{"as_of":"2026-08-11T01:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6ec8d254b4f5acfa97b31cd2b2a6ef8e142e35178d1c98cc30291b683eb20f8f","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T13:38:40.864020Z","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":"2026-07-03T11:28:04.708510Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2209.07797","last_updated":"2022-09-30T07:40:14Z","snapshot_observed_at":"2026-07-06T13:52:58.803007Z","submitted_at":"2022-09-16T08:53:35Z","title":"The Obscured Fraction of Quasars at Cosmic Noon","version":2},"cited_work":{"arxiv_id":"2209.07797","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.07797","snapshot_observed_at":"2026-07-03T11:28:04.708510Z","title":"2022 , month = dec, number =","venue":null,"work_id":"bd6ad15e-1167-456e-a678-6085c44403cd","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":75,"source":"arxiv_source","source_observed_at":"2026-06-27T09:31:03.142220Z"},"links":{"cited_paper":"/paper/2209.07797","citing_paper":"/paper/2606.12076"},"observation_digest":"sha256:63cdf75c81f37a0f88213f62aec5d7c445256fba32c6f9a02fe4fb02962caf22","observation_id":"4f926024-c9e4-495e-9f43-e638aedf0d86","resolution":{"observed_at":"2026-07-03T11:28:04.709908Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07797","last_updated":"2022-09-30T07:40:14Z","snapshot_observed_at":"2026-07-06T13:52:58.803007Z","submitted_at":"2022-09-16T08:53:35Z","title":"The Obscured Fraction of Quasars at Cosmic Noon","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07797","snapshot_observed_at":"2026-08-01T13:38:40.864020Z","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":"2026-08-07T11:36:56.346856Z","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":216,"source":"arxiv_source","source_observed_at":"2026-08-01T13:38:40.864020Z"},"links":{"cited_paper":"/paper/2209.07797","citing_paper":"/paper/2607.19057"},"observation_digest":"sha256:600a2c645d8971ef459bd1a999055c9a50dad12663356f16230525bf751f83f1","observation_id":"902337ab-6241-4990-ae39-5601ee917c86","resolution":{"observed_at":"2026-08-01T13:38:40.864020Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2209.07797/citation-record","integrity":"/paper/2209.07797/integrity","json":"/paper/2209.07797/citation-record.json","paper":"/paper/2209.07797"},"outbound":[],"paper":{"arxiv_id":"2209.07797","last_updated":"2022-09-30T07:40:14Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T13:52:58.803007Z","submitted_at":"2022-09-16T08:53:35Z","title":"The Obscured Fraction of Quasars at Cosmic Noon"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2209.07797."}