{"as_of":"2026-08-05T14:18:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:257c2adb69fffcfb285dd42e77645c9d7846d360064ee277f42e184168157b59","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":"2026-08-05T06:32:48.257954+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":"2026-08-01T00:33:52.672254Z","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":"2026-07-03T08:27:48.378611Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":"1405.1415","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-07-03T08:27:48.378611Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","venue":"astro-ph.HE","work_id":"c3a4267f-46ac-4c86-b3aa-dfcdaaa1f113","year":2014},"citing_paper":{"arxiv_id":"2605.20327","last_updated":"2026-05-19T18:00:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-19T18:00:01Z","title":"On the origin of anomalous dissipation in simulations of tidal disruption events","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2605.20327"},"observation_digest":"sha256:7730f7af523af83e224d41cd5e5f911d2e3608f8e6c9fe1cc88a884888e264b2","observation_id":"37492724-484d-44b4-a00f-ff9242afe348","resolution":{"observed_at":"2026-05-21T01:23:53.927538Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":"1405.1415","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-07-03T08:27:48.378611Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","venue":"astro-ph.HE","work_id":"c3a4267f-46ac-4c86-b3aa-dfcdaaa1f113","year":2014},"citing_paper":{"arxiv_id":"2606.04090","last_updated":"2026-06-02T18:00:03Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-02T18:00:03Z","title":"Mapping the nuclear environments of extreme coronal line emitting galaxies","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2606.04090"},"observation_digest":"sha256:d94b51a4c453c22f324039bc3db1f9b38bd19bcbdc72f750ab690b8d3c946744","observation_id":"9f13ec5c-97b0-4124-81e0-b5db4cf5a933","resolution":{"observed_at":"2026-06-28T09:11:49.325540Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":"1405.1415","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-07-03T08:27:48.378611Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","venue":"astro-ph.HE","work_id":"c3a4267f-46ac-4c86-b3aa-dfcdaaa1f113","year":2014},"citing_paper":{"arxiv_id":"2606.04740","last_updated":"2026-06-03T11:22:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-03T11:22:16Z","title":"TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2606.04740"},"observation_digest":"sha256:7fdc51c63817f53beb0982cf2ddd532898d483e8d2d161f8cb0db8ef27692cd2","observation_id":"973ed995-6ad2-4386-817e-3e37f37aabec","resolution":{"observed_at":"2026-06-28T05:31:40.103381Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":"1405.1415","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-07-03T08:27:48.378611Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","venue":"astro-ph.HE","work_id":"c3a4267f-46ac-4c86-b3aa-dfcdaaa1f113","year":2014},"citing_paper":{"arxiv_id":"2607.01604","last_updated":"2026-07-02T02:05:31Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-07-02T02:05:31Z","title":"Bolometric correction factor and radiative efficiency for the super-Eddington accretion flow in tidal disruption events","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2607.01604"},"observation_digest":"sha256:f0a28713574bd77c264eee506880d427b60030541a2f3dd598443abc08fb0206","observation_id":"a1f79146-7e1a-48a0-8e48-4f14dcb8f9d4","resolution":{"observed_at":"2026-07-03T08:27:48.380262Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-07-14T15:04:53.805474Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09850","last_updated":"2026-07-14T12:30:59Z","snapshot_observed_at":"2026-07-31T19:11:29.059557Z","submitted_at":"2026-07-10T18:00:00Z","title":"Low-hard to high-soft spectral state transitions in the faintest early-X-ray-detected optical tidal disruption event TDE 2025aarm","version":1},"reference_index":151,"source":"arxiv_source","source_observed_at":"2026-07-14T15:04:53.805474Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2607.09850"},"observation_digest":"sha256:8f8701fdd8c3eee789e102b6f434c33077c3d96a5c48a9fc5a719ba4495ecc3f","observation_id":"843db853-1a6c-40e2-a72d-d8c452946476","resolution":{"observed_at":"2026-07-14T15:04:53.805474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-07-14T04:54:13.013192Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11539","last_updated":"2026-07-13T13:23:31Z","snapshot_observed_at":"2026-08-04T04:21:20.548931Z","submitted_at":"2026-07-13T13:23:31Z","title":"Two Earliest Optical-UV Tidal Disruption Events Hidden in the SDSS DR7 Catalog Unveiled by the Transformer-Based Spectrum Classifier","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-14T04:54:13.013192Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2607.11539"},"observation_digest":"sha256:ce464d27cc4206b6a43bae208b646767d0291d824f2e63dfbb5845ada8df8894","observation_id":"ab51586a-46a1-41d7-bad0-ea6289f9f333","resolution":{"observed_at":"2026-07-14T04:54:13.013192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1415","snapshot_observed_at":"2026-08-01T00:33:52.672254Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.26205","last_updated":"2026-07-28T19:12:16Z","snapshot_observed_at":"2026-08-05T11:58:47.499728Z","submitted_at":"2026-07-28T19:12:16Z","title":"Binary disruptions driven by massive disks around massive black holes","version":1},"reference_index":223,"source":"arxiv_source","source_observed_at":"2026-08-01T00:33:52.672254Z"},"links":{"cited_paper":"/paper/1405.1415","citing_paper":"/paper/2607.26205"},"observation_digest":"sha256:9dfa56b8ec60468f2c17a005a775c62eb0d36215a9697adff82f46d8793ffe92","observation_id":"c49e16bd-3c36-41e7-a679-b8258db24a78","resolution":{"observed_at":"2026-08-01T00:33:52.672254Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1405.1415/citation-record","integrity":"/paper/1405.1415/integrity","json":"/paper/1405.1415/citation-record.json","paper":"/paper/1405.1415"},"outbound":[],"paper":{"arxiv_id":"1405.1415","last_updated":"2014-08-21T01:59:40Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:09Z","title":"A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1405.1415."}