{"as_of":"2026-08-11T04:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:becdea4330cb315f5518265cbdcc32d12b6f77a1ff09db36b39290e0ac8f1b4f","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T23:55:23.237270Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":41,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","snapshot_observed_at":"2026-08-11T03:27:21.030963Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.09055","snapshot_observed_at":"2026-07-13T16:48:58.103396Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-06T23:11:01.859050Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-13T16:48:58.103396Z"},"links":{"cited_paper":"/paper/1901.09055","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:e89f1305babdc24ef9ff05bb03aa711e7beec7fcdbb4e224a842a7409ca1c35c","observation_id":"db54359c-6f1d-4d03-8695-6d85f9c6ec99","resolution":{"observed_at":"2026-07-13T16:48:58.103396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","snapshot_observed_at":"2026-08-11T03:27:21.030963Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.09055","snapshot_observed_at":"2026-08-04T05:43:29.262089Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-06T23:11:01.859050Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.262089Z"},"links":{"cited_paper":"/paper/1901.09055","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:ca8dcb7526ea451731a91286555338229f8bedc4c6429f4d248635f4b1445865","observation_id":"8519bacb-5aea-4027-a9c5-cb56cf59d429","resolution":{"observed_at":"2026-08-04T05:43:29.262089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","snapshot_observed_at":"2026-08-11T03:27:21.030963Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","version":2},"cited_work":{"arxiv_id":"1901.09055","doi":"10.3847/1538-4357/ab1de2","metadata_source":"pith","pith_arxiv_id":"1901.09055","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","venue":"astro-ph.HE","work_id":"990fe6f4-b252-4f79-9d6a-c3115ac76ff4","year":2019},"citing_paper":{"arxiv_id":"2605.04896","last_updated":"2026-05-06T13:27:04Z","snapshot_observed_at":"2026-07-30T01:39:37.333910Z","submitted_at":"2026-05-06T13:27:04Z","title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-08T15:59:11.556246Z"},"links":{"cited_paper":"/paper/1901.09055","citing_paper":"/paper/2605.04896"},"observation_digest":"sha256:e334dc2499f3a5b5e5a19dbd6ee189d50f85a7acee2a92dfbb8af9f99a882868","observation_id":"d5595b12-0005-4b06-bbc5-0be1d037f80a","resolution":{"observed_at":"2026-07-04T23:45:06.107090Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","snapshot_observed_at":"2026-08-11T03:27:21.030963Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","version":2},"cited_work":{"arxiv_id":"1901.09055","doi":"10.3847/1538-4357/ab1de2","metadata_source":"pith","pith_arxiv_id":"1901.09055","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","venue":"astro-ph.HE","work_id":"990fe6f4-b252-4f79-9d6a-c3115ac76ff4","year":2019},"citing_paper":{"arxiv_id":"2607.06664","last_updated":"2026-07-07T18:00:01Z","snapshot_observed_at":"2026-08-07T09:00:48.980402Z","submitted_at":"2026-07-07T18:00:01Z","title":"Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors","version":1},"reference_index":164,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1901.09055","citing_paper":"/paper/2607.06664"},"observation_digest":"sha256:b0f0a66e0b4984a3d08b6b9084994bbc943f18c1868d50e1dbe3794081bf7beb","observation_id":"7a54aa08-5370-4a41-94b8-e352609a5ae8","resolution":{"observed_at":"2026-07-10T23:57:49.142897Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","snapshot_observed_at":"2026-08-11T03:27:21.030963Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.09055","snapshot_observed_at":"2026-08-04T23:55:23.237270Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.01634","last_updated":"2026-08-03T03:07:09Z","snapshot_observed_at":"2026-08-08T11:57:25.120642Z","submitted_at":"2026-08-03T03:07:09Z","title":"Parameter Estimation Horizon of Core-Collapse Supernovae with a Network of Gravitational-Wave Detectors","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T23:55:23.237270Z"},"links":{"cited_paper":"/paper/1901.09055","citing_paper":"/paper/2608.01634"},"observation_digest":"sha256:04a180d1ed2c18aa79fdb617a9102baadfceefefeae60c8c1c3ef86760d1f034","observation_id":"e93c748e-144a-44f4-8f0a-7d39293359b5","resolution":{"observed_at":"2026-08-04T23:55:23.237270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1901.09055/citation-record","integrity":"/paper/1901.09055/integrity","json":"/paper/1901.09055/citation-record.json","paper":"/paper/1901.09055"},"outbound":[],"paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-11T03:27:21.030963Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1901.09055."}