{"as_of":"2026-08-06T17:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:74e3714f5f48460f334215a89a51298b8ee0d5153827976e281c5a97a8bd4069","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-03T19:48:52.668705Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1503.02085","last_updated":"2015-03-06T21:00:59Z","snapshot_observed_at":"2026-07-06T04:11:15.487869Z","submitted_at":"2015-03-06T21:00:59Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","version":1},"cited_work":{"arxiv_id":"1503.02085","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.02085","snapshot_observed_at":"2026-07-03T19:48:52.668705Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","venue":"astro-ph.GA","work_id":"0fe3e671-8afc-42ca-9509-0107b8f6fbfb","year":2015},"citing_paper":{"arxiv_id":"2605.22918","last_updated":"2026-05-21T18:00:35Z","snapshot_observed_at":"2026-08-03T01:02:54.923618Z","submitted_at":"2026-05-21T18:00:35Z","title":"Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1503.02085","citing_paper":"/paper/2605.22918"},"observation_digest":"sha256:61f2f95f441291a92623160a8911dad1b762fe7670bb35f0fac70984c9e49a35","observation_id":"9a0ad164-7d44-4f98-ab05-3409154e01dd","resolution":{"observed_at":"2026-05-25T05:35:22.061475Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02085","last_updated":"2015-03-06T21:00:59Z","snapshot_observed_at":"2026-07-06T04:11:15.487869Z","submitted_at":"2015-03-06T21:00:59Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","version":1},"cited_work":{"arxiv_id":"1503.02085","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.02085","snapshot_observed_at":"2026-07-03T19:48:52.668705Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","venue":"astro-ph.GA","work_id":"0fe3e671-8afc-42ca-9509-0107b8f6fbfb","year":2015},"citing_paper":{"arxiv_id":"2606.00992","last_updated":"2026-05-31T04:15:31Z","snapshot_observed_at":"2026-07-06T23:41:39.172310Z","submitted_at":"2026-05-31T04:15:31Z","title":"Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1503.02085","citing_paper":"/paper/2606.00992"},"observation_digest":"sha256:aac1c7afd83150c064782b4213c2c7737b34af0ca01df94366ea004749c6309d","observation_id":"77f8100d-19a5-4527-9bdb-d9e72ff0045e","resolution":{"observed_at":"2026-06-28T17:32:25.208762Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02085","last_updated":"2015-03-06T21:00:59Z","snapshot_observed_at":"2026-07-06T04:11:15.487869Z","submitted_at":"2015-03-06T21:00:59Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","version":1},"cited_work":{"arxiv_id":"1503.02085","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.02085","snapshot_observed_at":"2026-07-03T19:48:52.668705Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","venue":"astro-ph.GA","work_id":"0fe3e671-8afc-42ca-9509-0107b8f6fbfb","year":2015},"citing_paper":{"arxiv_id":"2606.30802","last_updated":"2026-06-29T18:28:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-29T18:28:21Z","title":"A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec $\\sim$3-15","version":1},"reference_index":156,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1503.02085","citing_paper":"/paper/2606.30802"},"observation_digest":"sha256:aec51814d75b26ed69738f92e26028940348c5dab6b11209edabe468c5524afc","observation_id":"f521a358-3ae5-42fb-ad28-612e221fc22f","resolution":{"observed_at":"2026-07-01T03:45:19.903944Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02085","last_updated":"2015-03-06T21:00:59Z","snapshot_observed_at":"2026-07-06T04:11:15.487869Z","submitted_at":"2015-03-06T21:00:59Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","version":1},"cited_work":{"arxiv_id":"1503.02085","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.02085","snapshot_observed_at":"2026-07-03T19:48:52.668705Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?","venue":"astro-ph.GA","work_id":"0fe3e671-8afc-42ca-9509-0107b8f6fbfb","year":2015},"citing_paper":{"arxiv_id":"2607.01330","last_updated":"2026-07-01T18:00:04Z","snapshot_observed_at":"2026-08-06T01:12:16.079007Z","submitted_at":"2026-07-01T18:00:04Z","title":"Extreme outflow velocities and weak UV emission lines indicate quasars shedding their dust cocoons","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1503.02085","citing_paper":"/paper/2607.01330"},"observation_digest":"sha256:5ff496994ce253ad8bf915a8cdcc2adcc37f3acb043c253046ca814e96814e0b","observation_id":"65f86a6a-1557-4255-9787-58fa6c2abcd1","resolution":{"observed_at":"2026-07-03T19:48:52.673432Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1503.02085/citation-record","integrity":"/paper/1503.02085/integrity","json":"/paper/1503.02085/citation-record.json","paper":"/paper/1503.02085"},"outbound":[],"paper":{"arxiv_id":"1503.02085","last_updated":"2015-03-06T21:00:59Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T04:11:15.487869Z","submitted_at":"2015-03-06T21:00:59Z","title":"X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1503.02085."}