{"as_of":"2026-08-15T03:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:885d694702fd7e287ac6742b1a6d7f1a358f1779706c977ae45e188a946d65f7","coverage":[{"denominator":86,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":86,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T10:30:45.219142Z","state":"measured"},{"denominator":87,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":87,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-26T23:50:12.361235Z","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":"2026-07-03T22:08:58.814793Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"cited_work":{"arxiv_id":"1908.11258","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.11258","snapshot_observed_at":"2026-07-03T22:08:58.814793Z","title":"Camelio, T","venue":null,"work_id":"8eb0e379-67b9-4686-a94e-16d96c46bf3e","year":2019},"citing_paper":{"arxiv_id":"2606.17875","last_updated":"2026-06-16T12:47:17Z","snapshot_observed_at":"2026-08-14T11:31:14.463912Z","submitted_at":"2026-06-16T12:47:17Z","title":"Hybrid Stars with Post-Merger Rotation Profiles","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-26T23:50:12.361235Z"},"links":{"cited_paper":"/paper/1908.11258","citing_paper":"/paper/2606.17875"},"observation_digest":"sha256:4d2b6572307daa169a4c7b7e280069f7c03a2e83f00bb0f17fb6659e6b42db94","observation_id":"7cd5b759-9ec1-410d-8597-d4d41eebeae7","resolution":{"observed_at":"2026-07-03T22:08:58.816648Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1908.11258/citation-record","integrity":"/paper/1908.11258/integrity","json":"/paper/1908.11258/citation-record.json","paper":"/paper/1908.11258"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.913910Z","title":"Otherwise, determine Ω from Eq","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.913910Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:4f7e74816495e1e1c7e7384a7d231d1c56f192994ca883711e61e598fdca3d05","observation_id":"4095b468-239c-43b9-924f-320a781f8bb8","resolution":{"observed_at":"2026-08-14T10:30:44.913910Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.908933Z","title":"barotropic","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.908933Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ee8848d76ce9c7eff0fc666f1fbc98b89d3fb4c8edd39a606ffd8fd5d3fe3ba0","observation_id":"8a4dacfc-886a-49e3-bc72-8e639ba14fcb","resolution":{"observed_at":"2026-08-14T10:30:44.908933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.917213Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.917213Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:3bed58438ac0ce94801e95d4f4a0da4a4c4c4a87a8ab43c7620abed14159f4ed","observation_id":"c1d4e5af-33e7-4e99-ad90-2ac1a73caefa","resolution":{"observed_at":"2026-08-14T10:30:44.917213Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.920749Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.920749Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:f633f97840da0a3e6e54cfe65a8a99dbae467b3acb705b1388337f459280d09c","observation_id":"2f8ffda1-3190-4bc0-ad19-42533f2d3c57","resolution":{"observed_at":"2026-08-14T10:30:44.920749Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.924935Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.924935Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:2e50286fd3f2c1131c193d611b05e39c5667d9f5a02fe2775afe10ad99020ba2","observation_id":"de01c013-30b2-455e-8124-d6208aec82d1","resolution":{"observed_at":"2026-08-14T10:30:44.924935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.928613Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.928613Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:2fa8af8f29215aac6c3bc3703d8fa0dfb483fc564d422da72be33b7aca43c29f","observation_id":"a5495391-ed50-4bae-8d95-16c3cb786ef3","resolution":{"observed_at":"2026-08-14T10:30:44.928613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.326807Z","title":"Solve the EOS from p (if barotropic) or p, h (if non barotropic)","venue":null,"work_id":"017943db-8df8-41a2-99dd-4612b0b6de8f","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.932394Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:0bd5dc336ad1975ce016e1ede9db53e67c8f73f0c79f1c042c1a1ee2bd685eb2","observation_id":"b92dc603-1d6f-41db-bbd9-49c3632179fd","resolution":{"observed_at":"2026-08-14T10:30:46.330494Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.316166Z","title":null,"venue":null,"work_id":"075c400a-cdec-4dad-890d-641890eb6c74","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.935665Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:4b45b63cbd76b1458c120932f57b925e1d073f16ac2a70799daf875b90c266ba","observation_id":"5f571048-e059-4400-a1db-cc4bc3f6204e","resolution":{"observed_at":"2026-08-14T10:30:46.320117Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.304570Z","title":"same as above","venue":null,"work_id":"230e5287-0693-4cbc-92b5-b0fddfb881a8","year":2000},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.938751Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:e0747599ee069f09a2c7cd343ad7d361f4de694356bc721a0fa552c9c1782f13","observation_id":"ff42131b-7d29-44a8-8e10-054d8c301a12","resolution":{"observed_at":"2026-08-14T10:30:46.309074Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.292833Z","title":"The vice versa is also true","venue":null,"work_id":"7b66a8b3-e05a-4707-8437-fa4402b6ecd4","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.942740Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:b11251de39ff79e875cf6ef4a47b5254845e7356489bc74870e8bf0e64598d7f","observation_id":"5dff556a-fd16-47c8-81c6-7c5d5e663bc9","resolution":{"observed_at":"2026-08-14T10:30:46.296504Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.281955Z","title":null,"venue":null,"work_id":"255dce80-e3a3-4528-926c-77c739644d2f","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.946008Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:c2eb7c966e51c77e55cb477da94295745065bff8d423652ac807a422f683c5fd","observation_id":"701280f6-a96e-43b6-a896-e494937b0fec","resolution":{"observed_at":"2026-08-14T10:30:46.285855Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.271046Z","title":"However, this is not true in general for a non-barotropic star (but it is for the non-barotropic cases considered in this work) [18, 19, 21, 23, 24, 26]","venue":null,"work_id":"4b75e82f-1dbe-41e6-ab04-8c087773478d","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.949062Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ce55ff1f077622520f61c448c2694456771e84d06ccb55d10ccf2eec68569b3d","observation_id":"b1bd78cb-44d2-40da-9847-319248228ed3","resolution":{"observed_at":"2026-08-14T10:30:46.274880Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.260094Z","title":"III is that there are only two EOS quantities that can be directly determined from the Euler equation with- out solving the EOS, namely p and h","venue":null,"work_id":"fe838325-7081-42b6-bdca-17b6c771b564","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.952627Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:fcbbfbc4d42a97b45c2618a9bfd0a989d971b04ae1ce56f5ef6e732b45b6215f","observation_id":"0e9b0379-0154-402a-8809-d0bda66e5b2e","resolution":{"observed_at":"2026-08-14T10:30:46.264050Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.249042Z","title":null,"venue":null,"work_id":"2a925f8f-6cea-4bd8-be05-b1ecf5cca0eb","year":null},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.955960Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:a3efa1ef8401659ca4a6fb26ec035d1a9872b4a552bbf5cf56b34183d23f1236","observation_id":"7464859a-5112-4abf-9b19-9f8158fcc0ea","resolution":{"observed_at":"2026-08-14T10:30:46.252687Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.238841Z","title":"including viscosity [24]","venue":null,"work_id":"a4bf5356-4922-4fd0-a911-fceb852cd453","year":2020},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.959197Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:8261cfade8eee8b1b2829e2fb3f5ffb77c8c46f73d794601584ba29f2a513151","observation_id":"24b40de2-e18a-4005-98a7-d00fd66fc89a","resolution":{"observed_at":"2026-08-14T10:30:46.242347Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1305.3510","last_updated":"2013-05-15T14:59:02Z","snapshot_observed_at":"2026-08-15T00:17:45.363808Z","submitted_at":"2013-05-15T14:59:02Z","title":"The Nuclear Equation of State and Neutron Star Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.3510","snapshot_observed_at":"2026-08-14T10:30:44.964501Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.964501Z"},"links":{"cited_paper":"/paper/1305.3510","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ebdd98b210dc4a53a8b1ef54a9a546f3ee82a3090e91485fdfde7cdf5cc4054c","observation_id":"19196ca8-b022-4f3f-b2c4-b79d9fb047e7","resolution":{"observed_at":"2026-08-14T10:30:44.964501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.07820","last_updated":"2015-12-24T14:09:54Z","snapshot_observed_at":"2026-08-14T22:17:04.532643Z","submitted_at":"2015-12-24T14:09:54Z","title":"The Equation of State of Hot, Dense Matter and Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.07820","snapshot_observed_at":"2026-08-14T10:30:44.968450Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.968450Z"},"links":{"cited_paper":"/paper/1512.07820","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:e5aabd72cc481ecf5013c5857ceebed0d53e0b63ef1b2ce471e4ad90581bba5d","observation_id":"1b08d1a5-f7c9-414a-b46a-60b4af13e310","resolution":{"observed_at":"2026-08-14T10:30:44.968450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-14T19:09:49.769515Z","submitted_at":"2018-05-29T16:56:13Z","title":"GW170817: Measurements of Neutron Star Radii and Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11581","snapshot_observed_at":"2026-08-14T10:30:44.972295Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.972295Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bf9b27137f84ef9d49c39c2e2aaf9d4845402cba598e389bbd57dfe178fc9cb7","observation_id":"f7a068bf-9608-4da5-a0fe-9bd63483bdda","resolution":{"observed_at":"2026-08-14T10:30:44.972295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07898","last_updated":"2019-03-19T09:24:25Z","snapshot_observed_at":"2026-08-15T01:01:02.799035Z","submitted_at":"2019-03-19T09:24:25Z","title":"Thermodynamics conditions of matter in neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07898","snapshot_observed_at":"2026-08-14T10:30:44.976404Z","title":"Perego, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.976404Z"},"links":{"cited_paper":"/paper/1903.07898","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:49fe222fa44677f88ceb7a3bc097436db778de3a5c62e6299943638f3cd6d569","observation_id":"14c69457-7939-4e94-b02e-dfecb1240f84","resolution":{"observed_at":"2026-08-14T10:30:44.976404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.3409","last_updated":"2011-04-14T09:41:16Z","snapshot_observed_at":"2026-08-05T02:08:27.962255Z","submitted_at":"2010-11-10T16:31:00Z","title":"Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.3409","snapshot_observed_at":"2026-08-14T10:30:44.980232Z","title":"Fischer, I","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.980232Z"},"links":{"cited_paper":"/paper/1011.3409","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:3b809d78b67cb232fb9e6502f88264f9062cfb0b65ec74d6ff64d9fbf894ecb2","observation_id":"8eb30560-2448-401e-a304-5d4388291ffc","resolution":{"observed_at":"2026-08-14T10:30:44.980232Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.984139Z","title":"Punturo et al., Class","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.984139Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:956c04c80dfb81e3254611da61e726f47e556b3e124e785d33c4fc598545cd71","observation_id":"9ea5f1f4-2e4c-4732-bf8f-8bce0a8f1411","resolution":{"observed_at":"2026-08-14T10:30:44.984139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:44.987196Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.987196Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:04ebf72f55c6a46039dd2cd4232fa016ca1291c0db9e3dc3be76c9ea869068b0","observation_id":"3a8d4ca7-e2f6-4c1b-bba1-1d877743ed06","resolution":{"observed_at":"2026-08-14T10:30:44.987196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-14T10:30:44.990546Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.990546Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:18cb35708ff0ebcc632abc66cb338bd11093d7fbf2fd152ebf6040d8f610e9a8","observation_id":"642bb8fe-dce6-4ae6-a4e8-705d7db07688","resolution":{"observed_at":"2026-08-14T10:30:44.990546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05833","last_updated":"2017-10-24T12:03:18Z","snapshot_observed_at":"2026-08-14T20:23:19.773859Z","submitted_at":"2017-10-16T16:57:18Z","title":"Multi-messenger Observations of a Binary Neutron Star Merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05833","snapshot_observed_at":"2026-08-14T10:30:44.994149Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.994149Z"},"links":{"cited_paper":"/paper/1710.05833","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:8fdf9af1037d46d1150bd34b06a2f586e7686a6720f30af2206614ffd34d0e11","observation_id":"3405f6d0-b347-40dc-a495-d00ec9117705","resolution":{"observed_at":"2026-08-14T10:30:44.994149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05452","last_updated":"2017-10-16T16:57:35Z","snapshot_observed_at":"2026-08-14T20:23:19.381034Z","submitted_at":"2017-10-16T16:57:35Z","title":"Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05452","snapshot_observed_at":"2026-08-14T10:30:44.997608Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:44.997608Z"},"links":{"cited_paper":"/paper/1710.05452","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:7b4e1d8351ec2312a3073463005dc1447020b39a090927972a4f302d7679cd26","observation_id":"c256200c-4f4d-41b6-ab87-c85f7bfcda6a","resolution":{"observed_at":"2026-08-14T10:30:44.997608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.222293Z","title":"Burrows, Astrophys","venue":null,"work_id":"7bda4fad-e42a-4f74-be7b-47e17c33f85a","year":1988},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.001540Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bc01e1fe68d2faf5afee21d64462dc9014045b77ff8c45c55639688448d7e508","observation_id":"5551ecf6-27fd-4e4f-86d2-869d586a2086","resolution":{"observed_at":"2026-08-14T10:30:46.226522Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.212711Z","title":"Bonazzola, E","venue":null,"work_id":"77e652e3-3b5f-4af3-852e-48a67f644d4a","year":1993},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.004902Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:a6677d81ba23965e337c9422a1e1e62d531a853c62204164b21bd57bef04c7ea","observation_id":"132498b2-8708-4b88-93d8-fa73454efcc1","resolution":{"observed_at":"2026-08-14T10:30:46.216107Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9610265","last_updated":"1996-10-31T23:02:10Z","snapshot_observed_at":"2026-08-10T10:17:28.548010Z","submitted_at":"1996-10-31T23:02:10Z","title":"Rapid uniform rotation of protoneutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9610265","snapshot_observed_at":"2026-08-14T10:30:45.008379Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.008379Z"},"links":{"cited_paper":"/paper/astro-ph/9610265","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:7565c1bc255d3708c17b1c1fcf4267e76377d0c2de4bae42fbfc5eeac91db024","observation_id":"27b83a46-5cc0-4d2e-b30a-6a4abda491e2","resolution":{"observed_at":"2026-08-14T10:30:45.008379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.3532","last_updated":"2011-01-26T11:35:52Z","snapshot_observed_at":"2026-07-06T02:17:48.132379Z","submitted_at":"2010-10-18T09:35:29Z","title":"GRMHD in axisymmetric dynamical spacetimes: the X-ECHO code","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.3532","snapshot_observed_at":"2026-08-14T10:30:45.012212Z","title":"Bucciantini and L","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.012212Z"},"links":{"cited_paper":"/paper/1010.3532","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:6d8e405df3595a0bbf3729e6e8ff68ae2ff3768f071e1ea232909e12fb3c36dc","observation_id":"fb683243-1a72-44e6-baea-dc1bd8913bf5","resolution":{"observed_at":"2026-08-14T10:30:45.012212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.4308","last_updated":"2014-02-06T12:25:23Z","snapshot_observed_at":"2026-08-14T23:48:01.680040Z","submitted_at":"2014-01-17T11:09:34Z","title":"Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.4308","snapshot_observed_at":"2026-08-14T10:30:45.015921Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.015921Z"},"links":{"cited_paper":"/paper/1401.4308","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:534a256f87fa4c776a0ae4f6acb37201da8bf393f7cec1fc485a65a592887581","observation_id":"71281088-bbba-4557-86ea-2629d7f4d2fd","resolution":{"observed_at":"2026-08-14T10:30:45.015921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.07775","last_updated":"2018-08-10T15:26:49Z","snapshot_observed_at":"2026-08-14T19:01:25.363633Z","submitted_at":"2018-06-20T14:52:35Z","title":"Disk formation in the collapse of supramassive neutron stars","version":3},"cited_work":{"arxiv_id":"1806.07775","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.07775","snapshot_observed_at":"2026-08-14T10:30:45.857910Z","title":"Disk formation in the collapse of supramassive neutron stars","venue":"astro-ph.HE","work_id":"1e055d7c-ec2b-4989-b7b1-9a6032c8e9a5","year":2018},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.019516Z"},"links":{"cited_paper":"/paper/1806.07775","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:b1ab43ac80753ba8fdbf8d508e29ccabf5bda85e81fcb035ad42c1a243f0606e","observation_id":"56264f38-8cf9-4775-bdb3-214c2792e2a1","resolution":{"observed_at":"2026-08-14T10:30:45.862980Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.202055Z","title":null,"venue":null,"work_id":"50a44e76-2954-4bd3-b45c-4dfeb9f07851","year":1966},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.023217Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ee814b5636c29dd8e1daeba57761f92f9883f66aa73c87a8b6c716d5ac7be536","observation_id":"968f5b6f-1147-4eb5-a501-59fcea34758e","resolution":{"observed_at":"2026-08-14T10:30:46.206119Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.192679Z","title":null,"venue":null,"work_id":"27db1b60-d004-4be7-adbe-514b462f92ff","year":1969},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.026577Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ff4c3303cc88658478d5aa155cb5b25e8ba2237c5b104d1bf789d4edcf0492a1","observation_id":"d121dd7d-2212-45b5-af56-9b1f4f57c9e3","resolution":{"observed_at":"2026-08-14T10:30:46.195942Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.182825Z","title":null,"venue":null,"work_id":"41e28913-ba54-4e12-866b-c7998768b99f","year":1971},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.030245Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:d26e24d98a9cc48eeb7efa091cd68d4386bbe684f620b6e5ef2f4f7f16a13756","observation_id":"72038974-e73f-48e9-8f1b-d963371e4f68","resolution":{"observed_at":"2026-08-14T10:30:46.186030Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.172827Z","title":null,"venue":null,"work_id":"4e1ae3ab-785e-46e5-930d-661bc0437044","year":1977},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.033668Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:2b66696682dc46fc4bb52ca53431d735ed5c468782e17a656308acfd70fcc66a","observation_id":"3190285c-5a09-4b08-abfd-d29bae22267f","resolution":{"observed_at":"2026-08-14T10:30:46.176089Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.162083Z","title":"Uryu and Y","venue":null,"work_id":"1a919f07-e5af-4c36-9fe0-77b7a4be5bdd","year":1994},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.036968Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:1a9c28f6bcc45aa0516eb8bbd5cf49fda2bea06aa4076e5586d57cbe4b980668","observation_id":"43c2bb56-f257-49ae-a919-2ae25afd85b9","resolution":{"observed_at":"2026-08-14T10:30:46.166160Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.151453Z","title":null,"venue":null,"work_id":"019ba25f-0f37-4792-af26-67a142e55a7f","year":2006},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.040325Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:5118326a6067cd34b4970fec9758feb3739ad707c4ef07484a9b2d8855ea17c8","observation_id":"000fb4c2-c9d7-4479-9dc0-7fb9773f1d18","resolution":{"observed_at":"2026-08-14T10:30:46.154960Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.140767Z","title":"Espinosa Lara and M","venue":null,"work_id":"f68c4ffb-a444-472c-8e60-6fa85207757c","year":2007},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.043846Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:b77279ca935ba9b406d2fd1a6f976decd0b782af860f5d630c38431ade7678c8","observation_id":"0134004a-3a63-4b5f-a54b-a6c4ec8ac0fb","resolution":{"observed_at":"2026-08-14T10:30:46.144186Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1212.0778","last_updated":"2013-03-19T13:03:01Z","snapshot_observed_at":"2026-08-15T00:37:10.546480Z","submitted_at":"2012-12-04T16:16:56Z","title":"Self-consistent 2D models of fast rotating early-type star","version":2},"cited_work":{"arxiv_id":"1212.0778","doi":null,"metadata_source":"pith","pith_arxiv_id":"1212.0778","snapshot_observed_at":"2026-08-14T10:30:45.844609Z","title":"Self-consistent 2D models of fast rotating early-type star","venue":"astro-ph.SR","work_id":"b63c484b-41c1-4f5f-9138-204049470140","year":2012},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.047172Z"},"links":{"cited_paper":"/paper/1212.0778","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bb0b7dad5772ef6221f87f6a1c18f3cf435ea088642104db33695fd7e6238af4","observation_id":"c5a9b6e4-92ef-4fe3-9bfe-935a690ce3cd","resolution":{"observed_at":"2026-08-14T10:30:45.848779Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1402.4567","last_updated":"2014-11-19T08:00:07Z","snapshot_observed_at":"2026-08-14T23:44:09.829923Z","submitted_at":"2014-02-19T06:48:33Z","title":"A Novel Formulation by Lagrangian Variational Principle for Rotational Equilibria: Toward Multi-Dimensional Stellar Evolutions","version":3},"cited_work":{"arxiv_id":"1402.4567","doi":null,"metadata_source":"pith","pith_arxiv_id":"1402.4567","snapshot_observed_at":"2026-08-14T10:30:45.830799Z","title":"A Novel Formulation by Lagrangian Variational Principle for Rotational Equilibria: Toward Multi-Dimensional Stellar Evolutions","venue":"astro-ph.SR","work_id":"c4ffd818-74e9-431a-8a02-7efa23f70b65","year":2014},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.050621Z"},"links":{"cited_paper":"/paper/1402.4567","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ce3d605f61de989e14a400f17ee9542512a111a916fee5dc4c4058321b7391aa","observation_id":"324873a3-bd0d-4fbe-be21-2df75bd51b61","resolution":{"observed_at":"2026-08-14T10:30:45.834995Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.02693","last_updated":"2015-10-20T02:59:18Z","snapshot_observed_at":"2026-08-14T22:41:02.421810Z","submitted_at":"2015-07-09T20:02:03Z","title":"A versatile numerical method for obtaining structures of rapidly rotating baroclinic stars: self-consistent and systematic solutions with shellular-type rotation","version":2},"cited_work":{"arxiv_id":"1507.02693","doi":null,"metadata_source":"pith","pith_arxiv_id":"1507.02693","snapshot_observed_at":"2026-08-14T10:30:45.816521Z","title":"A versatile numerical method for obtaining structures of rapidly rotating baroclinic stars: self-consistent and systematic solutions with shellular-type rotation","venue":"astro-ph.SR","work_id":"cf5c9ade-d024-4586-8e8d-030d0672b3ef","year":2015},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.053829Z"},"links":{"cited_paper":"/paper/1507.02693","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:571c42f6bc64fb7d553f133e92a91322299e664c6dca99fa07ee0707c4542689","observation_id":"00676bac-d21d-428b-b92a-784f4a0dd034","resolution":{"observed_at":"2026-08-14T10:30:45.820730Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.130128Z","title":"Amendt, A","venue":null,"work_id":"d331ef37-8525-46ba-ae8f-323ef73e13ce","year":1989},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.057397Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:48ed027fd1d4c84cbb5a2bdc55e097ce56430500740915057535d039f2f14700","observation_id":"5ea8bb21-b324-42fb-a77c-26ea8f90091f","resolution":{"observed_at":"2026-08-14T10:30:46.134064Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.08716","last_updated":"2017-08-29T12:07:29Z","snapshot_observed_at":"2026-08-14T20:38:12.179605Z","submitted_at":"2017-08-29T12:07:29Z","title":"Analytic construction of baroclinic tori by non-linear summation","version":1},"cited_work":{"arxiv_id":"1708.08716","doi":null,"metadata_source":"pith","pith_arxiv_id":"1708.08716","snapshot_observed_at":"2026-08-14T10:30:45.802019Z","title":"Analytic construction of baroclinic tori by non-linear summation","venue":"astro-ph.HE","work_id":"9ebd5e65-1236-4dbf-a0cc-c5241cde1781","year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.060605Z"},"links":{"cited_paper":"/paper/1708.08716","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bb19ed492afcd9092065137ab7598f1b11e6151ad4335c3e7cc7be915c412cef","observation_id":"f5765c82-eb1a-411a-b0bf-6153a36a3ecb","resolution":{"observed_at":"2026-08-14T10:30:45.806036Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.118873Z","title":null,"venue":null,"work_id":"d8cbc336-f990-4e61-8dae-c8a86b323eb2","year":1970},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.064301Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:cfc204c312d9be75fb83746bfa9b017ff931099c973a44652679ac9c38d4f3f8","observation_id":"7251dd1f-d100-487e-86dc-7e756d9dedaf","resolution":{"observed_at":"2026-08-14T10:30:46.122637Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.107908Z","title":"Stergioulas, Living Reviews in Relativity 6, 3 (2003), ISSN 1433-8351, URL https://doi.org/10","venue":null,"work_id":"1ed24b57-7bd1-47b7-9616-9ab797d9522a","year":2003},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.068042Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:01eac9917865af6c073af7aac5c278107112854d83c5e6036d7cf0c2cda74404","observation_id":"3f66aa9f-bca3-4ce1-972e-c8edca2b17cd","resolution":{"observed_at":"2026-08-14T10:30:46.111685Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.071493Z","title":"Komatsu, Y","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.071493Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:fa4417b22bf44c302f5d8c4d8586e45373b14c8e1548bcba904df032e3b93303","observation_id":"0b3b869a-1e61-4d28-8ea7-aee6a2c025dd","resolution":{"observed_at":"2026-08-14T10:30:45.071493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.02643","last_updated":"2017-11-28T09:42:53Z","snapshot_observed_at":"2026-08-15T01:04:15.670008Z","submitted_at":"2017-09-08T10:55:46Z","title":"Modeling differential rotations of compact stars in equilibriums","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.02643","snapshot_observed_at":"2026-08-14T10:30:45.074876Z","title":"Ury¯ u, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.074876Z"},"links":{"cited_paper":"/paper/1709.02643","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:68316c95bd9c132c357f22b239e96fbf080c0002621483e3d414be09365b30bf","observation_id":"82021f0b-21ad-4780-8031-927d700893a4","resolution":{"observed_at":"2026-08-14T10:30:45.074876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.091042Z","title":"Witzany and P","venue":null,"work_id":"13a2b314-a1a3-4916-8d42-93dc7b9d54f4","year":2019},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.078373Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:82a672c4552d66198d18e05e5708ebe92008c2a05d495986c261d70c30a87793","observation_id":"6813f9b2-6976-4f30-adbf-e648e0c8f74b","resolution":{"observed_at":"2026-08-14T10:30:46.094616Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0310875","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.775863Z","title":"Villain, J","venue":null,"work_id":"4489dd3f-aa73-4943-9486-a8d25c954ba8","year":2004},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.081694Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:1e2a38c8ff8cfc51807cf833d5061914f2792d225267bf22935f6e31d63325fd","observation_id":"6864e208-7b1e-47d9-b4e2-3baaff97b07d","resolution":{"observed_at":"2026-08-14T10:30:45.780797Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0809.2325","last_updated":"2009-01-23T18:25:40Z","snapshot_observed_at":"2026-08-12T05:28:45.986844Z","submitted_at":"2008-09-13T10:46:25Z","title":"Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.2325","snapshot_observed_at":"2026-08-14T10:30:45.085451Z","title":"Cordero-Carri´ on, P","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.085451Z"},"links":{"cited_paper":"/paper/0809.2325","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:763af09d74b91f257e46d167153462c87e616a606988ad79b1da1a9d95ca7510","observation_id":"875b2437-7c4e-417f-98a5-cbbbcece5052","resolution":{"observed_at":"2026-08-14T10:30:45.085451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.5015","last_updated":"2011-09-20T14:53:24Z","snapshot_observed_at":"2026-08-13T14:48:48.407124Z","submitted_at":"2010-03-25T23:17:44Z","title":"An introduction to the theory of rotating relativistic stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.5015","snapshot_observed_at":"2026-08-14T10:30:45.089039Z","title":"Gourgoulhon, arXiv e-prints arXiv:1003.5015 (2010), 1003.5015","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.089039Z"},"links":{"cited_paper":"/paper/1003.5015","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:3bd3f80144ebd614c4a0cb8927bd94259ff5c6eb08159ba8fd8f9e0e76272fe2","observation_id":"7f57ebd2-79ad-457e-9422-e5dc435cdadf","resolution":{"observed_at":"2026-08-14T10:30:45.089039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.7375","last_updated":"2014-09-10T12:34:50Z","snapshot_observed_at":"2026-08-14T23:28:44.363098Z","submitted_at":"2014-06-28T09:15:53Z","title":"On the accuracy of the IWM-CFC approximation in differentially rotating relativistic stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.7375","snapshot_observed_at":"2026-08-14T10:30:45.092726Z","title":"Iosif and N","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.092726Z"},"links":{"cited_paper":"/paper/1406.7375","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:c9e230c590077faebc7344a1e02e42b83690e1331061e4a40cc98a1bc4847205","observation_id":"975e878d-c6f1-47ae-9009-19b4db048cd6","resolution":{"observed_at":"2026-08-14T10:30:45.092726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9411032","last_updated":"1994-11-08T16:22:58Z","snapshot_observed_at":"2026-07-07T01:10:17.952412Z","submitted_at":"1994-11-08T16:22:58Z","title":"Comparing Models of Rapidly Rotating Relativistic Stars Constructed by Two Numerical Methods","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9411032","snapshot_observed_at":"2026-08-14T10:30:45.096445Z","title":"Stergioulas and J","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.096445Z"},"links":{"cited_paper":"/paper/astro-ph/9411032","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ee3c0cb636be15de43ff926c4414e5b80a4e7899a4d9b53d0815832fe806d2a1","observation_id":"7f67dc93-caac-4f69-a388-e4d4496cd6ce","resolution":{"observed_at":"2026-08-14T10:30:45.096445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0312112","last_updated":"2004-05-12T17:22:57Z","snapshot_observed_at":"2026-07-07T03:18:39.687978Z","submitted_at":"2003-12-26T16:53:57Z","title":"Numerical simulation of orbiting black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0312112","snapshot_observed_at":"2026-08-14T10:30:45.100259Z","title":"Br¨ ugmann, W","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.100259Z"},"links":{"cited_paper":"/paper/gr-qc/0312112","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:40c0ecdcea1ce418d7880662e8eed8beab6589860271f3917da789ac4f81920d","observation_id":"b8d83319-4d57-4f58-b12b-bf8759c6c0cb","resolution":{"observed_at":"2026-08-14T10:30:45.100259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.104103Z","title":"Br¨ ugmann, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.104103Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:7f2706ea0d54ede10c48e3eed6d4f35c6232e8701b4b3b20a28077dae4e41f3d","observation_id":"31e14b21-645b-43d7-aa54-054057b78680","resolution":{"observed_at":"2026-08-14T10:30:45.104103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.4751","last_updated":"2011-08-11T09:46:12Z","snapshot_observed_at":"2026-08-10T14:54:20.028364Z","submitted_at":"2011-04-25T16:51:36Z","title":"Numerical relativity simulations of binary neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.4751","snapshot_observed_at":"2026-08-14T10:30:45.107746Z","title":"Thierfelder, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.107746Z"},"links":{"cited_paper":"/paper/1104.4751","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:d58620db51413ffeafef1b2a29fe4d09cf0f93b947ac1ea2a4819738a26f9603","observation_id":"3a6b5ee4-8827-48d2-9114-454ada80d986","resolution":{"observed_at":"2026-08-14T10:30:45.107746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01266","last_updated":"2015-04-06T11:34:31Z","snapshot_observed_at":"2026-08-14T22:53:33.440041Z","submitted_at":"2015-04-06T11:34:31Z","title":"Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01266","snapshot_observed_at":"2026-08-14T10:30:45.111585Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.111585Z"},"links":{"cited_paper":"/paper/1504.01266","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:b3f69e984aab8f919d3b3e34a574373da80d198cdf5067b6015a487bc8657c19","observation_id":"a4ed2abf-1f86-4431-8c71-75a2f04963ff","resolution":{"observed_at":"2026-08-14T10:30:45.111585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.07999","last_updated":"2016-09-19T08:43:56Z","snapshot_observed_at":"2026-08-14T21:59:54.444643Z","submitted_at":"2016-04-27T09:48:15Z","title":"Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.07999","snapshot_observed_at":"2026-08-14T10:30:45.115845Z","title":"Bernuzzi and T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.115845Z"},"links":{"cited_paper":"/paper/1604.07999","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:c064f6177843d7f31f0f3ca21dacc8175a6ea8725d374b0beb7a1a2c24266971","observation_id":"b1b8e46e-baa4-43c7-b3ea-6e04d26212f3","resolution":{"observed_at":"2026-08-14T10:30:45.115845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06959","last_updated":"2018-07-18T14:22:20Z","snapshot_observed_at":"2026-08-14T18:50:29.034880Z","submitted_at":"2018-07-18T14:22:20Z","title":"Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06959","snapshot_observed_at":"2026-08-14T10:30:45.119466Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.119466Z"},"links":{"cited_paper":"/paper/1807.06959","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:aee6d73d5bbce8d0f98b2d33ac03992f79e346b57db574b6fab08a35a524e44c","observation_id":"1a3b2abd-8476-4922-8f72-3bde5047a0d1","resolution":{"observed_at":"2026-08-14T10:30:45.119466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.2920","last_updated":"2010-04-27T16:38:50Z","snapshot_observed_at":"2026-07-06T02:04:43.515736Z","submitted_at":"2009-12-15T15:12:17Z","title":"Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.2920","snapshot_observed_at":"2026-08-14T10:30:45.122955Z","title":"Bernuzzi and D","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.122955Z"},"links":{"cited_paper":"/paper/0912.2920","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:96608e3b8576413200b5cb3006a9d89ffe38597149e950207a5b771ddb3ac8b1","observation_id":"27a6a7d1-ccd2-418d-ad98-f892bd0b6c53","resolution":{"observed_at":"2026-08-14T10:30:45.122955Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.5539","last_updated":"2012-02-20T10:28:35Z","snapshot_observed_at":"2026-08-08T19:46:08.712096Z","submitted_at":"2011-07-27T17:04:03Z","title":"Constraint damping for the Z4c formulation of general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.5539","snapshot_observed_at":"2026-08-14T10:30:45.126580Z","title":"Weyhausen, S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.126580Z"},"links":{"cited_paper":"/paper/1107.5539","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:12b567be779fb7164fe2565e5e0c39806d823d723fbf0b06aa2694a91d9b19d9","observation_id":"b784072d-528c-460a-b61d-2d6f88f6e516","resolution":{"observed_at":"2026-08-14T10:30:45.126580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.2901","last_updated":"2012-12-12T17:44:15Z","snapshot_observed_at":"2026-08-15T00:36:12.074558Z","submitted_at":"2012-12-12T17:44:15Z","title":"Compact binary evolutions with the Z4c formulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.2901","snapshot_observed_at":"2026-08-14T10:30:45.130453Z","title":"Hilditch, S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.130453Z"},"links":{"cited_paper":"/paper/1212.2901","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:6c631e948ab12ce6ee0ec553911211b28085dc75e3af3fbf37972329156afbbb","observation_id":"48820c0d-fdb1-486a-926f-47907d886635","resolution":{"observed_at":"2026-08-14T10:30:45.130453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.134273Z","title":"Borges, M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.134273Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:d0bda4a69d3709d257c6f4359081f2418b82b56a48be23dc355eecb674f5bf9a","observation_id":"368d7803-4d3f-4317-9b80-a61ac3c64ad9","resolution":{"observed_at":"2026-08-14T10:30:45.134273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.3611","last_updated":"2012-05-22T08:17:41Z","snapshot_observed_at":"2026-08-10T16:43:26.437988Z","submitted_at":"2011-09-16T13:28:23Z","title":"Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.3611","snapshot_observed_at":"2026-08-14T10:30:45.137929Z","title":"Bernuzzi, M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.137929Z"},"links":{"cited_paper":"/paper/1109.3611","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:a8efd274e16a11ed4138f30e311a260dcc0286bdb7f5e29821a8f0a8afb8152f","observation_id":"d28d7580-d89e-4c23-991f-c3299e6e3e31","resolution":{"observed_at":"2026-08-14T10:30:45.137929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07965","last_updated":"2018-03-21T15:28:55Z","snapshot_observed_at":"2026-08-14T19:33:56.034244Z","submitted_at":"2018-03-21T15:28:55Z","title":"High-resolution numerical relativity simulations of spinning binary neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07965","snapshot_observed_at":"2026-08-14T10:30:45.141690Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.141690Z"},"links":{"cited_paper":"/paper/1803.07965","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bf4e83b99b0c3a2b8203ffaf7ea6d9ab340b0fb0ee4100f9d62df908b5078613","observation_id":"b88f1592-33d3-4ae9-83c3-c9a3c7a31c36","resolution":{"observed_at":"2026-08-14T10:30:45.141690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.01625","last_updated":"2018-06-05T12:14:30Z","snapshot_observed_at":"2026-08-14T19:07:22.865818Z","submitted_at":"2018-06-05T12:14:30Z","title":"CoRe database of binary neutron star merger waveforms and its application in waveform development","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.01625","snapshot_observed_at":"2026-08-14T10:30:45.145383Z","title":"Dietrich, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.145383Z"},"links":{"cited_paper":"/paper/1806.01625","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:d3899a89acd6aae29f7000628970fdd738b74ef681e06b81c6d0052b67a2dd3d","observation_id":"76506d96-1c33-458e-8b5c-138a7dd5cfe8","resolution":{"observed_at":"2026-08-14T10:30:45.145383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06011","last_updated":"2019-07-19T10:05:00Z","snapshot_observed_at":"2026-08-14T16:32:03.624759Z","submitted_at":"2019-05-15T08:05:10Z","title":"Improving the NRTidal model for binary neutron star systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06011","snapshot_observed_at":"2026-08-14T10:30:45.148836Z","title":"Dietrich, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.148836Z"},"links":{"cited_paper":"/paper/1905.06011","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bc4fc89cb9b102fefb215181903ada8099b98ce029623da9ab14615026f4790b","observation_id":"844b8dc8-53e3-48dc-8bcb-29b817faae97","resolution":{"observed_at":"2026-08-14T10:30:45.148836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.08926","last_updated":"2017-08-29T18:00:01Z","snapshot_observed_at":"2026-08-15T00:14:29.869103Z","submitted_at":"2017-08-29T18:00:01Z","title":"Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.08926","snapshot_observed_at":"2026-08-14T10:30:45.152433Z","title":"Kiuchi, K","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.152433Z"},"links":{"cited_paper":"/paper/1708.08926","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:f0ec79f3e83cac1418c8cfd4933626f24ab30bb141f2e82663d00a43e6d01813","observation_id":"be452ef9-9cb2-4390-b85c-c6983f8dccdb","resolution":{"observed_at":"2026-08-14T10:30:45.152433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06251","last_updated":"2017-06-20T09:19:54Z","snapshot_observed_at":"2026-08-14T21:24:44.067402Z","submitted_at":"2016-12-19T16:22:12Z","title":"Entropy-limited hydrodynamics: a novel approach to relativistic hydrodynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06251","snapshot_observed_at":"2026-08-14T10:30:45.155985Z","title":"Guercilena, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.155985Z"},"links":{"cited_paper":"/paper/1612.06251","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:bf56ef638f845b185f6978d1e544af9536740eb144e2d70bac9e6a17bbc67f29","observation_id":"a7c9ea48-2600-46c5-b16d-4d95423a4c37","resolution":{"observed_at":"2026-08-14T10:30:45.155985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.5475","last_updated":"2010-11-24T20:00:22Z","snapshot_observed_at":"2026-07-06T02:19:41.983962Z","submitted_at":"2010-11-24T20:00:22Z","title":"Stationary, Axisymmetric Neutron Stars with Meridional Circulation in General Relativity","version":1},"cited_work":{"arxiv_id":"1011.5475","doi":null,"metadata_source":"pith","pith_arxiv_id":"1011.5475","snapshot_observed_at":"2026-08-14T10:30:45.489836Z","title":"Stationary, Axisymmetric Neutron Stars with Meridional Circulation in General Relativity","venue":"gr-qc","work_id":"58579d5d-3d23-4ba2-a5d4-8626aa00fee1","year":2010},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.159506Z"},"links":{"cited_paper":"/paper/1011.5475","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:0eb35e78fd36abb473bc97c495cb441929ac6a10a7f1dfe21e1c16d84342c36e","observation_id":"39b019a6-7aec-4867-93fc-cb584c4b6c2e","resolution":{"observed_at":"2026-08-14T10:30:45.493851Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.163367Z","title":null,"venue":null,"work_id":null,"year":1924},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.163367Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:1a01d9562bf5c165b25476af17c225246cd0f96d58cbe03eb4397f8cceb88393","observation_id":"314eb06b-0848-459d-9376-68754acf4860","resolution":{"observed_at":"2026-08-14T10:30:45.163367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.074411Z","title":null,"venue":null,"work_id":"307d40ba-f6e5-4bae-b7e8-e6c98919da8d","year":1971},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.167178Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:dded39bfd7a382383ea94f88eed7e66fa43f60d2e43e36467c68724151640b4f","observation_id":"0d813f76-4437-4b50-9dcd-917cef2fa97f","resolution":{"observed_at":"2026-08-14T10:30:46.078204Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.170988Z","title":"Burrows and J","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.170988Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:d9b123d3a9fbe40644aea4b30e11f73e28e255fc31782bde9d5f896df717639b","observation_id":"48e31f26-9c42-4ea5-be19-b7cf84bb95b7","resolution":{"observed_at":"2026-08-14T10:30:45.170988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.174871Z","title":"Keil and H","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.174871Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:86d9a07f657ac6ffe8e0d8acde3be4455df98147d782f948844f69e03a4af812","observation_id":"b4f0ed72-1abb-4f82-a8ce-9c1273e44a9b","resolution":{"observed_at":"2026-08-14T10:30:45.174871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.178650Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.178650Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:a3b1b7f1afbab167f89ed96c593544234e0fb94077cc730b1a25685a4a5a6308","observation_id":"b1af2844-7eb9-4b84-96cf-78165798f19c","resolution":{"observed_at":"2026-08-14T10:30:45.178650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.050836Z","title":null,"venue":null,"work_id":"e94e4b6f-b7fc-4c9b-a80a-535803b0f8d9","year":2012},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.182219Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:8e2d08a0344a426c9046c9a7ab15acb2a1f3d5d200f2ba8d735e6a342d30372f","observation_id":"b570b36a-a7da-48b7-b4fe-826213b13dc5","resolution":{"observed_at":"2026-08-14T10:30:46.054721Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.02945","last_updated":"2016-07-12T21:52:40Z","snapshot_observed_at":"2026-08-14T22:15:16.289631Z","submitted_at":"2016-01-10T15:14:14Z","title":"Spin evolution of a proto-neutron star","version":2},"cited_work":{"arxiv_id":"1601.02945","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.02945","snapshot_observed_at":"2026-08-14T10:30:45.416326Z","title":"Spin evolution of a proto-neutron star","venue":"astro-ph.HE","work_id":"960c3dea-6991-436e-bd63-6b211bc45280","year":2016},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.185882Z"},"links":{"cited_paper":"/paper/1601.02945","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:87e6d02986b181ea76f09acb18987c6ec8bf3bd387f0e7b2f49cb70b9e3a98d6","observation_id":"78305be9-74f6-4e26-86df-a0293187914e","resolution":{"observed_at":"2026-08-14T10:30:45.421004Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.400829Z","title":"Ferrari, G","venue":null,"work_id":"e8d60c02-9fe2-4360-a836-23f69e5d0502","year":2003},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.189640Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:170c61b466c72f67bc1ebee89e5b0de91041ed126952f7e5d8edaa7e91bf7518","observation_id":"b0714e12-f1e7-4f4d-9822-5566a6b894c0","resolution":{"observed_at":"2026-08-14T10:30:45.404655Z","resolver_source":"arxiv_id_nonexistent","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1704.01923","last_updated":"2017-08-11T15:58:17Z","snapshot_observed_at":"2026-08-14T21:07:57.069714Z","submitted_at":"2017-04-06T16:40:39Z","title":"Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.01923","snapshot_observed_at":"2026-08-14T10:30:45.192945Z","title":"Camelio, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.192945Z"},"links":{"cited_paper":"/paper/1704.01923","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:faa90ad4e2326de65cd66c8946b3ebcdf1840f8893f7784caf5d2a091d477fc8","observation_id":"5fc21d87-e3e7-4934-9412-e26ec0bbdf2a","resolution":{"observed_at":"2026-08-14T10:30:45.192945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.196827Z","title":"Chatterjee, T","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.196827Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:0b52609b2013306e366e17b131762952a4080ce7b8ac430e81ba94ef0557c990","observation_id":"48850e41-92e8-4bae-8c86-67c840195641","resolution":{"observed_at":"2026-08-14T10:30:45.196827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0110180","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.353522Z","title":"Rosswog and M","venue":null,"work_id":"d48a4e00-2b10-4d38-88cb-d8cdf471104e","year":2002},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.200678Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:b319c9d8d882f849658e81872d7a63d26eb17b3cdbf1e62f185f825557234cb5","observation_id":"e20b609f-64c0-401e-8a31-6eeb84c5a0c5","resolution":{"observed_at":"2026-08-14T10:30:45.360108Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.204388Z","title":"Bauswein, H.-T","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.204388Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:e01b7ffa74abf7e6cfdf209abc4d1eaa8d5c694718ff59106d1ba0d5e65552e0","observation_id":"ed22a475-a397-4c26-8a2d-db954b0f33ce","resolution":{"observed_at":"2026-08-14T10:30:45.204388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.02002","last_updated":"2020-03-12T08:02:28Z","snapshot_observed_at":"2026-08-14T17:47:59.038947Z","submitted_at":"2018-12-05T17:14:02Z","title":"Equation of state effects in core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.02002","snapshot_observed_at":"2026-08-14T10:30:45.208015Z","title":"Yasin, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.208015Z"},"links":{"cited_paper":"/paper/1812.02002","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:7a5f2703ad8a04028536b5b27414cf39347a03a8e4bb14081a4f49ee842e24f3","observation_id":"db76c4a1-a4bd-44ea-8d02-9e7ad79b88e0","resolution":{"observed_at":"2026-08-14T10:30:45.208015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:45.211772Z","title":null,"venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.211772Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:b53642db8262fbc9d78ba7f17b617a7424b06a5210865664b366c8ffd2dd765b","observation_id":"198cd6c3-d236-4798-abd4-0c7a0d4e717d","resolution":{"observed_at":"2026-08-14T10:30:45.211772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:30:46.033524Z","title":"De Pietri, A","venue":null,"work_id":"ce4a44e7-f70a-4907-a4d0-2d55001d35dc","year":2018},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.215508Z"},"links":{"citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:ddc46b0e2ab5cd5df22f55209e56884c39e90a8c977b1c8da1d44d15f2a35731","observation_id":"1fa08e41-9e77-46a3-a47f-9a26421f51fc","resolution":{"observed_at":"2026-08-14T10:30:46.037880Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.04036","last_updated":"2020-03-21T19:06:06Z","snapshot_observed_at":"2026-08-10T12:06:51.680220Z","submitted_at":"2019-10-09T14:54:25Z","title":"Numerical-relativity simulations of long-lived remnants of binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.04036","snapshot_observed_at":"2026-08-14T10:30:45.219142Z","title":"De Pietri, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T10:30:45.219142Z"},"links":{"cited_paper":"/paper/1910.04036","citing_paper":"/paper/1908.11258"},"observation_digest":"sha256:47c1f23282eb4ccd618d058f615c003d8bf372038d8104d1697662227035ea4f","observation_id":"45abae36-3911-493a-a11a-ee2e4844f7ef","resolution":{"observed_at":"2026-08-14T10:30:45.219142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.11258","last_updated":"2019-11-12T13:58:46Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-15T03:18:47.838979Z","submitted_at":"2019-08-29T14:35:09Z","title":"Rotating neutron stars with non-barotropic thermal profile"},"reference_resolution":{"displayed":86,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":2,"unresolved":59,"verified_exact":10,"verified_fuzzy":14},"total_outbound_references":86},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 86 of 86 outbound references and 1 inbound Pith citation observation for arXiv:1908.11258."}