{"as_of":"2026-08-10T13:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:29f6e64e3d1856b077ccb2b7e6f22900a7bfeb965a19be8621fa40b281da6f3c","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":"2026-08-10T06:31:04.303077+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":"2026-08-09T00:07:29.675638Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T21:58:59.601845Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2104.13672","last_updated":"2022-07-27T16:01:57Z","snapshot_observed_at":"2026-08-10T03:43:48.188481Z","submitted_at":"2021-04-28T09:51:45Z","title":"Models of binary neutron star remnants with tabulated equations of state","version":3},"cited_work":{"arxiv_id":"2104.13672","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.13672","snapshot_observed_at":"2026-07-03T21:58:59.601845Z","title":"Iosif and N","venue":null,"work_id":"3de79caa-d443-4374-acd8-4a9776a087d0","year":2022},"citing_paper":{"arxiv_id":"2409.10508","last_updated":"2025-02-20T10:17:01Z","snapshot_observed_at":"2026-07-06T19:16:14.638445Z","submitted_at":"2024-09-16T17:54:10Z","title":"General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-23T20:56:06.983493Z"},"links":{"cited_paper":"/paper/2104.13672","citing_paper":"/paper/2409.10508"},"observation_digest":"sha256:58ef75800112876a5c68ae4ab0a66678ae70cd2a20761821fdd010583aca6f1f","observation_id":"52a0a28b-b6e9-4f5b-b016-92c1fa990802","resolution":{"observed_at":"2026-05-09T04:41:37.842941Z","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":"2104.13672","last_updated":"2022-07-27T16:01:57Z","snapshot_observed_at":"2026-08-10T03:43:48.188481Z","submitted_at":"2021-04-28T09:51:45Z","title":"Models of binary neutron star remnants with tabulated equations of state","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.13672","snapshot_observed_at":"2026-08-09T00:07:29.675638Z","title":"Iosif and N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03973","last_updated":"2025-02-06T11:06:13Z","snapshot_observed_at":"2026-08-09T05:48:47.263112Z","submitted_at":"2025-02-06T11:06:13Z","title":"Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-09T00:07:29.675638Z"},"links":{"cited_paper":"/paper/2104.13672","citing_paper":"/paper/2502.03973"},"observation_digest":"sha256:e05fb43b9c792f7479e7443c961c9b967f4b3308acac41e24a9717e573796326","observation_id":"eb2e1576-68fa-4517-8dbb-a2d3f389f25b","resolution":{"observed_at":"2026-08-09T00:07:29.675638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.13672","last_updated":"2022-07-27T16:01:57Z","snapshot_observed_at":"2026-08-10T03:43:48.188481Z","submitted_at":"2021-04-28T09:51:45Z","title":"Models of binary neutron star remnants with tabulated equations of state","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.13672","snapshot_observed_at":"2026-08-04T18:11:12.479782Z","title":"Iosif and N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.10150","last_updated":"2025-09-12T11:25:29Z","snapshot_observed_at":"2026-08-09T15:23:20.807467Z","submitted_at":"2025-09-12T11:25:29Z","title":"Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-04T18:11:12.479782Z"},"links":{"cited_paper":"/paper/2104.13672","citing_paper":"/paper/2509.10150"},"observation_digest":"sha256:b708491600d4c642eb11b9f1382d0944ed94a3f82b46f95c6228a6c450fca472","observation_id":"523e2769-75ec-4407-b654-13973ae6b40c","resolution":{"observed_at":"2026-08-04T18:11:12.479782Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.13672","last_updated":"2022-07-27T16:01:57Z","snapshot_observed_at":"2026-08-10T03:43:48.188481Z","submitted_at":"2021-04-28T09:51:45Z","title":"Models of binary neutron star remnants with tabulated equations of state","version":3},"cited_work":{"arxiv_id":"2104.13672","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.13672","snapshot_observed_at":"2026-07-03T21:58:59.601845Z","title":"Iosif and N","venue":null,"work_id":"3de79caa-d443-4374-acd8-4a9776a087d0","year":2022},"citing_paper":{"arxiv_id":"2606.17875","last_updated":"2026-06-16T12:47:17Z","snapshot_observed_at":"2026-07-06T23:53:25.839293Z","submitted_at":"2026-06-16T12:47:17Z","title":"Hybrid Stars with Post-Merger Rotation Profiles","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-06-26T23:50:12.361235Z"},"links":{"cited_paper":"/paper/2104.13672","citing_paper":"/paper/2606.17875"},"observation_digest":"sha256:dd6cf32caa304ef8d37fab42f4507cb6c299cddd11c05d9cea7f3b19b57dce6f","observation_id":"968ccab2-3893-4e96-a335-fabb3dec065a","resolution":{"observed_at":"2026-07-03T21:58:59.603389Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2104.13672/citation-record","integrity":"/paper/2104.13672/integrity","json":"/paper/2104.13672/citation-record.json","paper":"/paper/2104.13672"},"outbound":[],"paper":{"arxiv_id":"2104.13672","last_updated":"2022-07-27T16:01:57Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-10T03:43:48.188481Z","submitted_at":"2021-04-28T09:51:45Z","title":"Models of binary neutron star remnants with tabulated equations of state"},"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 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2104.13672."}