264b5ad","resolution":{"observed_at":"2026-08-06T23:10:52.371952Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10626","last_updated":"2019-05-10T12:23:21Z","snapshot_observed_at":"2026-07-06T07:35:51.141303Z","submitted_at":"2019-02-27T16:36:29Z","title":"Identifying Galaxy Mergers in Observations and Simulations with Deep Learning","version":3},"cited_work":{"arxiv_id":"1902.10626","doi":null,"metadata_source":"pith","pith_arxiv_id":"1902.10626","snapshot_observed_at":"2026-08-06T23:10:52.322134Z","title":"Identifying Galaxy Mergers in Observations and Simulations with Deep Learning","venue":"astro-ph.GA","work_id":"8d2c31c9-ee33-4849-8487-8eda8e8bacbe","year":2019},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.215205Z"},"links":{"cited_paper":"/paper/1902.10626","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:d5d742981e46d20ea87ed6e964dcd6f10b8d16d4a971cde15e49698c881d08df","observation_id":"1babf66c-4d7d-4544-8f53-403b14e16ed2","resolution":{"observed_at":"2026-08-06T23:10:52.327918Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.05840","last_updated":"2020-12-10T17:31:52Z","snapshot_observed_at":"2026-08-04T17:12:36.904356Z","submitted_at":"2020-12-10T17:31:52Z","title":"Detection of large-scale X-ray bubbles in the Milky Way halo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.05840","snapshot_observed_at":"2026-08-06T23:10:48.276624Z","title":"Nature 588, 227–231","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.276624Z"},"links":{"cited_paper":"/paper/2012.05840","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:aebbefe4e435e71028e2f06ce9bd743396960a421f64c01f4d1f75faa9775f84","observation_id":"1b344bb2-9836-4f98-a96f-eb5f0e85eb6f","resolution":{"observed_at":"2026-08-06T23:10:48.276624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.2368","last_updated":"2011-05-12T04:40:53Z","snapshot_observed_at":"2026-07-06T02:27:37.801656Z","submitted_at":"2011-05-12T04:40:53Z","title":"Torus and AGN properties of nearby Seyfert galaxies: Results from fitting IR spectral energy distributions and spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.2368","snapshot_observed_at":"2026-08-06T23:10:40.992971Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:40.992971Z"},"links":{"cited_paper":"/paper/1105.2368","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:36281e9cbb44d8e572a176c5d16eb48e5846c9ca66964b4e178df99f4308d5fe","observation_id":"62842c71-43cf-4f71-8ffe-09b8a3735124","resolution":{"observed_at":"2026-08-06T23:10:40.992971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00780","last_updated":"2023-11-01T18:48:30Z","snapshot_observed_at":"2026-07-06T16:41:51.334062Z","submitted_at":"2023-11-01T18:48:30Z","title":"Overview of the Advanced X-ray Imaging Satellite (AXIS)","version":1},"cited_work":{"arxiv_id":"2311.00780","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.00780","snapshot_observed_at":"2026-08-06T23:10:52.205149Z","title":"Overview of the Advanced X-ray Imaging Satellite (AXIS)","venue":"astro-ph.IM","work_id":"0425721f-5a22-4fe7-a2e8-83421130421f","year":2023},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.626243Z"},"links":{"cited_paper":"/paper/2311.00780","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:2afcabcef4a829a1a96ec7a32f71a46362bd828d7e19a888256e5a5113088e72","observation_id":"380473e0-b2b5-45a3-bce5-79266cfb7837","resolution":{"observed_at":"2026-08-06T23:10:52.210362Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.00014","last_updated":"2022-08-31T18:00:00Z","snapshot_observed_at":"2026-08-08T10:44:44.313328Z","submitted_at":"2022-08-31T18:00:00Z","title":"BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes","version":1},"cited_work":{"arxiv_id":"2209.00014","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.00014","snapshot_observed_at":"2026-08-06T23:10:52.181340Z","title":"BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes","venue":"astro-ph.GA","work_id":"c64ea6ff-e533-4794-954c-16bebd491970","year":2022},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.656275Z"},"links":{"cited_paper":"/paper/2209.00014","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:fb6c8de8c783725015cb8e4d0e04d00ac1875eb7984f679d9172b01d08e27481","observation_id":"951dae26-7901-4ae5-9df8-c226d6900843","resolution":{"observed_at":"2026-08-06T23:10:52.186304Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.01479","last_updated":"2018-11-27T11:38:39Z","snapshot_observed_at":"2026-07-06T06:37:16.373053Z","submitted_at":"2018-05-03T18:00:04Z","title":"The abundances and properties of Dual AGN and their host galaxies in the EAGLE simulations","version":2},"cited_work":{"arxiv_id":"1805.01479","doi":null,"metadata_source":"pith","pith_arxiv_id":"1805.01479","snapshot_observed_at":"2026-08-06T23:10:52.157351Z","title":"The abundances and properties of Dual AGN and their host galaxies in the EAGLE simulations","venue":"astro-ph.GA","work_id":"8672fd89-8a51-429a-b606-be641a24ad77","year":2018},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.800003Z"},"links":{"cited_paper":"/paper/1805.01479","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:7e61f6c8b0ce98634f8bc4e5b3ceee312b75ebb8a188cc1e0232ee589b8447c3","observation_id":"0d586eaa-c577-44da-b624-22168de8ac6b","resolution":{"observed_at":"2026-08-06T23:10:52.164418Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.05528","last_updated":"2018-11-19T20:36:08Z","snapshot_observed_at":"2026-08-07T12:16:29.115504Z","submitted_at":"2018-11-13T20:59:51Z","title":"The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched on","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.05528","snapshot_observed_at":"2026-08-06T23:10:48.918055Z","title":"The most massive galaxies are always switched on","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.918055Z"},"links":{"cited_paper":"/paper/1811.05528","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:efce5161c648556d9bfa2b7d2024683e3d372e402e726b48cbfb56d59209e017","observation_id":"b095d296-e047-41c6-bc65-246055a47495","resolution":{"observed_at":"2026-08-06T23:10:48.918055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.12504","last_updated":"2023-08-16T17:49:28Z","snapshot_observed_at":"2026-07-06T15:30:18.137347Z","submitted_at":"2023-05-21T16:47:52Z","title":"Are we surprised to find SMBHs with JWST at z > 9?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.12504","snapshot_observed_at":"2026-08-06T23:10:49.229451Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:49.229451Z"},"links":{"cited_paper":"/paper/2305.12504","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:9bac929f36c967b499552dc0f30cff6d2b074fac9b732e943e603b0e5416bbe8","observation_id":"658e3e57-1646-4770-8302-46612d9def1a","resolution":{"observed_at":"2026-08-06T23:10:49.229451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.18731","last_updated":"2025-02-18T15:23:38Z","snapshot_observed_at":"2026-07-06T16:55:09.267685Z","submitted_at":"2023-11-30T17:27:08Z","title":"JADES: A large population of obscured, narrow line AGN at high redshift","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.18731","snapshot_observed_at":"2026-08-06T23:10:49.430949Z","title":"arXiv e-prints , arXiv:2311.18731doi: 10.48550/arXiv.2311","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:49.430949Z"},"links":{"cited_paper":"/paper/2311.18731","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:99b806194f81350a6da089c6eed0835b61bfdbdae7000de4e212d3cda27d99ec","observation_id":"52d26770-2086-48d9-bc65-bc3fc32dad27","resolution":{"observed_at":"2026-08-06T23:10:49.430949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.4368","last_updated":"2012-02-04T02:36:38Z","snapshot_observed_at":"2026-08-09T08:56:39.967929Z","submitted_at":"2011-07-21T20:00:40Z","title":"PRIMUS: The dependence of AGN accretion on host stellar mass and color","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.4368","snapshot_observed_at":"2026-08-06T23:10:40.845829Z","title":"little red dots","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:40.845829Z"},"links":{"cited_paper":"/paper/1107.4368","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:8726645778bd8d55fca278e565ba20388bb024e34ba7844fd8a0d65f1dcf6e02","observation_id":"af5657b4-99da-40a9-afe5-a8889e230463","resolution":{"observed_at":"2026-08-06T23:10:40.845829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.5433","last_updated":"2015-01-07T11:10:43Z","snapshot_observed_at":"2026-07-06T03:54:57.456461Z","submitted_at":"2014-09-18T20:00:04Z","title":"The Herschel view of the dominant mode of galaxy growth from z=4 to the present day","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.5433","snapshot_observed_at":"2026-08-06T23:10:49.636531Z","title":"A&A 575, A74","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:49.636531Z"},"links":{"cited_paper":"/paper/1409.5433","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:3a53b0ad7bc40fff618a0993e9fea9c7a99208b5a956f729b356a9d780fe29c7","observation_id":"05f8ec96-8dd7-4431-95a3-62a99c0990f9","resolution":{"observed_at":"2026-08-06T23:10:49.636531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.05653","last_updated":"2016-06-07T08:14:20Z","snapshot_observed_at":"2026-07-06T04:49:53.074843Z","submitted_at":"2016-03-17T20:00:01Z","title":"The origin of the $\\alpha$-enhancement of massive galaxies","version":3},"cited_work":{"arxiv_id":"1603.05653","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.05653","snapshot_observed_at":"2026-08-06T23:10:52.076561Z","title":"The origin of the $\\alpha$-enhancement of massive galaxies","venue":"astro-ph.GA","work_id":"f32206ba-fb81-425c-9f69-c4a7c03bb0ec","year":2016},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:49.811206Z"},"links":{"cited_paper":"/paper/1603.05653","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:d801f49096929dc911d7e44280aa49efa898e0b1d4613c056cd29f9d6d842b58","observation_id":"34b7ba41-a555-4c99-9cc5-707c67f07e08","resolution":{"observed_at":"2026-08-06T23:10:52.081726Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1207.4190","last_updated":"2012-12-05T13:57:52Z","snapshot_observed_at":"2026-07-30T22:19:18.323826Z","submitted_at":"2012-07-17T20:00:03Z","title":"Galaxy Zoo: Bulgeless Galaxies With Growing Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.4190","snapshot_observed_at":"2026-08-06T23:10:50.210272Z","title":"MNRAS 429, 2199–2211","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:50.210272Z"},"links":{"cited_paper":"/paper/1207.4190","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:23fd9fa0bfb1d445ceb17b64f049472b52ad53d6cfe563f182159b090d4319b2","observation_id":"c3a3a59e-ac77-4b59-9474-a00bdd3d5872","resolution":{"observed_at":"2026-08-06T23:10:50.210272Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.07482","last_updated":"2021-03-12T19:00:06Z","snapshot_observed_at":"2026-08-08T13:15:09.837010Z","submitted_at":"2021-03-12T19:00:06Z","title":"Resolving the Hot Dust Disk of ESO323-G77","version":1},"cited_work":{"arxiv_id":"2103.07482","doi":null,"metadata_source":"pith","pith_arxiv_id":"2103.07482","snapshot_observed_at":"2026-08-06T23:10:52.939717Z","title":"Resolving the Hot Dust Disk of ESO323-G77","venue":"astro-ph.GA","work_id":"02263dc4-a3cb-484b-bf5a-8bddd3628518","year":2021},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.566388Z"},"links":{"cited_paper":"/paper/2103.07482","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:65229af788d7918dd9ea4d5d0b66abda9acddb23364a5a09eff9ed001ec9701f","observation_id":"4ebe02cc-3d90-4c9a-a93c-1b7a47a8470e","resolution":{"observed_at":"2026-08-06T23:10:52.944905Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.15275","last_updated":"2022-04-22T11:30:15Z","snapshot_observed_at":"2026-08-09T16:48:30.802082Z","submitted_at":"2021-12-31T03:28:45Z","title":"Learned Coarse Models for Efficient Turbulence Simulation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.15275","snapshot_observed_at":"2026-08-06T23:10:50.641596Z","title":"arXiv e-prints , arXiv:2112.15275doi: 10.48550/arXiv.2112.15275, arXiv:2112.15275","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:50.641596Z"},"links":{"cited_paper":"/paper/2112.15275","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:651d3ce57d863026a1d1a2624615ef0ffea6e5cd59fbd90ad0ed8ba338bdfd77","observation_id":"4e8aabff-8c94-4437-8dcb-72fe36e9b132","resolution":{"observed_at":"2026-08-06T23:10:50.641596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.06772","last_updated":"2025-05-14T16:36:49Z","snapshot_observed_at":"2026-08-07T03:47:53.461409Z","submitted_at":"2024-09-10T18:00:00Z","title":"Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.06772","snapshot_observed_at":"2026-08-06T23:10:51.108699Z","title":"arXiv e-prints , arXiv:2409.06772doi:10","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.108699Z"},"links":{"cited_paper":"/paper/2409.06772","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:d1e960df247e66490d66b015e8ea372558a174bef4eddeac2c7464df0b5c48b7","observation_id":"17df7b74-8f18-4e7b-bb84-aa56c7df9726","resolution":{"observed_at":"2026-08-06T23:10:51.108699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.00010","last_updated":"2017-02-06T01:28:12Z","snapshot_observed_at":"2026-08-01T14:51:16.228932Z","submitted_at":"2016-11-30T21:00:00Z","title":"ALMA Observations Show Major Mergers Among the Host Galaxies of Fast-growing, High-redshift Supermassive Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.00010","snapshot_observed_at":"2026-08-06T23:10:51.221503Z","title":"ApJ 836, 8","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.221503Z"},"links":{"cited_paper":"/paper/1612.00010","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:102449378864aac4a0069b028f984e61eb3f34f2a24e1a3723c32f31a9469cd9","observation_id":"3416fed5-9ab2-48f0-8d3e-85ebdc9767d6","resolution":{"observed_at":"2026-08-06T23:10:51.221503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.04118","last_updated":"2015-01-16T21:34:35Z","snapshot_observed_at":"2026-08-05T06:29:45.742825Z","submitted_at":"2015-01-16T21:34:35Z","title":"The Spitzer mid-infrared AGN survey. II-the demographics and cosmic evolution of the AGN population","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.04118","snapshot_observed_at":"2026-08-06T23:10:46.200913Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:46.200913Z"},"links":{"cited_paper":"/paper/1501.04118","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:87fae566042b478694c0756be78edf44ab30a1765e0de4f9f8a3d510ed273a5e","observation_id":"c41cc521-333f-4074-8592-cbc7b41b65f2","resolution":{"observed_at":"2026-08-06T23:10:46.200913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.03589","last_updated":"2024-08-22T10:09:55Z","snapshot_observed_at":"2026-07-06T16:57:46.724781Z","submitted_at":"2023-12-06T16:29:25Z","title":"GA-NIFS: JWST discovers an offset AGN 740 million years after the Big Bang","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.03589","snapshot_observed_at":"2026-08-06T23:10:51.316501Z","title":"arXiv e-prints , arXiv:2312.03589doi: 10.48550/arXiv.2312","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.316501Z"},"links":{"cited_paper":"/paper/2312.03589","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:7336ea8f39d08a4797faede78e591e811c9dad70a8af4665d9a8bdb59bd50e39","observation_id":"845602cb-b093-4214-b2a2-2a845cd01156","resolution":{"observed_at":"2026-08-06T23:10:51.316501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.4857","last_updated":"2009-04-24T16:31:28Z","snapshot_observed_at":"2026-07-06T01:52:37.715652Z","submitted_at":"2009-03-27T17:18:44Z","title":"On the Size and Comoving Mass Density Evolution of Early-Type Galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.4857","snapshot_observed_at":"2026-08-06T23:10:51.411458Z","title":"ApJ 698, 1232–1243","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.411458Z"},"links":{"cited_paper":"/paper/0903.4857","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:92f6087083e38d98ba4568cfdb7cc669ba7f913471f86414c85e11f50b163569","observation_id":"3df6a911-7ae4-4636-b89e-6d9887860e8e","resolution":{"observed_at":"2026-08-06T23:10:51.411458Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.06236","last_updated":"2016-11-22T11:37:41Z","snapshot_observed_at":"2026-08-01T15:59:19.503139Z","submitted_at":"2016-11-18T21:00:07Z","title":"Host galaxies of luminous z$\\sim$0.6 quasars: Major mergers are not prevalent at the highest AGN luminosities","version":2},"cited_work":{"arxiv_id":"1611.06236","doi":null,"metadata_source":"pith","pith_arxiv_id":"1611.06236","snapshot_observed_at":"2026-08-06T23:10:51.832676Z","title":"Host galaxies of luminous z$\\sim$0.6 quasars: Major mergers are not prevalent at the highest AGN luminosities","venue":"astro-ph.GA","work_id":"fdbdab95-5fec-487e-bb43-661a339ad208","year":2016},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.417251Z"},"links":{"cited_paper":"/paper/1611.06236","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:ea68cc84b5e708242fd5512c8b342c325406f860aed053098c6b2baf06d88ea4","observation_id":"f3bd9bb0-7882-4e8a-ac12-48ada075b23e","resolution":{"observed_at":"2026-08-06T23:10:51.837951Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.07563","last_updated":"2019-01-22T19:00:00Z","snapshot_observed_at":"2026-08-01T18:26:11.386804Z","submitted_at":"2019-01-22T19:00:00Z","title":"Formation of massive black holes in rapidly growing pre-galactic gas clouds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.07563","snapshot_observed_at":"2026-08-06T23:10:51.434358Z","title":"Nature 566, 85–88","venue":null,"work_id":null,"year":1901},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.434358Z"},"links":{"cited_paper":"/paper/1901.07563","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:39ce172ec5a8366845d5e4244795f0b2fdc3a6c90762696ca9e37e768b50dc52","observation_id":"4fcae6a7-de0f-4f71-b04c-2c79aa5302e2","resolution":{"observed_at":"2026-08-06T23:10:51.434358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02710","last_updated":"2016-03-08T21:28:06Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:28:06Z","title":"The subarcsecond mid-infrared view of local active galactic nuclei: III. Polar dust emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02710","snapshot_observed_at":"2026-08-06T23:10:41.168514Z","title":"Assef, R.J., Eisenhardt, P.R.M., Stern, D., Tsai, C.W., Wu, J., Wylezalek, D., Blain, A.W., Bridge, C.R., Donoso, E., Gonzales, A., Gri ffith, R.L., Jarrett, T.H., 2015","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":109,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.168514Z"},"links":{"cited_paper":"/paper/1603.02710","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c8632b99cfa8ad0b078be4b6c00fb3ec6d2236c7af22a504224612e6df02e69f","observation_id":"8c3273ee-55b2-40d6-a155-b7334e98f8e3","resolution":{"observed_at":"2026-08-06T23:10:41.168514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.06888","last_updated":"2017-12-06T08:17:16Z","snapshot_observed_at":"2026-07-06T05:34:27.624728Z","submitted_at":"2017-03-20T18:00:04Z","title":"Eddington-Limited Accretion in z~2 WISE-selected Hot, Dust-Obscured Galaxies","version":2},"cited_work":{"arxiv_id":"1703.06888","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.06888","snapshot_observed_at":"2026-08-06T23:10:51.757608Z","title":"Eddington-Limited Accretion in z~2 WISE-selected Hot, Dust-Obscured Galaxies","venue":"astro-ph.GA","work_id":"5aa7e005-a19c-4ea9-b32d-f285abe8c60d","year":2017},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.440143Z"},"links":{"cited_paper":"/paper/1703.06888","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:53f07fedabd0cf44315c6a2b141f668c3241d224d4ac092936f8bde0ff213ba0","observation_id":"b7888993-c8b8-4145-a378-a98eaec5d006","resolution":{"observed_at":"2026-08-06T23:10:51.762537Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.07345","last_updated":"2019-09-09T07:38:56Z","snapshot_observed_at":"2026-07-06T07:46:17.829799Z","submitted_at":"2019-04-15T22:05:28Z","title":"Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) VIII. A less biased view of the early co-evolution of black holes and host galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.07345","snapshot_observed_at":"2026-08-06T23:10:45.037421Z","title":"Jacomy, M., Venturini, T., Heymann, S., Bastian, M., 2014","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.037421Z"},"links":{"cited_paper":"/paper/1904.07345","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a0aca72b04ba21f124d619383ebcf067e4417b934008650645e279f0133aa317","observation_id":"62b585e7-d4d6-4b4b-8705-7687bd9c08a1","resolution":{"observed_at":"2026-08-06T23:10:45.037421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5518","last_updated":"2012-08-27T22:03:21Z","snapshot_observed_at":"2026-08-06T05:01:34.397738Z","submitted_at":"2012-08-27T22:03:21Z","title":"Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.5518","snapshot_observed_at":"2026-08-06T23:10:51.445344Z","title":"Wylezalek, D., Morganti, R., 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.445344Z"},"links":{"cited_paper":"/paper/1208.5518","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:1e904979569c14d6e90287d3d75a7d320bb2fcbb19489aec15b11e2b9e1691f8","observation_id":"47fbf03a-9be6-4339-8239-7c89fb2da502","resolution":{"observed_at":"2026-08-06T23:10:51.445344Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.04888","last_updated":"2019-03-11T06:11:11Z","snapshot_observed_at":"2026-08-04T07:38:17.280834Z","submitted_at":"2018-10-11T08:16:52Z","title":"Black Hole Mass Scaling Relations for Spiral Galaxies. II. $M_{\\rm BH}$-$M_{\\rm *,tot}$ and $M_{\\rm BH}$-$M_{\\rm *,disk}$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.04888","snapshot_observed_at":"2026-08-06T23:10:42.739695Z","title":"Davis, S.W., Tchekhovskoy, A., 2020","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.739695Z"},"links":{"cited_paper":"/paper/1810.04888","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:e6e7f086b8b80187f1e26051f9b7400ae30beb4503b7d6ef20802cf3f487cd93","observation_id":"a0b1d836-08fc-4c31-8e5b-ff0295ed8cf5","resolution":{"observed_at":"2026-08-06T23:10:42.739695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.02642","last_updated":"2016-03-23T18:28:21Z","snapshot_observed_at":"2026-07-06T04:39:13.626957Z","submitted_at":"2015-12-08T21:00:05Z","title":"Discovery of extreme [OIII]5007A outflows in high-redshift red quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.02642","snapshot_observed_at":"2026-08-06T23:10:51.463958Z","title":"MNRAS 459, 3144–3160","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.463958Z"},"links":{"cited_paper":"/paper/1512.02642","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:d29e048cb3f55975b05e3e46b0caf7a42a2ee37de86aea4b0512b09a33da43a1","observation_id":"4692b891-5666-4554-913c-a58f958603a3","resolution":{"observed_at":"2026-08-06T23:10:51.463958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511734","last_updated":"2005-11-25T21:14:20Z","snapshot_observed_at":"2026-07-07T00:56:19.361558Z","submitted_at":"2005-11-25T21:14:20Z","title":"An Overdensity of Galaxies near the Most Distant Radio-Loud Quasar","version":1},"cited_work":{"arxiv_id":"astro-ph/0511734","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0511734","snapshot_observed_at":"2026-08-06T23:10:51.652791Z","title":"An Overdensity of Galaxies near the Most Distant Radio-Loud Quasar","venue":"astro-ph","work_id":"7586e28c-f208-431e-a607-91d6dfc741ef","year":2005},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.469444Z"},"links":{"cited_paper":"/paper/astro-ph/0511734","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:23b50b200cf8cafbce1a951820fa3b0a78db2229bdb40a51ca3a8bb9fa76c90f","observation_id":"26fa5348-398d-4400-be04-4bfc68668121","resolution":{"observed_at":"2026-08-06T23:10:51.661331Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.09720","last_updated":"2022-01-24T14:51:52Z","snapshot_observed_at":"2026-07-06T12:30:41.307938Z","submitted_at":"2022-01-24T14:51:52Z","title":"Constraining galaxy overdensities around three z~6.5 quasars with ALMA and MUSE","version":1},"cited_work":{"arxiv_id":"2201.09720","doi":null,"metadata_source":"pith","pith_arxiv_id":"2201.09720","snapshot_observed_at":"2026-08-06T23:10:52.692241Z","title":"Constraining galaxy overdensities around three z~6.5 quasars with ALMA and MUSE","venue":"astro-ph.GA","work_id":"fd6f1f61-bdef-4934-99bf-59763bb623e8","year":2022},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":141,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.237376Z"},"links":{"cited_paper":"/paper/2201.09720","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:960792e7eadc681b32b743e7b84d7736e9c4cd1b24c8c91d081fe5d1a18f5680","observation_id":"14821449-21a9-44f0-98ef-e678ec04b13a","resolution":{"observed_at":"2026-08-06T23:10:52.698093Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.06800","last_updated":"2015-03-23T20:00:31Z","snapshot_observed_at":"2026-08-08T20:51:49.097250Z","submitted_at":"2015-03-23T20:00:31Z","title":"The Launching of Cold Clouds by Galaxy Outflows I: Hydrodynamic Interactions with Radiative Cooling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.06800","snapshot_observed_at":"2026-08-06T23:10:49.078345Z","title":"Scannapieco, E., Oh, S.P., 2004","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:49.078345Z"},"links":{"cited_paper":"/paper/1503.06800","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:ae56cf5cdd9bfd4aeb3c09948713f999e6b87ecbd623aa50504ad1bb5371d1c9","observation_id":"6c2e7c11-71c4-44d2-a21b-137019384348","resolution":{"observed_at":"2026-08-06T23:10:49.078345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01672","last_updated":"2021-12-15T05:51:58Z","snapshot_observed_at":"2026-08-09T08:25:29.089695Z","submitted_at":"2021-08-03T18:00:00Z","title":"Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Hubble Space Telescope Discovers Double Quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01672","snapshot_observed_at":"2026-08-06T23:10:42.289560Z","title":"Chevallard, J., Charlot, S., 2016","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":162,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.289560Z"},"links":{"cited_paper":"/paper/2108.01672","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:264d8ac6a00027cb3fc5ef5e8dd286a2006d5315e1e404d9402705739117991c","observation_id":"4498bcab-1e9e-4cdd-a20a-1bc3bb0b9e2c","resolution":{"observed_at":"2026-08-06T23:10:42.289560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0605323","last_updated":"2006-07-20T20:44:48Z","snapshot_observed_at":"2026-07-07T01:00:19.847129Z","submitted_at":"2006-05-12T17:39:35Z","title":"The Feedback-Regulated Growth of Black Holes and Bulges through Gas Accretion and Starbursts in Cluster Central Dominant Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0605323","snapshot_observed_at":"2026-08-06T23:10:48.322068Z","title":"Rakshit, S., Stalin, C.S., Kotilainen, J., 2020","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":231,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.322068Z"},"links":{"cited_paper":"/paper/astro-ph/0605323","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:4e68a7875bc2e6a8d32950ed325758d7eef2b1f570f0987adfd663d774c781f5","observation_id":"4f6b4a2d-618e-4933-844f-0e2ff30d22b3","resolution":{"observed_at":"2026-08-06T23:10:48.322068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.1453","last_updated":"2010-07-08T20:00:00Z","snapshot_observed_at":"2026-08-08T07:57:36.495608Z","submitted_at":"2010-07-08T20:00:00Z","title":"Color-Magnitude Relations of Active and Non-Active Galaxies in the Chandra Deep Fields: High-Redshift Constraints and Stellar-Mass Selection Effects","version":1},"cited_work":{"arxiv_id":"1007.1453","doi":null,"metadata_source":"pith","pith_arxiv_id":"1007.1453","snapshot_observed_at":"2026-08-06T23:10:51.717795Z","title":"Color-Magnitude Relations of Active and Non-Active Galaxies in the Chandra Deep Fields: High-Redshift Constraints and Stellar-Mass Selection Effects","venue":"astro-ph.CO","work_id":"6a84dab6-49ca-4357-adf5-dfd99493a359","year":2010},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":391,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.451980Z"},"links":{"cited_paper":"/paper/1007.1453","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:6adff8c57c7ae47de1776a0fee35de564fd5b8067c038cd3827b02ea19f99702","observation_id":"f4de7387-9c33-4e79-94a2-a81b62d1c0af","resolution":{"observed_at":"2026-08-06T23:10:51.722884Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.6365","last_updated":"2014-06-24T20:00:17Z","snapshot_observed_at":"2026-07-06T03:47:11.838220Z","submitted_at":"2014-06-24T20:00:17Z","title":"A close-pair binary in a distant triple supermassive black-hole system","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.6365","snapshot_observed_at":"2026-08-06T23:10:42.915086Z","title":"Deane, R.P., Paragi, Z., Jarvis, M.J., Coriat, M., Bernardi, G., Fender, R.P., Frey, S., Heywood, I., Kl ¨ockner, H.R., Grainge, K., Rumsey, C., 2014","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":515,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.915086Z"},"links":{"cited_paper":"/paper/1406.6365","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:e234686d4a70ce6cb315d038aabb82d0f3ff81c2cc992b4619cf13aa3e812385","observation_id":"23099d65-d498-4ced-8288-f798910b62bc","resolution":{"observed_at":"2026-08-06T23:10:42.915086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0203468","last_updated":"2002-03-26T20:40:48Z","snapshot_observed_at":"2026-07-07T00:25:42.537283Z","submitted_at":"2002-03-26T20:40:48Z","title":"The slope of the black-hole mass versus velocity dispersion correlation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0203468","snapshot_observed_at":"2026-08-06T23:10:51.235976Z","title":"Tremmel, M., Karcher, M., Governato, F., V olonteri, M., Quinn, T.R., Pontzen, A., Anderson, L., Bellovary, J., 2017","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":753,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.235976Z"},"links":{"cited_paper":"/paper/astro-ph/0203468","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:0c1353f557e11f260329bc5419e04c36d44b4f3d0a16718414c897c0667405d1","observation_id":"f4d0f1c5-9c24-4797-9234-1edb0efedece","resolution":{"observed_at":"2026-08-06T23:10:51.235976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.15240","last_updated":"2024-02-23T10:08:22Z","snapshot_observed_at":"2026-08-05T01:54:09.091349Z","submitted_at":"2024-02-23T10:08:22Z","title":"AGN feedback in isolated galaxies with a SMUGGLE multiphase ISM","version":1},"cited_work":{"arxiv_id":"2402.15240","doi":null,"metadata_source":"pith","pith_arxiv_id":"2402.15240","snapshot_observed_at":"2026-08-06T23:10:51.997096Z","title":"AGN feedback in isolated galaxies with a SMUGGLE multiphase ISM","venue":"astro-ph.GA","work_id":"360cfab4-fc6f-45a8-8a9f-c993b2ad118e","year":2024},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":830,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:50.352351Z"},"links":{"cited_paper":"/paper/2402.15240","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:638b49622c558142b2418093cf6d344ce5f7b2eaaf469677d125f664c82659ad","observation_id":"88765484-9ae2-4aac-a4a4-3d0b126347b0","resolution":{"observed_at":"2026-08-06T23:10:52.002297Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4121","last_updated":"2009-04-26T21:08:41Z","snapshot_observed_at":"2026-07-06T01:53:49.504505Z","submitted_at":"2009-01-27T05:06:43Z","title":"Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.4121","snapshot_observed_at":"2026-08-06T23:10:44.802479Z","title":"Hickox, R.C., Mullaney, J.R., Alexander, D.M., Chen, C.T.J., Civano, F.M., Goulding, A.D., Hainline, K.N., 2014","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":919,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.802479Z"},"links":{"cited_paper":"/paper/0901.4121","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:074b36d4bc6229c76427ee8d99306d91ebcb447974d6f8bfe20ae96abf0d76f5","observation_id":"f7d4fd5e-d6c6-4b36-b113-30379da0da09","resolution":{"observed_at":"2026-08-06T23:10:44.802479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.08870","last_updated":"2024-09-12T09:30:57Z","snapshot_observed_at":"2026-07-06T18:14:20.889736Z","submitted_at":"2024-05-14T18:00:02Z","title":"A calibrated model for N-body dynamical friction acting on supermassive black holes","version":2},"cited_work":{"arxiv_id":"2405.08870","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.08870","snapshot_observed_at":"2026-08-06T23:10:53.430894Z","title":"A calibrated model for N-body dynamical friction acting on supermassive black holes","venue":"astro-ph.GA","work_id":"28ea9d3b-3d44-4566-b670-2f43c7f24dba","year":2024},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":977,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.904654Z"},"links":{"cited_paper":"/paper/2405.08870","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:bd92b523f3f14c2a6176a5c2585245811cc224cd253da44cf6a14085d63d1231","observation_id":"05a131eb-449a-4939-95ab-53aafe7e868d","resolution":{"observed_at":"2026-08-06T23:10:53.437233Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.7020","last_updated":"2015-01-14T20:45:38Z","snapshot_observed_at":"2026-07-06T03:47:23.645783Z","submitted_at":"2014-06-26T20:13:42Z","title":"Direct collapse black hole formation from synchronized pairs of atomic cooling halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.7020","snapshot_observed_at":"2026-08-06T23:10:51.423156Z","title":"Vito, F., Brandt, W.N., Comastri, A., Gilli, R., Ivison, R.J., Lanzuisi, G., Lehmer, B.D., Lopez, I.E., Tozzi, P., Vignali, C., 2024","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1063,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.423156Z"},"links":{"cited_paper":"/paper/1406.7020","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:ba4851b0b0155d5dbfe552264ba0e9300791b51239a1bbf253b366588d3c2c17","observation_id":"30f8cb23-cc3a-4199-8f4f-34763ea56e4b","resolution":{"observed_at":"2026-08-06T23:10:51.423156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.0477","last_updated":"2012-12-18T15:28:47Z","snapshot_observed_at":"2026-07-06T02:54:53.278834Z","submitted_at":"2012-09-03T20:11:27Z","title":"The Demographics of Broad Line Quasars in the Mass-Luminosity Plane II. Black Hole Mass and Eddington Ratio Functions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.0477","snapshot_observed_at":"2026-08-06T23:10:45.483861Z","title":"97 Kelly, B.C., Shen, Y ., 2013","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1195,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:45.483861Z"},"links":{"cited_paper":"/paper/1209.0477","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:527e509f8ba53d19a704a10d0043ca30582bafb9e207e0b5a1e4dfab9f911238","observation_id":"90270bd4-47c8-4d08-9843-4b996ced889a","resolution":{"observed_at":"2026-08-06T23:10:45.483861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.11535","last_updated":"2019-12-13T13:35:37Z","snapshot_observed_at":"2026-08-03T17:48:43.714675Z","submitted_at":"2018-10-26T21:26:12Z","title":"The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN","version":2},"cited_work":{"arxiv_id":"1810.11535","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.11535","snapshot_observed_at":"2026-08-06T23:10:53.284906Z","title":"The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN","venue":"astro-ph.GA","work_id":"98abc703-9322-4a36-a63c-19b47dbfc36f","year":2018},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1229,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.525516Z"},"links":{"cited_paper":"/paper/1810.11535","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:cedcf9485dff3bb10d9e87a5727bc00589ef91de609f2e6b1d48d820bc84e4a1","observation_id":"ff730035-e6cc-4a85-a144-3a30d5a84e37","resolution":{"observed_at":"2026-08-06T23:10:53.290176Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05053","last_updated":"2023-06-19T08:06:04Z","snapshot_observed_at":"2026-08-06T18:50:19.756933Z","submitted_at":"2023-05-08T21:16:07Z","title":"XQR-30: the ultimate XSHOOTER quasar sample at the reionization epoch","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05053","snapshot_observed_at":"2026-08-06T23:10:43.011147Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1420,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.011147Z"},"links":{"cited_paper":"/paper/2305.05053","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:29394eac531e5444bc02d4270ecebd2f0df221ee0c7c92e9f220e5b325417b8a","observation_id":"0a79db73-2730-4816-afc5-7822750c20cb","resolution":{"observed_at":"2026-08-06T23:10:43.011147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.03686","last_updated":"2018-10-23T20:15:46Z","snapshot_observed_at":"2026-07-06T07:06:49.418477Z","submitted_at":"2018-10-08T20:13:35Z","title":"On the structure and energetics of quasar broad absorption-line outflows","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.03686","snapshot_observed_at":"2026-08-06T23:10:44.712687Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1828,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.712687Z"},"links":{"cited_paper":"/paper/1810.03686","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:09feb219ec1a4770919f69fafefc043398438c68e0e9e466e9cfacd3e6b138de","observation_id":"beefdf0a-f048-4ada-846c-2ab6c814f777","resolution":{"observed_at":"2026-08-06T23:10:44.712687Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09223","last_updated":"2017-03-27T18:00:00Z","snapshot_observed_at":"2026-07-06T05:35:22.518259Z","submitted_at":"2017-03-27T18:00:00Z","title":"Simulating the interaction of jets with the intra-cluster medium","version":1},"cited_work":{"arxiv_id":"1703.09223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.09223","snapshot_observed_at":"2026-08-06T23:10:51.796054Z","title":"Simulating the interaction of jets with the intra-cluster medium","venue":"astro-ph.GA","work_id":"a50aac6a-a565-4610-bd91-4c68145d588e","year":2017},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":1995,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:51.429200Z"},"links":{"cited_paper":"/paper/1703.09223","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:4c96f57e2d4c79e1126bd4ae57783b2712d77a140f26427737837723d7e8be8f","observation_id":"2546171b-ef0f-4948-8c7e-5184ab4aec1d","resolution":{"observed_at":"2026-08-06T23:10:51.800884Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1705.01133","last_updated":"2017-05-02T18:30:03Z","snapshot_observed_at":"2026-07-06T05:40:33.281941Z","submitted_at":"2017-05-02T18:30:03Z","title":"Observational constraints on the specific accretion-rate distribution of X-ray selected AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.01133","snapshot_observed_at":"2026-08-06T23:10:43.984451Z","title":"Georgakakis, A., Ruiz, A., LaMassa, S.M., 2020","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2001,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.984451Z"},"links":{"cited_paper":"/paper/1705.01133","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:1560056020d4df7ad13a0beb77bb14546f0f4955cc31ec266b75e24a94540414","observation_id":"13b8e98d-3a70-4daa-8e2a-d951fdc1b035","resolution":{"observed_at":"2026-08-06T23:10:43.984451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0402348","last_updated":"2004-04-30T18:31:24Z","snapshot_observed_at":"2026-08-02T18:39:15.769182Z","submitted_at":"2004-02-13T21:55:56Z","title":"A Systematic Study of Radio-Induced X-ray Cavities in Clusters, Groups, and Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0402348","snapshot_observed_at":"2026-08-06T23:10:42.061508Z","title":"ApJ 607, 800–809","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2004,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.061508Z"},"links":{"cited_paper":"/paper/astro-ph/0402348","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:a8ae485726ce0a9ea38b49b188e295d5821663e16981e49b7e57aef5be5633d5","observation_id":"368e4d9e-7960-4db9-b303-5aa2ac4c82ac","resolution":{"observed_at":"2026-08-06T23:10:42.061508Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507410","last_updated":"2005-07-18T14:37:43Z","snapshot_observed_at":"2026-07-07T00:52:20.873493Z","submitted_at":"2005-07-18T14:37:43Z","title":"The Burst Alert Telescope (BAT) on the Swift MIDEX Mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507410","snapshot_observed_at":"2026-08-06T23:10:41.897976Z","title":"Space Sci","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2005,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.897976Z"},"links":{"cited_paper":"/paper/astro-ph/0507410","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:7b2778625fd51c60358c03d7d54a01dd9680f2487b3fe3cd21331740d7c1ce6d","observation_id":"5d8bc4f5-1774-4c73-a346-c6220d384c63","resolution":{"observed_at":"2026-08-06T23:10:41.897976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510371","last_updated":"2005-10-24T16:25:29Z","snapshot_observed_at":"2026-07-07T00:54:59.347704Z","submitted_at":"2005-10-12T20:29:34Z","title":"First Measurement of the Clustering Evolution of Photometrically-Classified Quasars","version":2},"cited_work":{"arxiv_id":"astro-ph/0510371","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0510371","snapshot_observed_at":"2026-08-06T23:10:52.491073Z","title":"First Measurement of the Clustering Evolution of Photometrically-Classified Quasars","venue":"astro-ph","work_id":"03464f32-e265-4a72-b858-19132211122b","year":2005},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2006,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.685274Z"},"links":{"cited_paper":"/paper/astro-ph/0510371","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:03baca043400c2f78db7376593e6ec5343113e12a6f0338331a49a15931a5528","observation_id":"2a2f43bb-f980-443e-8807-55fab9241e9d","resolution":{"observed_at":"2026-08-06T23:10:52.496192Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0607270","last_updated":"2006-07-12T20:03:23Z","snapshot_observed_at":"2026-08-08T22:07:14.256752Z","submitted_at":"2006-07-12T20:03:23Z","title":"AEGIS: The color-magnitude relation for X-ray selected AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0607270","snapshot_observed_at":"2026-08-06T23:10:47.763566Z","title":"ApJ 660, L11–L14","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2007,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:47.763566Z"},"links":{"cited_paper":"/paper/astro-ph/0607270","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:1d53cf1c638db9692b3e552002467f0e1f9e4aa9ed0cb4f2cba05a4ecdbf6ced","observation_id":"352c7785-c5f4-4879-b9a8-320f1192ede7","resolution":{"observed_at":"2026-08-06T23:10:47.763566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608259","last_updated":"2008-06-17T01:58:08Z","snapshot_observed_at":"2026-07-07T01:02:16.639888Z","submitted_at":"2006-08-11T20:36:44Z","title":"Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0608259","snapshot_observed_at":"2026-08-06T23:10:43.645762Z","title":"ApJS 179, 360–422","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2008,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.645762Z"},"links":{"cited_paper":"/paper/astro-ph/0608259","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:872fd76fe3a03783e892ba0f6484018091bf7073f25abec4e650c346cdc7c8db","observation_id":"5d598874-9327-42c0-a20e-703cf3dacb70","resolution":{"observed_at":"2026-08-06T23:10:43.645762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.2747","last_updated":"2008-10-15T17:23:50Z","snapshot_observed_at":"2026-08-04T21:05:42.367690Z","submitted_at":"2008-10-15T17:23:50Z","title":"A Catalog of Broad Absorption Line Quasars in Sloan Digital Sky Survey Data Release 5","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.2747","snapshot_observed_at":"2026-08-06T23:10:44.067216Z","title":"ApJ 692, 758–777","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2009,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.067216Z"},"links":{"cited_paper":"/paper/0810.2747","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:786a21cf9438c8c6e6514688ba17a61ea2f1e19b3eb836fa24d86f6367eb1bfe","observation_id":"4be4c11e-e338-4937-8de3-586755858ad4","resolution":{"observed_at":"2026-08-06T23:10:44.067216Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.2562","last_updated":"2010-05-14T16:06:14Z","snapshot_observed_at":"2026-08-04T12:14:31.965798Z","submitted_at":"2010-05-14T16:06:14Z","title":"Star formation in AGN hosts in GOODS-N","version":1},"cited_work":{"arxiv_id":"1005.2562","doi":null,"metadata_source":"pith","pith_arxiv_id":"1005.2562","snapshot_observed_at":"2026-08-06T23:10:52.046792Z","title":"Star formation in AGN hosts in GOODS-N","venue":"astro-ph.CO","work_id":"24210616-6c52-4cd9-ab08-f8400be47bc5","year":2010},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2010,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:50.022264Z"},"links":{"cited_paper":"/paper/1005.2562","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:7fc34e9d0eeb70f1c445956c67b51c26ea87d9f6d99b63da2fb2fc144736583d","observation_id":"74913b46-9503-4b13-b1a3-e9d7f1883060","resolution":{"observed_at":"2026-08-06T23:10:52.053497Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0811","last_updated":"2012-05-03T20:00:06Z","snapshot_observed_at":"2026-07-06T02:47:31.276435Z","submitted_at":"2012-05-03T20:00:06Z","title":"Mid-Infrared Selection of AGN with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-Selected AGN in COSMOS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.0811","snapshot_observed_at":"2026-08-06T23:10:50.786713Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2012,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:50.786713Z"},"links":{"cited_paper":"/paper/1205.0811","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:4f1322ec3518885e2cc2d5589315934e6c4101816924f1a34b68f83f6d1105a8","observation_id":"3d7c8b2a-2a30-44ed-9998-8ad8d10aaf96","resolution":{"observed_at":"2026-08-06T23:10:50.786713Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.1706","last_updated":"2013-10-09T12:48:07Z","snapshot_observed_at":"2026-07-06T03:17:34.061431Z","submitted_at":"2013-07-05T20:00:05Z","title":"A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.1706","snapshot_observed_at":"2026-08-06T23:10:43.818038Z","title":"ApJ 776, L41","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2013,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.818038Z"},"links":{"cited_paper":"/paper/1307.1706","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:e9b463232c9afdd04bed95cd14caf07902b8fe9a781288ca4db480401c322b7e","observation_id":"a10f9b88-ccbf-480c-b33c-5387aa00831d","resolution":{"observed_at":"2026-08-06T23:10:43.818038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01226","last_updated":"2015-04-06T07:41:55Z","snapshot_observed_at":"2026-07-06T04:14:07.916976Z","submitted_at":"2015-04-06T07:41:55Z","title":"Discovery of Millimeter-Wave Excess Emission in Radio-Quiet Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01226","snapshot_observed_at":"2026-08-06T23:10:41.983681Z","title":"MNRAS 451, 517–526","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2015,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.983681Z"},"links":{"cited_paper":"/paper/1504.01226","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:1424a55da18df888f79c21d6b3404c4bdc39addb07b37e96e5126fefc373a7f8","observation_id":"da9cfe28-a36f-471b-a1cd-f50fd6bc85e5","resolution":{"observed_at":"2026-08-06T23:10:41.983681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.00205","last_updated":"2016-05-04T14:10:44Z","snapshot_observed_at":"2026-08-04T18:09:39.951189Z","submitted_at":"2016-04-01T11:22:50Z","title":"ALMA resolves the torus of NGC 1068: continuum and molecular line emission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.00205","snapshot_observed_at":"2026-08-06T23:10:43.721143Z","title":"ApJ 823, L12","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2016,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.721143Z"},"links":{"cited_paper":"/paper/1604.00205","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:73bacf77bd3bc8ebf7af1290542103468b60ba5953264d0f5050b342e3d8f100","observation_id":"b4cf2bd9-8893-47f3-b67d-e744d1298cba","resolution":{"observed_at":"2026-08-06T23:10:43.721143Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.08007","last_updated":"2016-03-25T20:00:07Z","snapshot_observed_at":"2026-07-06T04:50:44.466723Z","submitted_at":"2016-03-25T20:00:07Z","title":"Gravitational torque-driven black hole growth and feedback in cosmological simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.08007","snapshot_observed_at":"2026-08-06T23:10:41.080021Z","title":"MNRAS 464, 2840–2853","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2017,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.080021Z"},"links":{"cited_paper":"/paper/1603.08007","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:60e25ea64bb13ac4070920b86f191288afb5399397a836509c9e8bff57cf21a8","observation_id":"b6550bed-19b7-4f4b-b76a-c1f56325e8e0","resolution":{"observed_at":"2026-08-06T23:10:41.080021Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.09901","last_updated":"2017-12-04T20:33:12Z","snapshot_observed_at":"2026-08-08T10:32:41.840135Z","submitted_at":"2017-06-29T18:00:05Z","title":"The WISE AGN Catalog","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.09901","snapshot_observed_at":"2026-08-06T23:10:41.415931Z","title":"ApJS 234, 23","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2018,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.415931Z"},"links":{"cited_paper":"/paper/1706.09901","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:dd3fde17906dd48cf026ef1fd94070044bc2583573cdf74bc975caac9708a62c","observation_id":"db4bf11f-aa30-4602-8cc7-237b82354242","resolution":{"observed_at":"2026-08-06T23:10:41.415931Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.05917","last_updated":"2019-02-15T18:00:31Z","snapshot_observed_at":"2026-08-04T05:23:12.121566Z","submitted_at":"2019-02-15T18:00:31Z","title":"The Origin of Radio Emission from Radio-Quiet AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.05917","snapshot_observed_at":"2026-08-06T23:10:48.149728Z","title":"Nature Astronomy 3, 387–396","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2019,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:48.149728Z"},"links":{"cited_paper":"/paper/1902.05917","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:155414306a5527ab42a17bcdbc219c2fd6d05ea53c8f56357ce5fc6f81b7ed13","observation_id":"465bf533-ac93-4155-ad02-388dc3638667","resolution":{"observed_at":"2026-08-06T23:10:48.149728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.11017","last_updated":"2024-04-17T02:48:13Z","snapshot_observed_at":"2026-07-30T23:13:43.117588Z","submitted_at":"2024-04-17T02:48:13Z","title":"SPHEREx: NASA's Near-Infrared Spectrophotmetric All-Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.11017","snapshot_observed_at":"2026-08-06T23:10:42.646726Z","title":"(Eds.), Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, p","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2020,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:42.646726Z"},"links":{"cited_paper":"/paper/2404.11017","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:c3f73e5361aee233958bd90daa74f0e31271bb22e040e2372654b0a495f8ec3f","observation_id":"465432e5-dbad-4d32-9fc8-695a7f4875d9","resolution":{"observed_at":"2026-08-06T23:10:42.646726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13232","last_updated":"2021-08-22T09:36:17Z","snapshot_observed_at":"2026-07-06T09:32:02.150002Z","submitted_at":"2020-06-23T18:00:05Z","title":"Properties of the Multiphase Outflows in Local (Ultra)luminous Infrared Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13232","snapshot_observed_at":"2026-08-06T23:10:43.555694Z","title":"MNRAS 505, 5753–5783","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2021,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:43.555694Z"},"links":{"cited_paper":"/paper/2006.13232","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:59f6e523a564b5927c7dfdd89dfcb0428820ed34b5aaa133964570aa8105e336","observation_id":"ad29fc82-139e-4188-8d7e-a2e7eb90fe73","resolution":{"observed_at":"2026-08-06T23:10:43.555694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01627","last_updated":"2022-08-02T17:56:52Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:56:52Z","title":"XMM-Newton and NuSTAR Observations of an Optically Quiescent Quasar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01627","snapshot_observed_at":"2026-08-06T23:10:44.308486Z","title":"ApJ 934, L34","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2022,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:44.308486Z"},"links":{"cited_paper":"/paper/2208.01627","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:13e64374160869791fd12889c16cdd9500c9ccb0d0afab99a85075f94bbcccac","observation_id":"01f5cc67-03cd-4d27-8002-dde669e2e4c7","resolution":{"observed_at":"2026-08-06T23:10:44.308486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.02531","last_updated":"2023-07-05T18:00:01Z","snapshot_observed_at":"2026-08-07T07:19:07.596321Z","submitted_at":"2023-07-05T18:00:01Z","title":"Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at $z\\sim6$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02531","snapshot_observed_at":"2026-08-06T23:10:41.143325Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress","version":2},"reference_index":2023,"source":"pdf_text","source_observed_at":"2026-08-06T23:10:41.143325Z"},"links":{"cited_paper":"/paper/2307.02531","citing_paper":"/paper/2506.19166"},"observation_digest":"sha256:d4295adb934df1bbfb34b8310031c6618f274814e12576f6e8e164661ab95f84","observation_id":"3d3779c2-9fca-4d71-9d30-f9707388e2f4","resolution":{"observed_at":"2026-08-06T23:10:41.143325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.19166","last_updated":"2025-08-15T15:04:58Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-09T02:11:28.382281Z","submitted_at":"2025-06-23T22:04:45Z","title":"What drives the growth of black holes: a decade of progress"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":7,"metadata_mismatch":8,"parse_uncertain":0,"unresolved":70,"verified_exact":15,"verified_fuzzy":0},"total_outbound_references":114},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 114 outbound references and 3 inbound Pith citation observations for arXiv:2506.19166."}