{"as_of":"2026-08-16T03:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:dcd07a6d2be9be9186ca312ff5ec2eed35c12111e03aa0ffd333bdb66a1a01eb","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":"2026-08-15T06:32:42.880941+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":"2026-08-15T15:15:04.623143Z","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":"2026-07-03T11:28:04.705984Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1501.04335","last_updated":"2015-02-11T16:36:54Z","snapshot_observed_at":"2026-08-14T23:03:40.755133Z","submitted_at":"2015-01-18T18:56:49Z","title":"Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN","version":2},"cited_work":{"arxiv_id":"1501.04335","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.04335","snapshot_observed_at":"2026-07-03T11:28:04.705984Z","title":"Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN","venue":"astro-ph.GA","work_id":"4e0fc166-6dae-4575-b43e-5a56b3b860da","year":2015},"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":55,"source":"arxiv_source","source_observed_at":"2026-06-27T09:31:03.142220Z"},"links":{"cited_paper":"/paper/1501.04335","citing_paper":"/paper/2606.12076"},"observation_digest":"sha256:697ebdd126b9f851ab59059b67f8c5020941fee3c9b5c886ce9013d8399ea57c","observation_id":"1140207a-614e-4455-a5d8-2611360b3c2d","resolution":{"observed_at":"2026-07-03T11:28:04.707230Z","resolver_source":"local_arxiv","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":"1501.04335","last_updated":"2015-02-11T16:36:54Z","snapshot_observed_at":"2026-08-14T23:03:40.755133Z","submitted_at":"2015-01-18T18:56:49Z","title":"Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.04335","snapshot_observed_at":"2026-08-15T15:15:04.623143Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.01249","last_updated":"2026-08-02T14:01:09Z","snapshot_observed_at":"2026-08-15T18:53:43.936121Z","submitted_at":"2026-08-02T14:01:09Z","title":"The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-15T15:15:04.623143Z"},"links":{"cited_paper":"/paper/1501.04335","citing_paper":"/paper/2608.01249"},"observation_digest":"sha256:a2242bbff137093502378061af3843349f8d4ad85a56c4ee5ca593a583058889","observation_id":"7c0c0980-2fa3-46c6-99aa-6992ee57a6ac","resolution":{"observed_at":"2026-08-15T15:15:04.623143Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1501.04335/citation-record","integrity":"/paper/1501.04335/integrity","json":"/paper/1501.04335/citation-record.json","paper":"/paper/1501.04335"},"outbound":[],"paper":{"arxiv_id":"1501.04335","last_updated":"2015-02-11T16:36:54Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T23:03:40.755133Z","submitted_at":"2015-01-18T18:56:49Z","title":"Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN"},"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 2 inbound Pith citation observations for arXiv:1501.04335."}