{"as_of":"2026-08-16T05:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f830e5edd7c59e5a8d9f974e9a63291a6d96cc2df3544bc2df57f0a7ad5c6eb5","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T05:14:38.834061Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T11:58:06.452953Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-08-11T05:14:38.834061Z","title":"Gilli, C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.17919","last_updated":"2025-07-02T15:11:58Z","snapshot_observed_at":"2026-08-13T17:32:07.055298Z","submitted_at":"2024-12-23T19:19:42Z","title":"Fermionic Dark Matter spikes: origin and growth of Black Hole seeds","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T05:14:38.834061Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2412.17919"},"observation_digest":"sha256:cacf1aaf104f4b084f5b8a8c34251a964064d489b15a3899bb761a9817d83c28","observation_id":"88c4aa82-8eae-4047-b857-57a20a9bb977","resolution":{"observed_at":"2026-08-11T05:14:38.834061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-08-05T06:04:38.558030Z","title":"arXiv:2206.03508","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.04553","last_updated":"2025-09-04T18:00:00Z","snapshot_observed_at":"2026-08-14T11:13:36.003009Z","submitted_at":"2025-09-04T18:00:00Z","title":"Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-05T06:04:38.558030Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2509.04553"},"observation_digest":"sha256:5c933059862dd0d876c061d53e3999329bce97ad0f115eae91c224377d602b98","observation_id":"90940caa-05d7-4902-bd89-854fd0bda228","resolution":{"observed_at":"2026-08-05T06:04:38.558030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":"2206.03508","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-07-03T11:58:06.452953Z","title":"title Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","venue":null,"work_id":"d8fe1db8-db3a-448e-8a78-2417f0bd8372","year":2022},"citing_paper":{"arxiv_id":"2606.12076","last_updated":"2026-06-10T13:41:54Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-10T13:41:54Z","title":"X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-06-27T09:31:03.142220Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2606.12076"},"observation_digest":"sha256:0b80163a77b37b42d8f9d85717cbd4942b28bc71a6f9c590bcc56eb031942a0d","observation_id":"36c6faca-4524-4d21-b12b-3bc33da37c5e","resolution":{"observed_at":"2026-07-03T11:28:04.776967Z","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":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":"2206.03508","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-07-03T11:58:06.452953Z","title":"title Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","venue":null,"work_id":"d8fe1db8-db3a-448e-8a78-2417f0bd8372","year":2022},"citing_paper":{"arxiv_id":"2606.12511","last_updated":"2026-07-25T15:53:46Z","snapshot_observed_at":"2026-08-15T05:45:43.107781Z","submitted_at":"2026-06-10T18:00:00Z","title":"Unification models of Active Galactic Nuclei","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-06-27T09:13:32.045559Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2606.12511"},"observation_digest":"sha256:20f9d6cee26f71e838120af167a02221120f994e990e153639c005f39337f57d","observation_id":"bf16431e-b5c2-4c4b-8682-71efc98067ce","resolution":{"observed_at":"2026-07-03T11:58:06.454564Z","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":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-08-02T11:51:38.075544Z","title":"title Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2606.12511","last_updated":"2026-07-25T15:53:46Z","snapshot_observed_at":"2026-08-15T05:45:43.107781Z","submitted_at":"2026-06-10T18:00:00Z","title":"Unification models of Active Galactic Nuclei","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-02T11:51:38.075544Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2606.12511"},"observation_digest":"sha256:7f26645c94670e419187c9af2039c64d27739aaf94657769b569b6883dbf91b7","observation_id":"0bc717d4-0ef6-4afb-bfe9-f9a888479ee3","resolution":{"observed_at":"2026-08-02T11:51:38.075544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":"2206.03508","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-07-03T11:58:06.452953Z","title":"title Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","venue":null,"work_id":"d8fe1db8-db3a-448e-8a78-2417f0bd8372","year":2022},"citing_paper":{"arxiv_id":"2606.30734","last_updated":"2026-06-29T18:00:03Z","snapshot_observed_at":"2026-08-14T02:30:34.560548Z","submitted_at":"2026-06-29T18:00:03Z","title":"The Lifetimes of High-redshift Quasars Suggest Magnetic Disk Support","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-01T01:55:17.964847Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2606.30734"},"observation_digest":"sha256:a0b818f0f4d924a88599242c969474c8a880dd535c7ffe555944df5850b22355","observation_id":"b252f308-295f-472c-b00b-54776b6c4381","resolution":{"observed_at":"2026-07-01T12:35:44.161896Z","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":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.03508","snapshot_observed_at":"2026-08-01T13:38:31.529260Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19057","last_updated":"2026-07-21T12:45:36Z","snapshot_observed_at":"2026-08-14T12:22:56.355344Z","submitted_at":"2026-07-21T12:45:36Z","title":"An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars","version":1},"reference_index":111,"source":"arxiv_source","source_observed_at":"2026-08-01T13:38:31.529260Z"},"links":{"cited_paper":"/paper/2206.03508","citing_paper":"/paper/2607.19057"},"observation_digest":"sha256:25540e8fd1f5090177ce9907e38932f0e038b78ad2ed279e650630ffd89f2915","observation_id":"5af14067-9f34-426c-83ef-1bce856a5819","resolution":{"observed_at":"2026-08-01T13:38:31.529260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2206.03508/citation-record","integrity":"/paper/2206.03508/integrity","json":"/paper/2206.03508/citation-record.json","paper":"/paper/2206.03508"},"outbound":[],"paper":{"arxiv_id":"2206.03508","last_updated":"2022-07-22T07:02:01Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-13T15:28:28.556598Z","submitted_at":"2022-06-07T18:00:02Z","title":"Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium"},"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 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2206.03508."}