{"as_of":"2026-08-09T02:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4a18c680ce2e0b3bf596956fc0e5acc2ed5d46f464df50e568e9b0333732e37f","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":"2026-08-08T06:32:00.761636+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":"2026-08-06T18:41:12.335664Z","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":"2026-07-09T03:25:57.940946Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1402.4803","last_updated":"2014-05-02T04:29:13Z","snapshot_observed_at":"2026-07-06T03:36:27.214082Z","submitted_at":"2014-02-19T21:00:01Z","title":"Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4803","snapshot_observed_at":"2026-08-06T18:41:12.335664Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.07785","last_updated":"2025-07-10T14:07:37Z","snapshot_observed_at":"2026-08-09T01:52:33.796066Z","submitted_at":"2025-07-10T14:07:37Z","title":"Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T18:41:12.335664Z"},"links":{"cited_paper":"/paper/1402.4803","citing_paper":"/paper/2507.07785"},"observation_digest":"sha256:1dad8490dc52d724847b84ee1ac0f1a22d94cc3684158ccb51c0ab1f74c7d2ca","observation_id":"f1bd649a-6b4a-48dd-89c5-3eafb87a09bd","resolution":{"observed_at":"2026-08-06T18:41:12.335664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.4803","last_updated":"2014-05-02T04:29:13Z","snapshot_observed_at":"2026-07-06T03:36:27.214082Z","submitted_at":"2014-02-19T21:00:01Z","title":"Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger","version":2},"cited_work":{"arxiv_id":"1402.4803","doi":null,"metadata_source":"pith","pith_arxiv_id":"1402.4803","snapshot_observed_at":"2026-07-09T03:25:57.940946Z","title":"Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger","venue":"astro-ph.HE","work_id":"9769972f-e200-4000-adc5-bccf40cb251a","year":2014},"citing_paper":{"arxiv_id":"2607.07668","last_updated":"2026-07-08T17:23:41Z","snapshot_observed_at":"2026-07-11T23:20:19.214464Z","submitted_at":"2026-07-08T17:23:41Z","title":"Subsolar-mass binary mergers of strange stars and neutron stars: gravitational waves and ejecta","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-09T03:17:52.224143Z"},"links":{"cited_paper":"/paper/1402.4803","citing_paper":"/paper/2607.07668"},"observation_digest":"sha256:1f2aacf2f68b1d25620f4c19f1e2c6990107f9a2808478c5aa6810095a5f91f4","observation_id":"fdaac0b0-43ef-4c76-8f69-212b6cccf282","resolution":{"observed_at":"2026-07-09T03:25:57.942175Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1402.4803","last_updated":"2014-05-02T04:29:13Z","snapshot_observed_at":"2026-07-06T03:36:27.214082Z","submitted_at":"2014-02-19T21:00:01Z","title":"Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4803","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10818","last_updated":"2026-07-12T16:08:28Z","snapshot_observed_at":"2026-08-08T16:02:02.874872Z","submitted_at":"2026-07-12T16:08:28Z","title":"Late-time emission-line profiles from kilonova models","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1402.4803","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:004cbf86e70aa59bdbaddaa9f3e196bc521517cee387312cf6614e4fd6f9c6e9","observation_id":"1839438c-e1af-4458-aa32-15fd7239e851","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1402.4803/citation-record","integrity":"/paper/1402.4803/integrity","json":"/paper/1402.4803/citation-record.json","paper":"/paper/1402.4803"},"outbound":[],"paper":{"arxiv_id":"1402.4803","last_updated":"2014-05-02T04:29:13Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T03:36:27.214082Z","submitted_at":"2014-02-19T21:00:01Z","title":"Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1402.4803."}