{"as_of":"2026-08-17T13:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e9b268354505516e8fb33bd0fb77a81ddee0570b3b35ee955db9f2b4bc2a904e","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:33:47.702343Z","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":"2026-07-12T03:38:27.687542Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0908.0386","last_updated":"2009-10-16T05:09:43Z","snapshot_observed_at":"2026-08-15T06:39:47.430551Z","submitted_at":"2009-08-04T05:58:34Z","title":"What broad emission lines tell us about how active galactic nuclei work","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0386","snapshot_observed_at":"2026-08-11T04:33:47.702343Z","title":"What broad emission lines tell us about how active galactic nuclei work","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.702343Z"},"links":{"cited_paper":"/paper/0908.0386","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:e460805fa43217f177be8f1bd9357d5a354d8b1a9f12d36bc81c09b21ddbc774","observation_id":"ad22197b-df74-4136-ae2f-6d2fe1f4248a","resolution":{"observed_at":"2026-08-11T04:33:47.702343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0386","last_updated":"2009-10-16T05:09:43Z","snapshot_observed_at":"2026-08-15T06:39:47.430551Z","submitted_at":"2009-08-04T05:58:34Z","title":"What broad emission lines tell us about how active galactic nuclei work","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0386","snapshot_observed_at":"2026-08-04T18:47:40.941208Z","title":"NAR53(7-10), 140–148 (2009) https://doi.org/10.1016/j.newar.2009.09","venue":null,"work_id":null,"year":2009},"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":69,"source":"pdf_text","source_observed_at":"2026-08-04T18:47:40.941208Z"},"links":{"cited_paper":"/paper/0908.0386","citing_paper":"/paper/2509.09607"},"observation_digest":"sha256:64d57e8e414b12273dde0a6eb23a3eda3118689adda385084d05bdaf239c0899","observation_id":"cd16b63a-ae97-417b-a552-b54fb6b21e59","resolution":{"observed_at":"2026-08-04T18:47:40.941208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0386","last_updated":"2009-10-16T05:09:43Z","snapshot_observed_at":"2026-08-15T06:39:47.430551Z","submitted_at":"2009-08-04T05:58:34Z","title":"What broad emission lines tell us about how active galactic nuclei work","version":2},"cited_work":{"arxiv_id":"0908.0386","doi":null,"metadata_source":"pith","pith_arxiv_id":"0908.0386","snapshot_observed_at":"2026-07-12T03:38:27.687542Z","title":"What broad emission lines tell us about how active galactic nuclei work","venue":"astro-ph.CO","work_id":"ac2b38cd-893c-4828-9ac2-3d6e4d44470d","year":2009},"citing_paper":{"arxiv_id":"2607.03291","last_updated":"2026-07-03T13:01:11Z","snapshot_observed_at":"2026-08-16T00:11:23.533407Z","submitted_at":"2026-07-03T13:01:11Z","title":"Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference","version":1},"reference_index":179,"source":"arxiv_source","source_observed_at":"2026-07-12T03:29:42.101488Z"},"links":{"cited_paper":"/paper/0908.0386","citing_paper":"/paper/2607.03291"},"observation_digest":"sha256:6b1e96f6ef60989502dd4244c83d998a20688cc2e9c667905dedf2f3adb6376e","observation_id":"36b10daa-fb43-4d42-b48c-3015d580fb69","resolution":{"observed_at":"2026-07-12T03:38:27.689617Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/0908.0386/citation-record","integrity":"/paper/0908.0386/integrity","json":"/paper/0908.0386/citation-record.json","paper":"/paper/0908.0386"},"outbound":[],"paper":{"arxiv_id":"0908.0386","last_updated":"2009-10-16T05:09:43Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T06:39:47.430551Z","submitted_at":"2009-08-04T05:58:34Z","title":"What broad emission lines tell us about how active galactic nuclei work"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0908.0386."}