{"as_of":"2026-08-12T14:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6b578a8f0be7d2355a56ce0ff2108a8c159246c6764fae603e371053d6804b3a","coverage":[{"denominator":91,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":91,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T18:36:01.163906Z","state":"measured"},{"denominator":92,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":92,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+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":"2026-06-28T09:24:35.059596Z","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":"2026-07-02T04:06:35.395231Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"cited_work":{"arxiv_id":"2412.07846","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.07846","snapshot_observed_at":"2026-07-02T04:06:35.395231Z","title":"Perna, O","venue":null,"work_id":"6c1b2a26-e6bb-46bc-b56f-0f87aee96508","year":2025},"citing_paper":{"arxiv_id":"2606.02966","last_updated":"2026-06-02T00:08:57Z","snapshot_observed_at":"2026-07-06T23:43:17.879245Z","submitted_at":"2026-06-02T00:08:57Z","title":"Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-06-28T09:24:35.059596Z"},"links":{"cited_paper":"/paper/2412.07846","citing_paper":"/paper/2606.02966"},"observation_digest":"sha256:2093cb40061213a372b0441ef5e0ad8345b17383d87644ba09eb14f44f733cfd","observation_id":"c756b65b-4cd5-4295-b4a1-69fb3062c6a4","resolution":{"observed_at":"2026-07-02T04:06:35.396526Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2412.07846/citation-record","integrity":"/paper/2412.07846/integrity","json":"/paper/2412.07846/citation-record.json","paper":"/paper/2412.07846"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:36:00.616298Z","title":"Numerical simula- tions of BNS mergers also generally suggest that a hypermassive NS phase is likely necessary to launch a successful GRB jet (see e.g","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.616298Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:742f67cb1d9607b11c3214240840ebe765f6d419fc7970090a59fde9c1b6e294","observation_id":"ac02105c-a603-4c91-8db9-6178a35994ba","resolution":{"observed_at":"2026-08-11T18:36:00.616298Z","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":"2026-08-11T18:36:00.627531Z","title":"When the disk mass is high, Md ≳ 0.1 M⊙, the BH will inevitably produce a long-lived jet, leading to a detectable lbGRB","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.627531Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:61c7315bb0a3f08d658d7c4ddee766d728b5881e8ae162f4af98f27800abff95","observation_id":"79b2a423-e0be-4f35-939f-82632a722d29","resolution":{"observed_at":"2026-08-11T18:36:00.627531Z","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":"2026-08-11T18:36:00.632969Z","title":"supramassive","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.632969Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:97057b14fd48cf4596ab08b313025af4d4ea24aa191f74c45716b0aab5a36bd8","observation_id":"7f58bcfd-2557-4f8f-afdf-03cc0e60753b","resolution":{"observed_at":"2026-08-11T18:36:00.632969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05938","last_updated":"2017-11-08T18:27:39Z","snapshot_observed_at":"2026-07-06T06:04:31.085287Z","submitted_at":"2017-10-16T18:01:14Z","title":"Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05938","snapshot_observed_at":"2026-08-11T18:36:00.661391Z","title":"Margalit and B","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.661391Z"},"links":{"cited_paper":"/paper/1710.05938","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:9a922aee1dbc783893402870dfc158b97f425443b3c6d23fdc15addc83a8677e","observation_id":"096475fd-b27c-487a-872d-26b43343ad71","resolution":{"observed_at":"2026-08-11T18:36:00.661391Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-12T03:03:39.833293Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-11T18:36:00.668658Z","title":"Shibata, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.668658Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:dc6bb2370c09f4308e801b7598c1305a21f093d9c0a4ee54c13c5c9108270411","observation_id":"c7c6df35-03a4-4c8f-a0f2-d46d6d90d31b","resolution":{"observed_at":"2026-08-11T18:36:00.668658Z","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":"2026-08-11T18:36:00.639172Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.639172Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:d60bb9eef3ba5801771a8040e426678833686e17fc37597c189a4831dbdb1d98","observation_id":"634d0905-6a30-4939-91d3-e4df5b5ef824","resolution":{"observed_at":"2026-08-11T18:36:00.639172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.09693","last_updated":"2018-10-30T18:31:23Z","snapshot_observed_at":"2026-07-06T06:46:45.734215Z","submitted_at":"2018-06-25T20:34:21Z","title":"Superluminal motion of a relativistic jet in the neutron star merger GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.09693","snapshot_observed_at":"2026-08-11T18:36:00.644906Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.644906Z"},"links":{"cited_paper":"/paper/1806.09693","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:5d72178488180aa55894ae0c046af0b04e5eb1ea771418b7c59a856d377ba29e","observation_id":"287238c4-b76d-4d38-9290-4a0eb78fd015","resolution":{"observed_at":"2026-08-11T18:36:00.644906Z","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":"2026-08-07T22:20:24.299342Z","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":"2026-08-11T18:36:00.650793Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.650793Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:c779a02932f2d8536566299061f140a29f48914381a67230b1381b64ea7cfcbe","observation_id":"408fc7a8-966d-4e8b-9a60-0aab0f901e1b","resolution":{"observed_at":"2026-08-11T18:36:00.650793Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00314","last_updated":"2018-01-03T12:22:48Z","snapshot_observed_at":"2026-07-06T06:07:12.295602Z","submitted_at":"2017-11-01T12:44:46Z","title":"Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00314","snapshot_observed_at":"2026-08-11T18:36:00.693380Z","title":"Rezzolla, E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.693380Z"},"links":{"cited_paper":"/paper/1711.00314","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:d4d860b2e2258ceccce3d22cd9e54e50c56ac2269551571dd939bd90159aa530","observation_id":"0d1adeac-5e04-488e-a8ef-9b141c75f4e4","resolution":{"observed_at":"2026-08-11T18:36:00.693380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.03656","last_updated":"2019-06-24T09:32:38Z","snapshot_observed_at":"2026-07-06T07:51:54.378890Z","submitted_at":"2019-05-09T14:27:41Z","title":"Constraint on the maximum mass of neutron stars using GW170817 event","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.03656","snapshot_observed_at":"2026-08-11T18:36:00.699152Z","title":"Shibata, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.699152Z"},"links":{"cited_paper":"/paper/1905.03656","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:22d2a8346d13699c74a13b1e6c2121f37699c3d403535733698fc7b49ab9cf2d","observation_id":"1fbd4b86-e079-4bc3-8888-5d7b059387f3","resolution":{"observed_at":"2026-08-11T18:36:00.699152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00549","last_updated":"2018-05-31T11:15:49Z","snapshot_observed_at":"2026-07-06T06:26:08.146670Z","submitted_at":"2018-03-01T18:36:24Z","title":"New constraints on radii and tidal deformabilities of neutron stars from GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00549","snapshot_observed_at":"2026-08-11T18:36:00.675531Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.675531Z"},"links":{"cited_paper":"/paper/1803.00549","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:132dfa7b17d901be10bb71a9a162b316bcc1a98fb45ba8b5c5b3c5c888bfef23","observation_id":"68aaa5ac-84c7-4c2d-a54f-6ad305578568","resolution":{"observed_at":"2026-08-11T18:36:00.675531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.11161","last_updated":"2019-05-30T18:58:04Z","snapshot_observed_at":"2026-07-06T07:04:59.871975Z","submitted_at":"2018-09-28T17:48:24Z","title":"Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.11161","snapshot_observed_at":"2026-08-11T18:36:00.682308Z","title":"Radice, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.682308Z"},"links":{"cited_paper":"/paper/1809.11161","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:b8ac89ac22ce34215a6b61edd007e07cef1468151ae7250077b98c2c12e3ca37","observation_id":"013795aa-6e81-400e-a431-369b2f1d2aab","resolution":{"observed_at":"2026-08-11T18:36:00.682308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03647","last_updated":"2017-12-24T17:36:18Z","snapshot_observed_at":"2026-07-06T06:08:41.171622Z","submitted_at":"2017-11-09T23:34:10Z","title":"GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03647","snapshot_observed_at":"2026-08-11T18:36:00.688144Z","title":"Radice, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.688144Z"},"links":{"cited_paper":"/paper/1711.03647","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:65cbd844dc545c1bfbaa88e13de3e4c77710ea76deb1554e5f50bc708596152a","observation_id":"cde47a5b-a51d-40e8-8a1d-c7c5c5708f4f","resolution":{"observed_at":"2026-08-11T18:36:00.688144Z","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":"2026-08-11T18:36:00.723554Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.723554Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:476e0c12e692d1c6769d5b47ad3e82a77709778a0bab106b9fa189b7a54f175b","observation_id":"6bedcdd8-9b2c-405d-a486-4ef955a8e821","resolution":{"observed_at":"2026-08-11T18:36:00.723554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9810274","last_updated":"1998-10-19T00:42:38Z","snapshot_observed_at":"2026-07-07T01:22:39.300566Z","submitted_at":"1998-10-19T00:42:38Z","title":"Collapsars - Gamma-Ray Bursts and Explosions in \"Failed Supernovae\"","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9810274","snapshot_observed_at":"2026-08-11T18:36:00.730044Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.730044Z"},"links":{"cited_paper":"/paper/astro-ph/9810274","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:ed6e78e21d12b0b074edc92814a6d34f7820788618f12a8461d1f3394de65e5b","observation_id":"0c9ff7c6-f526-4e9a-9bb1-6f7e32114ad4","resolution":{"observed_at":"2026-08-11T18:36:00.730044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11355","last_updated":"2020-12-21T09:29:31Z","snapshot_observed_at":"2026-08-05T18:31:06.496451Z","submitted_at":"2020-02-26T08:41:01Z","title":"Multi-messenger constraints on the neutron-star equation of state and the Hubble constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.11355","snapshot_observed_at":"2026-08-11T18:36:00.704630Z","title":"Dietrich, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.704630Z"},"links":{"cited_paper":"/paper/2002.11355","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:a526aef25d7350bee58559321c027bfa2e5a3f6bcf44cb491dc29f67d3d5c365","observation_id":"71fa18cb-7d75-496c-a22d-79d9ad5652c5","resolution":{"observed_at":"2026-08-11T18:36:00.704630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.08425","last_updated":"2019-06-28T16:52:11Z","snapshot_observed_at":"2026-08-12T12:51:19.663541Z","submitted_at":"2019-04-17T18:00:01Z","title":"Jet-cocoon outflows from neutron star mergers: structure, light curves, and fundamental physics","version":2},"cited_work":{"arxiv_id":"1904.08425","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.08425","snapshot_observed_at":"2026-08-11T18:36:02.729282Z","title":"Jet-cocoon outflows from neutron star mergers: structure, light curves, and fundamental physics","venue":"astro-ph.HE","work_id":"c067409f-9826-43b7-a83c-7d06eb710e8a","year":2019},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.711145Z"},"links":{"cited_paper":"/paper/1904.08425","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:ace1d4b50fb688e0905867c1f1587f4a6801fad3e872a9e462534adfb8209a08","observation_id":"ada6613b-c5c1-462e-a22b-7ca389184107","resolution":{"observed_at":"2026-08-11T18:36:02.735175Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-11T18:36:00.717233Z","title":"Kouveliotou, C","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.717233Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:cf4158bece532f95709c32ef757a57f162861da0b991a62410eb21ad2074b3e8","observation_id":"05a0274b-7d55-4222-a984-169edb43d463","resolution":{"observed_at":"2026-08-11T18:36:00.717233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.09675","last_updated":"2023-10-28T06:53:19Z","snapshot_observed_at":"2026-07-06T13:11:42.962634Z","submitted_at":"2022-05-19T16:34:30Z","title":"Fermi-LAT Detection of a GeV Afterglow from a Compact Stellar Merger","version":4},"cited_work":{"arxiv_id":"2205.09675","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.09675","snapshot_observed_at":"2026-08-11T18:36:02.586667Z","title":"Fermi-LAT Detection of a GeV Afterglow from a Compact Stellar Merger","venue":"astro-ph.HE","work_id":"e4baab9a-141a-43f8-b40c-0b22de6d52c6","year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.766384Z"},"links":{"cited_paper":"/paper/2205.09675","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:0b7b56c290f5fcf6ac13f343cba9630d9dfd17baed3767e38a1b1c65558723bc","observation_id":"1ef1ba7b-5bfb-4891-ba9d-d6cf2b10a101","resolution":{"observed_at":"2026-08-11T18:36:02.594073Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.10864","last_updated":"2022-08-26T18:27:49Z","snapshot_observed_at":"2026-07-06T13:02:56.257094Z","submitted_at":"2022-04-22T18:00:00Z","title":"A Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.10864","snapshot_observed_at":"2026-08-11T18:36:00.737239Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.737239Z"},"links":{"cited_paper":"/paper/2204.10864","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:963efe74eba461ac5a751d7e16e1798bd70e0751331f6c2ebd5132260963f6a4","observation_id":"f98c911f-b4b8-4dfe-8ea7-95022499c2df","resolution":{"observed_at":"2026-08-11T18:36:00.737239Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.03363","last_updated":"2022-12-11T15:39:56Z","snapshot_observed_at":"2026-08-09T00:43:12.488819Z","submitted_at":"2022-09-07T18:00:00Z","title":"A nearby long gamma-ray burst from a merger of compact objects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.03363","snapshot_observed_at":"2026-08-11T18:36:00.742979Z","title":"Troja, C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.742979Z"},"links":{"cited_paper":"/paper/2209.03363","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:a5d56e79b7dea243bc663f9d15aa018d2efefacbc7a3f7093a06941d64a566f0","observation_id":"ce1c529b-1456-432a-b4e2-96a2aca95982","resolution":{"observed_at":"2026-08-11T18:36:00.742979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.12771","last_updated":"2022-10-04T06:39:43Z","snapshot_observed_at":"2026-07-06T13:04:13.261577Z","submitted_at":"2022-04-27T08:42:38Z","title":"A long-duration gamma-ray burst with a peculiar origin","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.12771","snapshot_observed_at":"2026-08-11T18:36:00.749771Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.749771Z"},"links":{"cited_paper":"/paper/2204.12771","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:34c5d13de35d77033b139401c6fb8c9d8cea322c7d03729629e48bb377ba3d91","observation_id":"086333ad-6b28-46e7-bc45-fae98adddf26","resolution":{"observed_at":"2026-08-11T18:36:00.749771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.00038","last_updated":"2023-11-01T18:06:47Z","snapshot_observed_at":"2026-08-07T23:22:15.316673Z","submitted_at":"2023-08-31T18:00:00Z","title":"A Unified Picture of Short and Long Gamma-ray Bursts from Compact Binary Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.00038","snapshot_observed_at":"2026-08-11T18:36:00.790781Z","title":"Gottlieb, B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.790781Z"},"links":{"cited_paper":"/paper/2309.00038","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:34929019d92e6bc16c7a680387a1feed2f01bee03ed5137d66af71c4290c1fc1","observation_id":"618f1a35-3746-4626-9b5b-bea6ab3b92fd","resolution":{"observed_at":"2026-08-11T18:36:00.790781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.13657","last_updated":"2025-04-21T17:44:37Z","snapshot_observed_at":"2026-07-06T19:53:25.777341Z","submitted_at":"2024-11-20T19:03:15Z","title":"A Unified Model of Kilonovae and GRBs in Binary Mergers Establishes Neutron Stars as the Central Engines of Short GRBs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.13657","snapshot_observed_at":"2026-08-11T18:36:00.796755Z","title":"Gottlieb, B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.796755Z"},"links":{"cited_paper":"/paper/2411.13657","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:5b697bc89ddf393530ba5766309a8b231dfd9e11e1c46f133c94cdb3d5afd885","observation_id":"5998c6b9-0c9d-4a36-acd5-7189bd4b14b2","resolution":{"observed_at":"2026-08-11T18:36:00.796755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.02098","last_updated":"2023-07-05T08:19:23Z","snapshot_observed_at":"2026-07-06T15:50:26.113234Z","submitted_at":"2023-07-05T08:19:23Z","title":"JWST detection of heavy neutron capture elements in a compact object merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02098","snapshot_observed_at":"2026-08-11T18:36:00.772446Z","title":"Levan, B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.772446Z"},"links":{"cited_paper":"/paper/2307.02098","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:049c01e1f21a5d07532541d75d0efe231ea4b9ea5c90e3047f083611cbdbe142","observation_id":"1d8c48b0-30b3-44ac-b047-87703a22add2","resolution":{"observed_at":"2026-08-11T18:36:00.772446Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.05689","last_updated":"2024-11-21T09:15:04Z","snapshot_observed_at":"2026-07-06T15:52:56.032035Z","submitted_at":"2023-07-11T18:01:02Z","title":"Magnetar emergence in a peculiar gamma-ray burst from a compact star merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.05689","snapshot_observed_at":"2026-08-11T18:36:00.778649Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.778649Z"},"links":{"cited_paper":"/paper/2307.05689","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:0bd3577f1d517e03b507b7b7dde222fe958c623def8d86aa7d19026f1c26da39","observation_id":"3c9e9ec4-3349-4297-ac24-88029b10fadc","resolution":{"observed_at":"2026-08-11T18:36:00.778649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12935","last_updated":"2023-04-26T04:15:03Z","snapshot_observed_at":"2026-08-07T12:28:30.744837Z","submitted_at":"2023-03-22T22:30:40Z","title":"GRB 191019A: a short gamma-ray burst in disguise from the disk of an active galactic nucleus","version":2},"cited_work":{"arxiv_id":"2303.12935","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.12935","snapshot_observed_at":"2026-08-11T18:36:02.517037Z","title":"GRB 191019A: a short gamma-ray burst in disguise from the disk of an active galactic nucleus","venue":"astro-ph.HE","work_id":"efd657ab-e895-436f-9b25-13bc8b32b9f0","year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.784494Z"},"links":{"cited_paper":"/paper/2303.12935","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:42a9572f805f1e17894e251356c6a2d6b8a6f4df3fae030b96237b4aa973feb1","observation_id":"05950d1f-2e94-4525-b94d-5abe927a7e0d","resolution":{"observed_at":"2026-08-11T18:36:02.523455Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.01656","last_updated":"2022-07-29T13:34:59Z","snapshot_observed_at":"2026-08-11T22:50:28.793425Z","submitted_at":"2022-02-03T16:09:38Z","title":"Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.01656","snapshot_observed_at":"2026-08-11T18:36:00.819869Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.819869Z"},"links":{"cited_paper":"/paper/2202.01656","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:dfead977ee4d1fe9c3d73b0b7a40fb48d068c82a3ee42e0aba3cb0a0e5f2e38a","observation_id":"75ecb0d7-8a74-4b65-afcc-bbe46416ea41","resolution":{"observed_at":"2026-08-11T18:36:00.819869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.08697","last_updated":"2017-04-27T18:00:05Z","snapshot_observed_at":"2026-08-03T05:57:23.863319Z","submitted_at":"2017-04-27T18:00:05Z","title":"The Fate of Neutron Star Binary Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.08697","snapshot_observed_at":"2026-08-11T18:36:00.826149Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.826149Z"},"links":{"cited_paper":"/paper/1704.08697","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:c56afec543d889befc09c544e19c01fcf5ddd8d49c2fb776ec5f7906216ccdcf","observation_id":"4bc69097-0998-4e08-8625-76d0e74da6df","resolution":{"observed_at":"2026-08-11T18:36:00.826149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.02158","last_updated":"2024-11-25T09:35:54Z","snapshot_observed_at":"2026-08-12T06:16:02.759924Z","submitted_at":"2024-09-03T18:00:00Z","title":"Uniform Modeling of Observed Kilonovae: Implications for Diversity and the Progenitors of Merger-Driven Long Gamma-Ray Bursts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.02158","snapshot_observed_at":"2026-08-11T18:36:00.802339Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.802339Z"},"links":{"cited_paper":"/paper/2409.02158","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:d038251020976323bd3f43c1275e005dd09045484615c336e9b05b2b6aacb3c0","observation_id":"0594fbd7-1ebc-4fc3-8cb3-ffb225035435","resolution":{"observed_at":"2026-08-11T18:36:00.802339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0712.1036","last_updated":"2008-04-16T20:50:19Z","snapshot_observed_at":"2026-07-06T01:32:58.935959Z","submitted_at":"2007-12-06T21:21:18Z","title":"The lowest-mass stellar black holes: catastrophic death of neutron stars in gamma-ray bursts","version":2},"cited_work":{"arxiv_id":"0712.1036","doi":null,"metadata_source":"pith","pith_arxiv_id":"0712.1036","snapshot_observed_at":"2026-08-11T18:36:02.424398Z","title":"The lowest-mass stellar black holes: catastrophic death of neutron stars in gamma-ray bursts","venue":"astro-ph","work_id":"a3717cef-fe2c-44f8-baa6-38b0419b4110","year":2007},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.807520Z"},"links":{"cited_paper":"/paper/0712.1036","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:e45fd9068e0fef372fa2360998a459f6bc6dde65d9d5821dd8003cd09479893c","observation_id":"d9892d09-56e4-4a23-bb2e-c06f0b3fe6ab","resolution":{"observed_at":"2026-08-11T18:36:02.429991Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1504.07605","last_updated":"2015-04-28T19:19:38Z","snapshot_observed_at":"2026-07-06T04:16:21.146865Z","submitted_at":"2015-04-28T19:19:38Z","title":"The Fate of the Compact Remnant in Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.07605","snapshot_observed_at":"2026-08-11T18:36:00.813950Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.813950Z"},"links":{"cited_paper":"/paper/1504.07605","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:48e949a3cc7f316422ce7a650e1d9ce69ed17559fdcc9d000c1ea28129e3927b","observation_id":"a951bea8-b166-40d2-80e3-6d5e4c8a2b53","resolution":{"observed_at":"2026-08-11T18:36:00.813950Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05124","last_updated":"2022-07-11T18:33:55Z","snapshot_observed_at":"2026-08-10T17:13:00.811696Z","submitted_at":"2022-07-11T18:33:55Z","title":"PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05124","snapshot_observed_at":"2026-08-11T18:36:00.847818Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.847818Z"},"links":{"cited_paper":"/paper/2207.05124","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:c5e36433279ff4979330381a8aed624c99a649fdfa37c74f62b766b18e0f43bf","observation_id":"7596213e-b845-47b6-8f8d-24ec5b3bd582","resolution":{"observed_at":"2026-08-11T18:36:00.847818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.4584","last_updated":"2010-06-23T16:35:32Z","snapshot_observed_at":"2026-07-06T02:12:05.106403Z","submitted_at":"2010-06-23T16:35:32Z","title":"Further Evidence for the Bimodal Distribution of Neutron Star Masses","version":1},"cited_work":{"arxiv_id":"1006.4584","doi":null,"metadata_source":"pith","pith_arxiv_id":"1006.4584","snapshot_observed_at":"2026-08-11T18:36:02.253623Z","title":"Further Evidence for the Bimodal Distribution of Neutron Star Masses","venue":"astro-ph.HE","work_id":"84c9b636-06b0-484a-9de1-d03e22d817c3","year":2010},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.852887Z"},"links":{"cited_paper":"/paper/1006.4584","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:703aa3c10a1525bdab97305d3d1411c07ed38ff113ebab7a9a1ed780fafeb4bf","observation_id":"610c778c-6095-4865-84f5-9eb1cb2f4415","resolution":{"observed_at":"2026-08-11T18:36:02.259363Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.06102","last_updated":"2020-03-20T02:25:43Z","snapshot_observed_at":"2026-08-06T04:17:09.015079Z","submitted_at":"2020-01-16T22:43:11Z","title":"Gravitational waves or deconfined quarks: what causes the premature collapse of neutron stars born in short gamma-ray bursts?","version":2},"cited_work":{"arxiv_id":"2001.06102","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.06102","snapshot_observed_at":"2026-08-11T18:36:02.345522Z","title":"Gravitational waves or deconfined quarks: what causes the premature collapse of neutron stars born in short gamma-ray bursts?","venue":"astro-ph.HE","work_id":"682e603d-24f9-493f-974c-ad440c8bef16","year":2020},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.831893Z"},"links":{"cited_paper":"/paper/2001.06102","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:2ce5dbed1aeaaca33c8ae1d40bc314477ce0b7c17c3a7de46d367c5c9c429cd1","observation_id":"2fc516ef-861a-4cfb-b493-946815410781","resolution":{"observed_at":"2026-08-11T18:36:02.351058Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.07941","last_updated":"2025-01-08T11:55:30Z","snapshot_observed_at":"2026-08-12T11:57:08.102737Z","submitted_at":"2024-10-10T14:07:43Z","title":"Incidence of afterglow plateaus in gamma-ray bursts associated with binary neutron star mergers","version":3},"cited_work":{"arxiv_id":"2410.07941","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.07941","snapshot_observed_at":"2026-08-11T18:36:02.318819Z","title":"Incidence of afterglow plateaus in gamma-ray bursts associated with binary neutron star mergers","venue":"astro-ph.HE","work_id":"ae92c609-79d8-4d00-8b15-a7fa3a940d1e","year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.837337Z"},"links":{"cited_paper":"/paper/2410.07941","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:1becae82b217b74feb9540aeb8ac1b4be438cf2ff742a026376079815bf31e22","observation_id":"0f5acb9e-0d97-430c-acd8-fd7d5fd82ec6","resolution":{"observed_at":"2026-08-11T18:36:02.324655Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1706.09438","last_updated":"2017-09-18T14:45:33Z","snapshot_observed_at":"2026-07-06T05:48:53.684011Z","submitted_at":"2017-06-28T18:30:26Z","title":"Formation of Double Neutron Star Systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.09438","snapshot_observed_at":"2026-08-11T18:36:00.842228Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.842228Z"},"links":{"cited_paper":"/paper/1706.09438","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:c9d26982c27a38994e905e288b47935e85e3bcd08b9615f6a549c517dd14d048","observation_id":"2dfdb7a6-78e3-4dec-bc5f-5f069c7ac53b","resolution":{"observed_at":"2026-08-11T18:36:00.842228Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01495","last_updated":"2021-04-08T09:19:00Z","snapshot_observed_at":"2026-08-12T12:19:26.751215Z","submitted_at":"2020-11-03T06:06:46Z","title":"Heavy double neutron stars: birth, mid-life and death","version":2},"cited_work":{"arxiv_id":"2011.01495","doi":null,"metadata_source":"pith","pith_arxiv_id":"2011.01495","snapshot_observed_at":"2026-08-11T18:36:02.175476Z","title":"Heavy double neutron stars: birth, mid-life and death","venue":"astro-ph.HE","work_id":"b85c3849-6536-4698-a964-9a56b388d876","year":2020},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.872919Z"},"links":{"cited_paper":"/paper/2011.01495","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:0527572364a3e45247c220e68013f17c5d6e96ffeeb8444f159e0d87cf026393","observation_id":"3abfdbf2-6c7a-4d7c-aa94-f0562f83f344","resolution":{"observed_at":"2026-08-11T18:36:02.181237Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.13244","last_updated":"2023-12-20T18:16:12Z","snapshot_observed_at":"2026-08-10T11:10:01.336007Z","submitted_at":"2023-12-20T18:16:12Z","title":"Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.13244","snapshot_observed_at":"2026-08-11T18:36:00.878084Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.878084Z"},"links":{"cited_paper":"/paper/2312.13244","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:30c7771690946057c99610f178add2e8601cb70e9810c085c32cee12535395c7","observation_id":"9229f439-f1b7-4498-b57f-0821ce9a3588","resolution":{"observed_at":"2026-08-11T18:36:00.878084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.01665","last_updated":"2016-05-05T17:43:59Z","snapshot_observed_at":"2026-08-03T17:47:52.719584Z","submitted_at":"2016-05-05T17:43:59Z","title":"The millisecond pulsar mass distribution: Evidence for bimodality and constraints on the maximum neutron star mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.01665","snapshot_observed_at":"2026-08-11T18:36:00.857808Z","title":"Antoniadis, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.857808Z"},"links":{"cited_paper":"/paper/1605.01665","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:6b3bcd7c992717a09a08b634f97a75b0f46bb4433434d250c7b4b912ea244fd0","observation_id":"85314c21-56ba-43c6-81aa-c80b82c6761b","resolution":{"observed_at":"2026-08-11T18:36:00.857808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.07889","last_updated":"2018-04-25T01:53:09Z","snapshot_observed_at":"2026-07-06T06:00:57.001365Z","submitted_at":"2017-09-22T18:01:01Z","title":"Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.07889","snapshot_observed_at":"2026-08-11T18:36:00.862878Z","title":"Alsing, H","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.862878Z"},"links":{"cited_paper":"/paper/1709.07889","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:cb53ecc258c3a6781b7310a26c04fe96787f449ffcc5bf3fdb258bb0d3f2015a","observation_id":"09879e6c-b97d-48e9-9c45-cb09558f90d5","resolution":{"observed_at":"2026-08-11T18:36:00.862878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.00032","last_updated":"2020-04-30T18:04:12Z","snapshot_observed_at":"2026-08-12T14:03:49.529628Z","submitted_at":"2020-04-30T18:04:12Z","title":"A Population-Informed Mass Estimate for Pulsar J0740+6620","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.00032","snapshot_observed_at":"2026-08-11T18:36:00.867842Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.867842Z"},"links":{"cited_paper":"/paper/2005.00032","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:a1342cf5fd9db19fdc9a2b316093760dc3598a46c662ace56c46f6f073a2ca02","observation_id":"083bc8e2-1498-4312-83ef-91a3b6924dd5","resolution":{"observed_at":"2026-08-11T18:36:00.867842Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.06083","last_updated":"2016-04-11T19:42:35Z","snapshot_observed_at":"2026-07-06T04:43:45.267725Z","submitted_at":"2016-01-22T17:39:26Z","title":"Maximum mass, moment of inertia and compactness of relativistic stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.06083","snapshot_observed_at":"2026-08-11T18:36:00.902060Z","title":"Breu and L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.902060Z"},"links":{"cited_paper":"/paper/1601.06083","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:e5cbff212366e5ec18f49cf04c8b02a5452689313c5683b238281d44b809c01f","observation_id":"6e125493-be02-4621-bdd5-d6d3bbde7a83","resolution":{"observed_at":"2026-08-11T18:36:00.902060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.05183","last_updated":"2022-04-08T06:22:28Z","snapshot_observed_at":"2026-08-07T22:04:24.788063Z","submitted_at":"2021-11-09T14:49:51Z","title":"Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.05183","snapshot_observed_at":"2026-08-11T18:36:00.908362Z","title":"Kashyap, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.908362Z"},"links":{"cited_paper":"/paper/2111.05183","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:eacd56af0ede7a39db4ae3d80cb479d0f4e4153e61c5f2e9b4332955efc634d8","observation_id":"4dfd42c4-ddc3-4fec-a3ac-32d5768faba0","resolution":{"observed_at":"2026-08-11T18:36:00.908362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701083","last_updated":"2007-11-12T20:35:56Z","snapshot_observed_at":"2026-07-07T01:05:52.255088Z","submitted_at":"2007-01-04T07:26:50Z","title":"Fallback and Black Hole Production in Massive Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0701083","snapshot_observed_at":"2026-08-11T18:36:00.883645Z","title":"Zhang, S","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.883645Z"},"links":{"cited_paper":"/paper/astro-ph/0701083","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:a2fd6a8151218fa6abd37551b2788317d03c8ba0ef9984502c0e9b81d0c84db8","observation_id":"c63f39f4-34dc-49a1-a7d7-e721a52dd87a","resolution":{"observed_at":"2026-08-11T18:36:00.883645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.2859","last_updated":"2008-11-18T08:34:44Z","snapshot_observed_at":"2026-07-06T01:47:41.369729Z","submitted_at":"2008-11-18T08:34:44Z","title":"Exploring the consequences of pairing algorithms for binary stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.2859","snapshot_observed_at":"2026-08-11T18:36:00.889653Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.889653Z"},"links":{"cited_paper":"/paper/0811.2859","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:767dd6d33ddc26512514f3e0741861d8e2874fbd0560ec63c9e57f0a5a1cf179","observation_id":"5c0dd118-de3b-4cb3-96c2-831c80a77452","resolution":{"observed_at":"2026-08-11T18:36:00.889653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.03863","last_updated":"2020-02-10T15:27:24Z","snapshot_observed_at":"2026-08-10T22:09:36.230010Z","submitted_at":"2020-02-10T15:27:24Z","title":"The Dynamics of Binary Neutron Star Mergers and of GW170817","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.03863","snapshot_observed_at":"2026-08-11T18:36:00.895837Z","title":"Radice, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.895837Z"},"links":{"cited_paper":"/paper/2002.03863","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:52efbfedf84569f484d81a32b698a56826a38ccc226e2ac7cd860f976867cc0f","observation_id":"ec738e3c-b57b-4e70-b37c-3d316abfe46f","resolution":{"observed_at":"2026-08-11T18:36:00.895837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.06636","last_updated":"2016-07-22T11:26:39Z","snapshot_observed_at":"2026-07-06T05:04:33.578185Z","submitted_at":"2016-07-22T11:26:39Z","title":"Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.06636","snapshot_observed_at":"2026-08-11T18:36:00.932937Z","title":"Dietrich, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.932937Z"},"links":{"cited_paper":"/paper/1607.06636","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:687b815d7a1a865b1bf9f1a6589d461acc496fb10c39fa7c0d72fced0315bde3","observation_id":"334a73b7-89a8-455b-b033-11b7aa4a82fe","resolution":{"observed_at":"2026-08-11T18:36:00.932937Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.01466","last_updated":"2019-05-14T04:00:45Z","snapshot_observed_at":"2026-07-06T07:36:59.181170Z","submitted_at":"2019-03-04T19:00:00Z","title":"Revisiting the lower bound on tidal deformability derived by AT 2017gfo","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.01466","snapshot_observed_at":"2026-08-11T18:36:00.938783Z","title":"Kiuchi, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.938783Z"},"links":{"cited_paper":"/paper/1903.01466","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:e7b4e5e75cc65ba52c6c575a74212d1fc1b7d8fe52253014607cf99a35a09735","observation_id":"fe620953-cc9f-4d6f-a4ab-2b6caf47740e","resolution":{"observed_at":"2026-08-11T18:36:00.938783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.05864","last_updated":"2022-05-17T17:23:43Z","snapshot_observed_at":"2026-08-02T10:17:36.873510Z","submitted_at":"2021-12-10T23:11:27Z","title":"Probing the incompressibility of nuclear matter at ultra-high density through the prompt collapse of asymmetric neutron star binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.05864","snapshot_observed_at":"2026-08-11T18:36:00.913727Z","title":"Perego, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.913727Z"},"links":{"cited_paper":"/paper/2112.05864","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:72405ede1bb32410cfe5f5d6e7dcaafe96aa2d0ea2d264b83875471713bd4e89","observation_id":"0636b28c-3752-4d50-a276-555a1590f2b6","resolution":{"observed_at":"2026-08-11T18:36:00.913727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.15067","last_updated":"2024-02-28T16:04:56Z","snapshot_observed_at":"2026-08-11T03:57:53.664750Z","submitted_at":"2023-08-29T07:00:04Z","title":"Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.15067","snapshot_observed_at":"2026-08-11T18:36:00.920338Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.920338Z"},"links":{"cited_paper":"/paper/2308.15067","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:d30acf44115bb55b7b8b3a0943bafaa36c73fbcefb951a7aef6b2b1e14439dd5","observation_id":"34197c54-f587-4ab1-aefc-ce192806141b","resolution":{"observed_at":"2026-08-11T18:36:00.920338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.4370","last_updated":"2011-05-22T20:59:21Z","snapshot_observed_at":"2026-08-01T14:37:15.229171Z","submitted_at":"2011-05-22T20:59:21Z","title":"Binary Neutron Star Mergers: Dependence on the Nuclear Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.4370","snapshot_observed_at":"2026-08-11T18:36:00.925967Z","title":"Hotokezaka, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.925967Z"},"links":{"cited_paper":"/paper/1105.4370","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:9318e10cf5ca8954ecc774bb6b3d19416d148c877368d6707df596972aaaf382","observation_id":"ba76297b-5760-4a7b-acfa-2880d1ba2417","resolution":{"observed_at":"2026-08-11T18:36:00.925967Z","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":"2026-08-11T18:36:00.609217Z","title":"We note that this is a rough estimate and possibly subject to change with more future data","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.609217Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:5158563243d93c1865a09a86b829d0da44dca9f1b39a6527362f0ab79ecc0e89","observation_id":"485f74bc-0685-487c-b688-3364ee2185fc","resolution":{"observed_at":"2026-08-11T18:36:00.609217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0412","last_updated":"2011-08-30T10:39:40Z","snapshot_observed_at":"2026-07-06T02:31:46.808257Z","submitted_at":"2011-08-01T20:00:01Z","title":"Efficient Generation of Jets from Magnetically Arrested Accretion on a Rapidly Spinning Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0412","snapshot_observed_at":"2026-08-11T18:36:00.969035Z","title":"Tchekhovskoy, R","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.969035Z"},"links":{"cited_paper":"/paper/1108.0412","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:ede2a7abc624c71bf70274548bad31df330b12cb14d285a59453211f4c0cc8ba","observation_id":"f6f47de0-9f6f-492b-825f-a07fb2e7a86c","resolution":{"observed_at":"2026-08-11T18:36:00.969035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-08-11T18:36:00.945146Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.945146Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:650891a3ac061830a91379177f82e1700fe639ce822a1be697ffaa656bf3706f","observation_id":"bcd436b2-d477-418a-801b-a692179abeaa","resolution":{"observed_at":"2026-08-11T18:36:00.945146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.01763","last_updated":"2022-06-03T18:00:08Z","snapshot_observed_at":"2026-08-11T03:41:25.817722Z","submitted_at":"2022-06-03T18:00:08Z","title":"Short GRB Host Galaxies I: Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.01763","snapshot_observed_at":"2026-08-11T18:36:00.951066Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.951066Z"},"links":{"cited_paper":"/paper/2206.01763","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:7998df94e6b8f53e1e330207f396c9c92cc1c99fb017fb009f0006312af08035","observation_id":"096184ee-d2b4-4810-92ec-bd20e5a2bc6b","resolution":{"observed_at":"2026-08-11T18:36:00.951066Z","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":"2026-08-11T18:36:00.958880Z","title":"Gehrels, J","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.958880Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:8107c695612a9aa3a6ebab0b553e4f1cddf7ed9981356cb172c38b8b290fcf59","observation_id":"63816926-06f6-4687-bccb-5c1ac25b9a4a","resolution":{"observed_at":"2026-08-11T18:36:00.958880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.00638","last_updated":"2023-08-02T15:54:46Z","snapshot_observed_at":"2026-07-06T16:01:18.530479Z","submitted_at":"2023-08-01T16:12:20Z","title":"A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.00638","snapshot_observed_at":"2026-08-11T18:36:00.964067Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.964067Z"},"links":{"cited_paper":"/paper/2308.00638","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:db8443ae332d5a6dca7602cab7c75246a3802dfa0fb369ef10489d85d3e6e87c","observation_id":"8f58ff06-c4f2-43d2-9479-f48d0aca458c","resolution":{"observed_at":"2026-08-11T18:36:00.964067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.01842","last_updated":"2015-05-07T20:00:32Z","snapshot_observed_at":"2026-07-06T04:17:14.373478Z","submitted_at":"2015-05-07T20:00:32Z","title":"Does the Collapse of a Supramassive Neutron Star Leave a Debris Disk?","version":1},"cited_work":{"arxiv_id":"1505.01842","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.01842","snapshot_observed_at":"2026-08-11T18:36:01.691534Z","title":"Does the Collapse of a Supramassive Neutron Star Leave a Debris Disk?","venue":"astro-ph.HE","work_id":"ff7fb600-5868-41d8-add6-a942839a8c2e","year":2015},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.998478Z"},"links":{"cited_paper":"/paper/1505.01842","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:fdf855bdbdbe53f7c6e01cf41063a0ad92cfd12425f210666654fc1131ce0e6b","observation_id":"041797f4-d171-425f-86a7-ccfcea748a23","resolution":{"observed_at":"2026-08-11T18:36:01.817470Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1310.4506","last_updated":"2013-10-16T20:01:05Z","snapshot_observed_at":"2026-07-06T03:25:47.809707Z","submitted_at":"2013-10-16T20:01:05Z","title":"Constraints on long-lived remnants of neutron star binary mergers from late-time radio observations of short duration gamma-ray bursts","version":1},"cited_work":{"arxiv_id":"1310.4506","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.4506","snapshot_observed_at":"2026-08-11T18:36:01.889441Z","title":"Constraints on long-lived remnants of neutron star binary mergers from late-time radio observations of short duration gamma-ray bursts","venue":"astro-ph.HE","work_id":"d9569219-923e-4fb7-a3c2-2f95078a90d8","year":2013},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.973998Z"},"links":{"cited_paper":"/paper/1310.4506","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:efd02284d9c8df648ad78860b96587576edd83afa641c4c836966e3a865b890e","observation_id":"3fd5c7ec-ef7b-4a18-a2ef-ac17eb67121b","resolution":{"observed_at":"2026-08-11T18:36:01.895554Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01692","last_updated":"2016-01-07T21:00:10Z","snapshot_observed_at":"2026-07-06T04:42:11.317805Z","submitted_at":"2016-01-07T21:00:10Z","title":"Testing the Magnetar Model via Late Time Radio Observations of Two Macronova Candidates","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.01692","snapshot_observed_at":"2026-08-11T18:36:00.980324Z","title":"Horesh, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.980324Z"},"links":{"cited_paper":"/paper/1601.01692","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:ece6c0905a827f84767a30104c3ebb81cc938a9d758c0dd1a2c1a6409f8c875d","observation_id":"b8a9a9ba-0564-4fe3-b631-1ddcc1eef34a","resolution":{"observed_at":"2026-08-11T18:36:00.980324Z","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":"2026-08-11T18:36:00.621582Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.621582Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:d9a538d1c58e1e4581328ad6d4beea49dd3859209e03bcbad55e2601bff85e56","observation_id":"dcdeb85d-e6fd-4f0f-96cf-d1d0043e7ea0","resolution":{"observed_at":"2026-08-11T18:36:00.621582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.01181","last_updated":"2021-07-20T15:26:20Z","snapshot_observed_at":"2026-08-09T11:50:44.600317Z","submitted_at":"2021-04-02T18:00:02Z","title":"Survival times of supramassive neutron stars resulting from binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.01181","snapshot_observed_at":"2026-08-11T18:36:00.986616Z","title":"Beniamini and W","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.986616Z"},"links":{"cited_paper":"/paper/2104.01181","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:306f552f8f049245d4aff17ffbda526a6002b36b74836030d656a30ce3ca5e0f","observation_id":"d4061f4b-9876-44ae-8f5b-59c8c5030c50","resolution":{"observed_at":"2026-08-11T18:36:00.986616Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09164","last_updated":"2023-11-24T19:53:13Z","snapshot_observed_at":"2026-08-09T04:07:38.103999Z","submitted_at":"2023-08-17T19:46:33Z","title":"Constraining the long-lived supramassive neutron stars by magnetar boosted kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09164","snapshot_observed_at":"2026-08-11T18:36:00.993179Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.993179Z"},"links":{"cited_paper":"/paper/2308.09164","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:a2dbe8cb59156858648108ae54ee4463523cbc00f58cd100aa4f04dc2376d19a","observation_id":"b26fbb08-2281-4715-b32a-e33d2f64b91c","resolution":{"observed_at":"2026-08-11T18:36:00.993179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03684","last_updated":"2018-04-10T18:41:45Z","snapshot_observed_at":"2026-07-06T06:32:44.292339Z","submitted_at":"2018-04-10T18:41:45Z","title":"Short gamma-ray burst central engines","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03684","snapshot_observed_at":"2026-08-11T18:36:01.004876Z","title":"Ciolfi, International Journal of Modern Physics D 27, 1842004 (2018), arXiv:1804.03684 [astro-ph.HE]","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.004876Z"},"links":{"cited_paper":"/paper/1804.03684","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:0226c133ec30d1c3e82baf1216f1eb9567ed0111e264db3620a05ee3c069bb2b","observation_id":"4b626b6c-a673-42fd-b8a9-f26d417b4efe","resolution":{"observed_at":"2026-08-11T18:36:01.004876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04828","last_updated":"2016-09-15T20:00:12Z","snapshot_observed_at":"2026-07-06T05:10:58.923264Z","submitted_at":"2016-09-15T20:00:12Z","title":"The Properties of Short gamma-ray burst Jets Triggered by neutron star mergers","version":1},"cited_work":{"arxiv_id":"1609.04828","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.04828","snapshot_observed_at":"2026-08-11T18:36:01.649938Z","title":"The Properties of Short gamma-ray burst Jets Triggered by neutron star mergers","venue":"astro-ph.HE","work_id":"e1ee5052-7886-4640-b771-9305f7a4ba8d","year":2016},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.010811Z"},"links":{"cited_paper":"/paper/1609.04828","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:8bd157bdbb34128d7af9d3780538fe502e7832db9abeb8fba7825e45ef74fc92","observation_id":"084aefe8-d017-43bd-b5f5-518078a89108","resolution":{"observed_at":"2026-08-11T18:36:01.656381Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.15721","last_updated":"2024-02-16T06:01:12Z","snapshot_observed_at":"2026-08-07T13:11:02.937261Z","submitted_at":"2023-06-27T18:00:05Z","title":"A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.15721","snapshot_observed_at":"2026-08-11T18:36:01.016891Z","title":"Kiuchi, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.016891Z"},"links":{"cited_paper":"/paper/2306.15721","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:ef33cce6fd921c99f00896d62806e07f28ec4a0a599c3348d3f2bc104f32bea8","observation_id":"e43e89c8-5453-4f80-898c-da998a43b8ca","resolution":{"observed_at":"2026-08-11T18:36:01.016891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6304","last_updated":"2012-12-10T15:22:55Z","snapshot_observed_at":"2026-07-06T02:52:37.689341Z","submitted_at":"2012-07-26T15:48:53Z","title":"Black Hole-Neutron Star Mergers: Disk Mass Predictions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.6304","snapshot_observed_at":"2026-08-11T18:36:01.023189Z","title":"Foucart, Phys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.023189Z"},"links":{"cited_paper":"/paper/1207.6304","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:287337de7eade248b7255e435b1b27d3f4c4a0896bcea4b00d74042555f30495","observation_id":"c942142f-db6d-4997-8ddf-aa75521f4760","resolution":{"observed_at":"2026-08-11T18:36:01.023189Z","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":"2026-08-11T18:36:01.029392Z","title":"Abbott, others (LIGO Scientific Collaboration, and V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.029392Z"},"links":{"citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:b44564737ba3296a24228ac43c40cb8e79d57385baea49475a402e197935f06c","observation_id":"1e7ed42d-4f5c-4065-8d0c-16c166208afe","resolution":{"observed_at":"2026-08-11T18:36:01.029392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10645","last_updated":"2022-08-22T23:57:29Z","snapshot_observed_at":"2026-08-11T10:59:17.152456Z","submitted_at":"2022-06-21T18:00:15Z","title":"Angular Momentum Transport in Proto-Neutron Stars and the Fate of Neutron Star Merger Remnants","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.10645","snapshot_observed_at":"2026-08-11T18:36:01.035823Z","title":"Margalit, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.035823Z"},"links":{"cited_paper":"/paper/2206.10645","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:18c5b405f94bfc867e4cb8a99f1b9d93d4b1b149ac600ba5254398a21c0fecb8","observation_id":"70015b55-1323-4336-b285-53eeb0b4e6fb","resolution":{"observed_at":"2026-08-11T18:36:01.035823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9910565","last_updated":"1999-11-01T15:28:06Z","snapshot_observed_at":"2026-07-07T01:29:27.201153Z","submitted_at":"1999-11-01T15:28:06Z","title":"On the Maximum Mass of Differentially Rotating Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9910565","snapshot_observed_at":"2026-08-11T18:36:01.041687Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.041687Z"},"links":{"cited_paper":"/paper/astro-ph/9910565","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:00e689b13426cb967f212fe5f98951ec549c7047c66fb70ec49906b7c8b1412d","observation_id":"8e874713-aac3-442a-8422-eaeffb836062","resolution":{"observed_at":"2026-08-11T18:36:01.041687Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.1352","last_updated":"2014-02-12T01:39:06Z","snapshot_observed_at":"2026-07-06T03:27:31.142558Z","submitted_at":"2013-11-06T11:19:36Z","title":"Nuclear Equation of State from Observations of Short Gamma-Ray Burst Remnants","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.1352","snapshot_observed_at":"2026-08-11T18:36:01.047688Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.047688Z"},"links":{"cited_paper":"/paper/1311.1352","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:c0bddac03241bc37379a7e7a936098ab4efd681bf5d12512af3b4387d89bf67b","observation_id":"bc2cc05f-d958-4456-a4c8-ff90e6ddbd52","resolution":{"observed_at":"2026-08-11T18:36:01.047688Z","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":"2026-07-06T06:43:04.228880Z","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":"2026-08-11T18:36:01.053400Z","title":"Dietrich, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.053400Z"},"links":{"cited_paper":"/paper/1806.01625","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:5b3b4a362ab95599181ed98ff8bf421de77c03df6e4cecfdd156531cadd71b7d","observation_id":"573b9fb4-3b3f-44e0-8494-f2d8ed845648","resolution":{"observed_at":"2026-08-11T18:36:01.053400Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.16366","last_updated":"2023-03-28T12:40:25Z","snapshot_observed_at":"2026-08-03T16:06:46.576194Z","submitted_at":"2022-10-28T19:01:58Z","title":"Second release of the CoRe database of binary neutron star merger waveforms","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.16366","snapshot_observed_at":"2026-08-11T18:36:01.059909Z","title":"Gonzalez et al., Class","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.059909Z"},"links":{"cited_paper":"/paper/2210.16366","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:e684604f6ebf8cb928ffa82246a7934111acdcdd3b35b39ba3e6929534c45fd7","observation_id":"f64c785a-2ead-402d-8963-42fc6c852d13","resolution":{"observed_at":"2026-08-11T18:36:01.059909Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.11491","last_updated":"2022-10-20T18:00:05Z","snapshot_observed_at":"2026-07-06T14:08:22.637175Z","submitted_at":"2022-10-20T18:00:05Z","title":"Binary neutron star merger simulations with neutrino transport and turbulent viscosity: impact of different schemes and grid resolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.11491","snapshot_observed_at":"2026-08-11T18:36:01.066426Z","title":"Zappa, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.066426Z"},"links":{"cited_paper":"/paper/2210.11491","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:59a53e05381b90f729f059e632574e9050ffe4815342ddcba370950c17334a54","observation_id":"8a00095c-268d-4ed7-84a6-a30b8e438603","resolution":{"observed_at":"2026-08-11T18:36:01.066426Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0610128","last_updated":"2006-10-26T17:23:13Z","snapshot_observed_at":"2026-07-07T03:23:14.583543Z","submitted_at":"2006-10-26T17:23:13Z","title":"Calibration of Moving Puncture Simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0610128","snapshot_observed_at":"2026-08-11T18:36:01.073130Z","title":"Bruegmann, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.073130Z"},"links":{"cited_paper":"/paper/gr-qc/0610128","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:670eb42c718b7b0ab05f9537666d9421f98de14520147f99c8d8287f785961c9","observation_id":"4bd84e00-df94-4e28-ab89-8251102fd9f6","resolution":{"observed_at":"2026-08-11T18:36:01.073130Z","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":"2026-08-11T18:36:01.078925Z","title":"Thierfelder, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.078925Z"},"links":{"cited_paper":"/paper/1104.4751","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:7be517faf21cacbd5d40518004094f3e8d38d78e4ed4f1a56b12b5dbd0f71a8c","observation_id":"53cf7b4d-bd73-4123-b23a-74928711c0ed","resolution":{"observed_at":"2026-08-11T18:36:01.078925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.6502","last_updated":"2012-10-22T08:09:07Z","snapshot_observed_at":"2026-07-06T02:50:48.420841Z","submitted_at":"2012-06-27T20:00:19Z","title":"THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.6502","snapshot_observed_at":"2026-08-11T18:36:01.087262Z","title":"Radice and L","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.087262Z"},"links":{"cited_paper":"/paper/1206.6502","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:ebbbb4b438d19151d4180f4a2a1b44b4c00bfe3f7226dd1c482983d8e71e9b63","observation_id":"97a2e395-bc95-4068-aefa-d34acb87f360","resolution":{"observed_at":"2026-08-11T18:36:01.087262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.5004","last_updated":"2014-02-20T17:59:38Z","snapshot_observed_at":"2026-08-10T14:54:19.071745Z","submitted_at":"2013-12-17T23:36:43Z","title":"High-Order Fully General-Relativistic Hydrodynamics: new Approaches and Tests","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.5004","snapshot_observed_at":"2026-08-11T18:36:01.095461Z","title":"Radice, L","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.095461Z"},"links":{"cited_paper":"/paper/1312.5004","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:add9b95f45fc818b884e18025f1e904e3836215a7652e5259a50896c5f408c39","observation_id":"7a1b916e-6bb7-4d8a-a0f0-ced541b9bcbe","resolution":{"observed_at":"2026-08-11T18:36:01.095461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.00551","last_updated":"2015-02-02T17:10:41Z","snapshot_observed_at":"2026-08-06T20:25:05.697765Z","submitted_at":"2015-02-02T17:10:41Z","title":"High-Order Numerical-Relativity Simulations of Binary Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.00551","snapshot_observed_at":"2026-08-11T18:36:01.101476Z","title":"Radice, L","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.101476Z"},"links":{"cited_paper":"/paper/1502.00551","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:60b1bc36396bda576352ee895274379bf101bd2a8d9db7f39284050e0213cda7","observation_id":"78d507b2-7339-4af6-bf83-29d0645a7313","resolution":{"observed_at":"2026-08-11T18:36:01.101476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6244","last_updated":"2014-06-06T16:44:21Z","snapshot_observed_at":"2026-07-06T03:36:55.289462Z","submitted_at":"2014-02-25T17:07:42Z","title":"Quasiuniversal properties of neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.6244","snapshot_observed_at":"2026-08-11T18:36:01.107230Z","title":"Bernuzzi, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.107230Z"},"links":{"cited_paper":"/paper/1402.6244","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:d635863c785836aa6818faa8de1f73f869d962ebbe720841305ba3106777281e","observation_id":"a8d80832-9a5d-4f67-85ec-64fc6286e90c","resolution":{"observed_at":"2026-08-11T18:36:01.107230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.12644","last_updated":"2024-03-01T03:03:14Z","snapshot_observed_at":"2026-07-06T16:22:14.069796Z","submitted_at":"2023-09-22T06:29:24Z","title":"Maximum gravitational mass $M_{\\rm TOV}=2.25^{+0.08}_{-0.07}M_\\odot$ inferred at about $3\\%$ precision with multimessenger data of neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.12644","snapshot_observed_at":"2026-08-11T18:36:01.112742Z","title":"Fan, M.-Z","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.112742Z"},"links":{"cited_paper":"/paper/2309.12644","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:42d9a49c010ed25b62d6aba444f63f11e64b8b645e8e04d2c2a786722a00bd6d","observation_id":"1b70de86-97c4-4293-932f-8dbf925b9e3e","resolution":{"observed_at":"2026-08-11T18:36:01.112742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04872","last_updated":"2019-12-09T18:26:13Z","snapshot_observed_at":"2026-08-11T03:54:17.183217Z","submitted_at":"2019-07-10T18:01:08Z","title":"Spiral-wave wind for the blue kilonova","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04872","snapshot_observed_at":"2026-08-11T18:36:01.119276Z","title":"Nedora, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.119276Z"},"links":{"cited_paper":"/paper/1907.04872","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:658e2f3b679a05636ce27c06aa50a0a7afc3e3433a683bc67dcdcaadec95297e","observation_id":"067ebe0b-0fe2-4b8e-abde-fb0f48499b76","resolution":{"observed_at":"2026-08-11T18:36:01.119276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.11110","last_updated":"2021-11-11T21:01:43Z","snapshot_observed_at":"2026-07-06T10:16:47.864366Z","submitted_at":"2020-11-22T21:29:00Z","title":"Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.11110","snapshot_observed_at":"2026-08-11T18:36:01.124736Z","title":"Nedora, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.124736Z"},"links":{"cited_paper":"/paper/2011.11110","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:1b7d645832ed81302192e9cd6a44ab7fbfee62fd80b99ae6ebe7322ed3356a97","observation_id":"e7f84cf7-b08f-4290-98aa-4d9aa04a2b49","resolution":{"observed_at":"2026-08-11T18:36:01.124736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.18185","last_updated":"2025-07-11T12:52:43Z","snapshot_observed_at":"2026-08-01T23:29:05.874114Z","submitted_at":"2024-09-26T18:00:13Z","title":"Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.18185","snapshot_observed_at":"2026-08-11T18:36:01.129795Z","title":"Bernuzzi, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.129795Z"},"links":{"cited_paper":"/paper/2409.18185","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:5839738f37d30ddb074c6ac93bf4d037094f46a26ce6a61148d66f339379a18f","observation_id":"022663e7-a481-47e0-8187-2eb36dba2584","resolution":{"observed_at":"2026-08-11T18:36:01.129795Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.07750","last_updated":"2018-02-21T19:04:09Z","snapshot_observed_at":"2026-08-10T08:02:58.652817Z","submitted_at":"2018-02-21T19:04:09Z","title":"Effects of Fall-Back Accretion on Proto-Magnetar Outflows in Gamma-Ray Bursts and Superluminous Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.07750","snapshot_observed_at":"2026-08-11T18:36:01.135778Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.135778Z"},"links":{"cited_paper":"/paper/1802.07750","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:cc37998e440f2e16ba9ebaead5af4d802dea7228637930ec5a926ddcaf2caaaf","observation_id":"40fa33a4-e3b0-451e-b567-678991268927","resolution":{"observed_at":"2026-08-11T18:36:01.135778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12284","last_updated":"2023-12-08T07:36:41Z","snapshot_observed_at":"2026-08-10T16:08:34.503222Z","submitted_at":"2023-03-22T03:23:27Z","title":"Jets from neutron-star merger remnants and massive blue kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12284","snapshot_observed_at":"2026-08-11T18:36:01.141200Z","title":"Combi and D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.141200Z"},"links":{"cited_paper":"/paper/2303.12284","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:924bcc1e43663517712e5246a7cb116069597233e4f5a952feb3e68a341618b8","observation_id":"07e0ffc3-6980-4a07-89d7-1d3f7cfb2493","resolution":{"observed_at":"2026-08-11T18:36:01.141200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.04461","last_updated":"2021-05-06T12:34:33Z","snapshot_observed_at":"2026-07-06T10:02:54.326546Z","submitted_at":"2020-10-09T09:41:23Z","title":"Systematics of prompt black-hole formation in neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.04461","snapshot_observed_at":"2026-08-11T18:36:01.146621Z","title":"Bauswein, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.146621Z"},"links":{"cited_paper":"/paper/2010.04461","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:327c895e6d076fae0b59340f6d595bcca43cc82916069c7d3c5b3d44223d9cff","observation_id":"f681e30f-e5bc-4f7d-b122-2bc85129d9f0","resolution":{"observed_at":"2026-08-11T18:36:01.146621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.00940","last_updated":"2021-11-01T12:01:33Z","snapshot_observed_at":"2026-08-12T12:49:41.036419Z","submitted_at":"2021-09-02T13:31:03Z","title":"Quasi-universal behaviour of the threshold mass in unequal-mass, spinning binary neutron-star mergers","version":2},"cited_work":{"arxiv_id":"2109.00940","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.00940","snapshot_observed_at":"2026-08-11T18:36:01.257654Z","title":"Quasi-universal behaviour of the threshold mass in unequal-mass, spinning binary neutron-star mergers","venue":"gr-qc","work_id":"5b89cdaf-7476-42f4-b150-6b60e8746537","year":2021},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.152786Z"},"links":{"cited_paper":"/paper/2109.00940","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:e5654a5005891501bdd6551da996c9018b03b77f96b51b0aaba3221dab3bcc6c","observation_id":"39b51cd2-1a96-4ae6-ac34-0242fdb0a6cf","resolution":{"observed_at":"2026-08-11T18:36:01.264310Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.11851","last_updated":"2021-12-22T12:58:07Z","snapshot_observed_at":"2026-08-05T04:03:55.827485Z","submitted_at":"2021-12-22T12:58:07Z","title":"Investigating the mass-ratio dependence of the prompt-collapse threshold with numerical-relativity simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.11851","snapshot_observed_at":"2026-08-11T18:36:01.158528Z","title":"K¨ olsch, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.158528Z"},"links":{"cited_paper":"/paper/2112.11851","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:9d1530eabe35da9742c2678a96d6599f3e0a11a0d54d01efc64679ced5db0d9a","observation_id":"2b061f6b-39a9-4e09-b6e3-a07e164074d2","resolution":{"observed_at":"2026-08-11T18:36:01.158528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.02415","last_updated":"2020-03-25T08:32:07Z","snapshot_observed_at":"2026-07-06T08:42:12.220605Z","submitted_at":"2019-12-05T07:36:47Z","title":"Modelling Double Neutron Stars: Radio and Gravitational Waves","version":4},"cited_work":{"arxiv_id":"1912.02415","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.02415","snapshot_observed_at":"2026-08-11T18:36:01.211125Z","title":"Modelling Double Neutron Stars: Radio and Gravitational Waves","venue":"astro-ph.HE","work_id":"14362c22-c8c3-4dc8-890a-0c297e5271c0","year":2019},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:01.163906Z"},"links":{"cited_paper":"/paper/1912.02415","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:1b6a342e7ab01fbc83e0586be6ff963b31411b1c8e21f51b3e9c86fea6a0c010","observation_id":"cf6f87fd-a655-4129-aad6-b6cf34771e40","resolution":{"observed_at":"2026-08-11T18:36:01.218725Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-11T19:15:42.421284Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars"},"reference_resolution":{"displayed":91,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":78,"verified_exact":13,"verified_fuzzy":0},"total_outbound_references":91},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 91 of 91 outbound references and 1 inbound Pith citation observation for arXiv:2412.07846."}