{"as_of":"2026-08-15T11:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:71b5f1d77b4f85f9e8d44dd419992c01ca59e6999eb882cabfc803831ac3c1af","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:19:00.607583Z","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":8,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-11T23:20:51.951904Z","title":"N., Kondapally, R., Williams, W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.02622","last_updated":"2024-12-03T17:50:49Z","snapshot_observed_at":"2026-08-12T20:00:52.389871Z","submitted_at":"2024-12-03T17:50:49Z","title":"High-z stellar masses can be recovered robustly with JWST photometry","version":1},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-08-11T23:20:51.951904Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2412.02622"},"observation_digest":"sha256:ee783ffbffb9f00b54cd11f363cb2b33d293b91cec1744d713020faf569cbc8a","observation_id":"2142d191-4165-44f9-811b-92fac5d3a7e7","resolution":{"observed_at":"2026-08-11T23:20:51.951904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-11T21:08:52.461993Z","title":"Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.04983","last_updated":"2024-12-06T12:07:44Z","snapshot_observed_at":"2026-08-14T07:19:12.269532Z","submitted_at":"2024-12-06T12:07:44Z","title":"Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr","version":1},"reference_index":160,"source":"pdf_text","source_observed_at":"2026-08-11T21:08:52.461993Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2412.04983"},"observation_digest":"sha256:3a653cd245e081ed886729226818a0679774d0a93921423350e89f7f18bcbb7f","observation_id":"70d3f6aa-fb95-4c73-bf58-bfd76eae460e","resolution":{"observed_at":"2026-08-11T21:08:52.461993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-11T12:29:56.581815Z","title":"G., Kocevski, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.14248","last_updated":"2024-12-18T19:00:02Z","snapshot_observed_at":"2026-08-14T12:20:40.607561Z","submitted_at":"2024-12-18T19:00:02Z","title":"Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T12:29:56.581815Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2412.14248"},"observation_digest":"sha256:9bd19510b8bb5fb40ca7474c564016a8797a27833e4c0b57fd69ef54bc155027","observation_id":"851fa07f-9897-4750-8383-dfc728da3b82","resolution":{"observed_at":"2026-08-11T12:29:56.581815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-04T18:47:40.755015Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.09607","last_updated":"2025-09-11T16:47:50Z","snapshot_observed_at":"2026-08-14T05:02:24.881223Z","submitted_at":"2025-09-11T16:47:50Z","title":"Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-04T18:47:40.755015Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2509.09607"},"observation_digest":"sha256:18797ed1ef407dc237d35ffd2502ecf43b98cd448747cddf6f47efcaaaac6381","observation_id":"7a729765-3246-47a4-8e6f-8f41eb59b4db","resolution":{"observed_at":"2026-08-04T18:47:40.755015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":"2305.14418","doi":"10.48550/arxiv.2305.14418","metadata_source":"arxiv_reference","pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Kocevski, Dale D","venue":"arXiv (Cornell University)","work_id":"e7735461-d03b-4c78-8376-1b1411e034cf","year":2024},"citing_paper":{"arxiv_id":"2604.18173","last_updated":"2026-04-20T12:32:48Z","snapshot_observed_at":"2026-08-13T01:59:36.194422Z","submitted_at":"2026-04-20T12:32:48Z","title":"Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-05-10T04:58:18.085345Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2604.18173"},"observation_digest":"sha256:fb574951dd7628cc8e543b4cc96afb7390e0d394291a11475307fa76a00e102c","observation_id":"5e479e3e-cb5e-4d9e-ae42-7bae4237612f","resolution":{"observed_at":"2026-05-10T05:00:36.924938Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":"2305.14418","doi":"10.48550/arxiv.2305.14418","metadata_source":"arxiv_reference","pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Kocevski, Dale D","venue":"arXiv (Cornell University)","work_id":"e7735461-d03b-4c78-8376-1b1411e034cf","year":2024},"citing_paper":{"arxiv_id":"2605.06769","last_updated":"2026-07-09T09:36:58Z","snapshot_observed_at":"2026-07-12T23:17:31.068177Z","submitted_at":"2026-05-07T18:00:01Z","title":"Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model","version":1},"reference_index":212,"source":"arxiv_source","source_observed_at":"2026-05-11T00:53:14.584468Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2605.06769"},"observation_digest":"sha256:901bd7f2256b63f56cc71d45e45f3f509c174914cc62528947de1c0e6c46d233","observation_id":"299ea48e-5fa6-44db-a5ba-733468e32914","resolution":{"observed_at":"2026-05-11T01:30:51.643092Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":"2305.14418","doi":"10.48550/arxiv.2305.14418","metadata_source":"arxiv_reference","pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Kocevski, Dale D","venue":"arXiv (Cornell University)","work_id":"e7735461-d03b-4c78-8376-1b1411e034cf","year":2024},"citing_paper":{"arxiv_id":"2606.04081","last_updated":"2026-06-02T18:00:00Z","snapshot_observed_at":"2026-07-06T23:44:14.261541Z","submitted_at":"2026-06-02T18:00:00Z","title":"The role of major mergers in triggering super-Eddington accretion","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-06-28T08:58:09.556687Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2606.04081"},"observation_digest":"sha256:54c07c5c68a5350eaf6211c3867785593f86c06d2d42ec8e6fdac8771a8c82cf","observation_id":"7df6f61c-66f7-4cd7-ae67-3ed983af9a74","resolution":{"observed_at":"2026-06-28T09:01:48.747691Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":"2305.14418","doi":"10.48550/arxiv.2305.14418","metadata_source":"arxiv_reference","pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Kocevski, Dale D","venue":"arXiv (Cornell University)","work_id":"e7735461-d03b-4c78-8376-1b1411e034cf","year":2024},"citing_paper":{"arxiv_id":"2606.05281","last_updated":"2026-06-03T18:00:00Z","snapshot_observed_at":"2026-08-03T00:56:47.377000Z","submitted_at":"2026-06-03T18:00:00Z","title":"Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-28T05:20:29.507384Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2606.05281"},"observation_digest":"sha256:d90e0470d6ce265ae7e1561a86ff82fb0cb92631a37acbdbc80f5703bb2d757b","observation_id":"c31cdea9-90a0-43ae-939e-1e531a8cc16c","resolution":{"observed_at":"2026-07-02T10:06:51.568125Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":"2305.14418","doi":"10.48550/arxiv.2305.14418","metadata_source":"arxiv_reference","pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Kocevski, Dale D","venue":"arXiv (Cornell University)","work_id":"e7735461-d03b-4c78-8376-1b1411e034cf","year":2024},"citing_paper":{"arxiv_id":"2607.00084","last_updated":"2026-06-30T19:23:00Z","snapshot_observed_at":"2026-08-06T12:38:42.213654Z","submitted_at":"2026-06-30T19:23:00Z","title":"Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-07-02T18:25:22.489682Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2607.00084"},"observation_digest":"sha256:1e24f719e996ae0512dc35eed249c89db3b21e74be9ee8560d572fe0c1627249","observation_id":"4d70044c-11f7-4283-90b0-2822614fa079","resolution":{"observed_at":"2026-07-02T18:27:16.080001Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T12:50:12.236141+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-07-11T21:10:16.126324Z","title":"and Kocevski, Dale D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.04176","last_updated":"2026-07-15T10:51:44Z","snapshot_observed_at":"2026-08-13T04:52:27.331984Z","submitted_at":"2026-07-05T08:50:15Z","title":"Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP","version":1},"reference_index":177,"source":"arxiv_source","source_observed_at":"2026-07-11T21:10:16.126324Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2607.04176"},"observation_digest":"sha256:3032bb51ca137912723bb5b56561a1107a5751607cb557bacbca4b985efd7130","observation_id":"02cec2bc-b82c-46d8-a3de-85ddfe97f220","resolution":{"observed_at":"2026-07-11T21:10:16.126324Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-02T08:46:56.683272Z","title":"and Kocevski, Dale D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.04176","last_updated":"2026-07-15T10:51:44Z","snapshot_observed_at":"2026-08-13T04:52:27.331984Z","submitted_at":"2026-07-05T08:50:15Z","title":"Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP","version":2},"reference_index":177,"source":"arxiv_source","source_observed_at":"2026-08-02T08:46:56.683272Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2607.04176"},"observation_digest":"sha256:b8f2d9f63384dcde473448c4ae6736969b9eed46d4a9ed05113cdf14825a79a9","observation_id":"818c9f96-d6a3-41d1-a86d-83494846a0af","resolution":{"observed_at":"2026-08-02T08:46:56.683272Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-08T16:36:20.649011Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05267","last_updated":"2026-08-05T18:00:00Z","snapshot_observed_at":"2026-08-13T04:40:26.580767Z","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":101,"source":"arxiv_source","source_observed_at":"2026-08-08T16:36:20.649011Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2608.05267"},"observation_digest":"sha256:83ab1f447c54eed3c9f30911f4b00840cd16f261221e25b173bf61a766cb447a","observation_id":"424e0438-c4ad-455a-a746-ae7bf564ae83","resolution":{"observed_at":"2026-08-08T16:36:20.649011Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.14418","snapshot_observed_at":"2026-08-14T04:19:00.607583Z","title":"arXiv , author =:2305.14418 , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10070","last_updated":"2026-08-10T18:00:01Z","snapshot_observed_at":"2026-08-15T03:40:56.639387Z","submitted_at":"2026-08-10T18:00:01Z","title":"A cosmic collision in the making: JWST/NIRISS reveals a merging and maturing protocluster core at z~3 around a red quasar","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:00.607583Z"},"links":{"cited_paper":"/paper/2305.14418","citing_paper":"/paper/2608.10070"},"observation_digest":"sha256:dff0cc70233a7fd6fe0c6e387b60749a9ba5e9af27700033737fb98051e66dcc","observation_id":"7b5111dc-2661-4f5e-9706-a7dc5f9398c0","resolution":{"observed_at":"2026-08-14T04:19:00.607583Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2305.14418/citation-record","integrity":"/paper/2305.14418/integrity","json":"/paper/2305.14418/citation-record.json","paper":"/paper/2305.14418"},"outbound":[],"paper":{"arxiv_id":"2305.14418","last_updated":"2023-05-23T18:00:01Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-13T11:35:14.867316Z","submitted_at":"2023-05-23T18:00:01Z","title":"Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2305.14418."}