{"as_of":"2026-08-23T16:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d3fed7c802ef340afea6ac67a416f93fa9e5a7973982ef2dc17125598f4113de","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":"2026-08-23T06:30:58.430688+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":"2026-08-15T14:31:40.508915Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2307.08584","last_updated":"2023-07-17T15:55:46Z","snapshot_observed_at":"2026-08-19T04:00:18.140349Z","submitted_at":"2023-07-17T15:55:46Z","title":"Using spectral modeling to break light-curve degeneracies of type II supernovae interacting with circumstellar material","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.08584","snapshot_observed_at":"2026-08-06T18:34:11.982756Z","title":"Using spectral modeling to break light-curve degeneracies of type II supernovae interacting with circumstellar material","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.08078","last_updated":"2025-07-10T18:00:03Z","snapshot_observed_at":"2026-08-20T19:59:00.521226Z","submitted_at":"2025-07-10T18:00:03Z","title":"SN 2023ixf: The Closest Supernova of the Decade","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T18:34:11.982756Z"},"links":{"cited_paper":"/paper/2307.08584","citing_paper":"/paper/2507.08078"},"observation_digest":"sha256:e81dd53c2119d1d9311071e83e53daae94556837b4495c90baa3099db795abb6","observation_id":"c5efb4c7-1b0b-4b82-88f8-21d92fa425df","resolution":{"observed_at":"2026-08-06T18:34:11.982756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.08584","last_updated":"2023-07-17T15:55:46Z","snapshot_observed_at":"2026-08-19T04:00:18.140349Z","submitted_at":"2023-07-17T15:55:46Z","title":"Using spectral modeling to break light-curve degeneracies of type II supernovae interacting with circumstellar material","version":1},"cited_work":{"arxiv_id":"2307.08584","doi":"10.48550/arxiv.2307.08584","metadata_source":"arxiv_reference","pith_arxiv_id":"2307.08584","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"372555e6-1a1a-4f9e-ace1-e9c01885cb1a","year":null},"citing_paper":{"arxiv_id":"2605.21062","last_updated":"2026-05-20T11:46:03Z","snapshot_observed_at":"2026-08-15T16:45:29.141673Z","submitted_at":"2026-05-20T11:46:03Z","title":"Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models","version":1},"reference_index":208,"source":"arxiv_source","source_observed_at":"2026-05-21T02:13:20.739968Z"},"links":{"cited_paper":"/paper/2307.08584","citing_paper":"/paper/2605.21062"},"observation_digest":"sha256:59671b6f2d8c275caca59a8bf6b46da863c7e80044e790a3ff886e494241a5f3","observation_id":"fb9d1353-8a80-435d-af9f-c09a46d8cbe0","resolution":{"observed_at":"2026-05-21T02:13:54.829403Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-21T08:24:13.896857+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-21T08:24:13.896857+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.08584","last_updated":"2023-07-17T15:55:46Z","snapshot_observed_at":"2026-08-19T04:00:18.140349Z","submitted_at":"2023-07-17T15:55:46Z","title":"Using spectral modeling to break light-curve degeneracies of type II supernovae interacting with circumstellar material","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.08584","snapshot_observed_at":"2026-08-01T17:54:02.745467Z","title":"Dessart and W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.17488","last_updated":"2026-07-20T02:24:30Z","snapshot_observed_at":"2026-08-14T19:45:45.557457Z","submitted_at":"2026-07-20T02:24:30Z","title":"Surrogate models for type II supernovae: Probing low-energy explosions and interaction-free regimes","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-01T17:54:02.745467Z"},"links":{"cited_paper":"/paper/2307.08584","citing_paper":"/paper/2607.17488"},"observation_digest":"sha256:d9884b18b9bee03eacfc84cc92b39d9082f3de1a6fc5707c4242588db4eca7c8","observation_id":"91bd94f3-5ddd-44c5-8c67-5be9142866e0","resolution":{"observed_at":"2026-08-01T17:54:02.745467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.08584","last_updated":"2023-07-17T15:55:46Z","snapshot_observed_at":"2026-08-19T04:00:18.140349Z","submitted_at":"2023-07-17T15:55:46Z","title":"Using spectral modeling to break light-curve degeneracies of type II supernovae interacting with circumstellar material","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.08584","snapshot_observed_at":"2026-08-15T14:31:40.508915Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07455","last_updated":"2026-08-07T17:47:58Z","snapshot_observed_at":"2026-08-19T19:00:33.782038Z","submitted_at":"2026-08-07T17:47:58Z","title":"White Dwarf Kicks via Episodic Mass Ejection from Red Giant Stars","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-15T14:31:40.508915Z"},"links":{"cited_paper":"/paper/2307.08584","citing_paper":"/paper/2608.07455"},"observation_digest":"sha256:ad34c1197b7f595fc84ed235946aa8ef230713553b8da3d4eb00a4848dfb89d1","observation_id":"ac90c545-086f-4993-b076-6ac005fb4258","resolution":{"observed_at":"2026-08-15T14:31:40.508915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2307.08584/citation-record","integrity":"/paper/2307.08584/integrity","json":"/paper/2307.08584/citation-record.json","paper":"/paper/2307.08584"},"outbound":[],"paper":{"arxiv_id":"2307.08584","last_updated":"2023-07-17T15:55:46Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-19T04:00:18.140349Z","submitted_at":"2023-07-17T15:55:46Z","title":"Using spectral modeling to break light-curve degeneracies of type II supernovae interacting with circumstellar material"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2307.08584."}