{"as_of":"2026-08-08T20:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4213e3fb6c85e4c10cec1da1ac8297f024484096a297d7d4713b598bfefc22ac","coverage":[{"denominator":136,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T00:43:19.676262Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.04092/citation-record","integrity":"/paper/2608.04092/integrity","json":"/paper/2608.04092/citation-record.json","paper":"/paper/2608.04092"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1607.03540","last_updated":"2017-03-22T21:26:33Z","snapshot_observed_at":"2026-07-06T05:03:20.569229Z","submitted_at":"2016-07-12T23:03:39Z","title":"Binary neutron-star mergers: a review of Einstein's richest laboratory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03540","snapshot_observed_at":"2026-08-08T00:43:18.892648Z","title":"Baiotti and L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.892648Z"},"links":{"cited_paper":"/paper/1607.03540","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:c798a20f3566cfb78eed48c2b13f0416b1d41eefac962681e4369889a3091c93","observation_id":"1a7a51b9-2de1-444c-befc-3ae6cf190356","resolution":{"observed_at":"2026-08-08T00:43:18.892648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.02350","last_updated":"2019-08-06T20:23:10Z","snapshot_observed_at":"2026-07-06T08:12:49.194429Z","submitted_at":"2019-08-06T20:23:10Z","title":"Merger and Mass Ejection of Neutron-Star Binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.02350","snapshot_observed_at":"2026-08-08T00:43:18.897747Z","title":"Shibata and K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.897747Z"},"links":{"cited_paper":"/paper/1908.02350","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:63aa8ca4d9552fb5e45bc050fe8a5052df21a1e5bb9c725ed614d5eb14948f64","observation_id":"7220bd01-8241-4667-87cc-957790976424","resolution":{"observed_at":"2026-08-08T00:43:18.897747Z","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":"2026-08-08T01:11:42.313131Z","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":"2026-08-08T00:43:18.902810Z","title":"Radice, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.902810Z"},"links":{"cited_paper":"/paper/2002.03863","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:5d72406726e732e95b489c021726aca0c5530c74213c4674bace6107f3b23f9f","observation_id":"dc9a8695-d7ab-40ce-8f07-abd205c0d9eb","resolution":{"observed_at":"2026-08-08T00:43:18.902810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06419","last_updated":"2020-10-25T11:10:09Z","snapshot_observed_at":"2026-07-06T09:12:10.157011Z","submitted_at":"2020-04-14T11:04:04Z","title":"Neutron Star Merger Remnants","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06419","snapshot_observed_at":"2026-08-08T00:43:18.909533Z","title":"Bernuzzi, Gen.Rel.Grav.52, 108 (2020), arXiv:2004.06419 [astro-ph.HE]","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.909533Z"},"links":{"cited_paper":"/paper/2004.06419","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:b5677105ae2597cf2219f7875a745bc05e7bac4768648333eed675b402e6968c","observation_id":"a1cfa3d6-7b78-4ac6-ac77-50ebd0fec7a7","resolution":{"observed_at":"2026-08-08T00:43:18.909533Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.4553","last_updated":"2015-05-13T14:07:20Z","snapshot_observed_at":"2026-08-03T21:35:03.622564Z","submitted_at":"2014-12-15T11:55:06Z","title":"Modeling the dynamics of tidally-interacting binary neutron stars up to merger","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.4553","snapshot_observed_at":"2026-08-08T00:43:18.932685Z","title":"Bernuzzi, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.932685Z"},"links":{"cited_paper":"/paper/1412.4553","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:9f603405a3cc05fbaefda576e470d26c9c1dbe5564b2cf8ca4c0281713578087","observation_id":"10cdfeca-e2f1-4b58-9391-bca1da1e6a3b","resolution":{"observed_at":"2026-08-08T00:43:18.932685Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07456","last_updated":"2024-07-16T08:23:55Z","snapshot_observed_at":"2026-08-05T15:50:26.974469Z","submitted_at":"2023-11-13T16:41:19Z","title":"New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.07456","snapshot_observed_at":"2026-08-08T00:43:18.938178Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.938178Z"},"links":{"cited_paper":"/paper/2311.07456","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:5e9f1ff8289a1f39b083a9e359f6b9f6da42c84056e94dd4a5d6e88dc48d6e90","observation_id":"cee134bd-dabc-4ef9-8b87-eb2cbdadaaaf","resolution":{"observed_at":"2026-08-08T00:43:18.938178Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.11418","last_updated":"2020-01-20T15:41:47Z","snapshot_observed_at":"2026-08-05T23:57:43.650321Z","submitted_at":"2019-08-29T18:41:11Z","title":"kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.11418","snapshot_observed_at":"2026-08-08T00:43:18.948346Z","title":"Breschi, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.948346Z"},"links":{"cited_paper":"/paper/1908.11418","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:e55d1a0a30503eba3c4991006c7da5695f825b5e17a563265dd23a50551b5281","observation_id":"422fe9b3-74ed-4cb4-b744-f2a0290d5727","resolution":{"observed_at":"2026-08-08T00:43:18.948346Z","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":"2026-08-08T00:43:18.956459Z","title":"Kashyap, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.956459Z"},"links":{"cited_paper":"/paper/2111.05183","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:073d8257708e0190e5d44b76ebd6f36495e8e274935fc78faa63029a58126ac2","observation_id":"84516551-4d2b-4278-8323-f49cbaf0bb1e","resolution":{"observed_at":"2026-08-08T00:43:18.956459Z","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":"2026-08-08T00:43:18.963170Z","title":"Perego, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.963170Z"},"links":{"cited_paper":"/paper/2112.05864","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:1f2fdb2353f71561a951ebfef7d81bb832cf9872740220a91d835211813295fd","observation_id":"3c34be60-7a87-417f-a7c3-f7c0efd2c370","resolution":{"observed_at":"2026-08-08T00:43:18.963170Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.04333","last_updated":"2020-08-12T14:46:52Z","snapshot_observed_at":"2026-08-06T02:47:43.822013Z","submitted_at":"2020-08-10T18:00:46Z","title":"Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and Nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.04333","snapshot_observed_at":"2026-08-08T00:43:18.968889Z","title":"Nedora, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.968889Z"},"links":{"cited_paper":"/paper/2008.04333","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:01cdc18914a22601cd79d071f37d3c347478ef3e5b67ecf8cedb319802ac1794","observation_id":"cf2d00d6-c5a5-4393-b4f5-2e90eb951b08","resolution":{"observed_at":"2026-08-08T00:43:18.968889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07637","last_updated":"2023-06-27T13:42:40Z","snapshot_observed_at":"2026-07-06T14:18:10.647862Z","submitted_at":"2022-11-14T18:59:53Z","title":"Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07637","snapshot_observed_at":"2026-08-08T00:43:18.975565Z","title":"Kiuchi, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.975565Z"},"links":{"cited_paper":"/paper/2211.07637","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:7e9f5c5634d9c0fb46c8a0c6f4b40090357a2e4e9a415c4a541e45687c6020d8","observation_id":"3b8236d0-a88d-4c27-8a73-4447d6ea4f2e","resolution":{"observed_at":"2026-08-08T00:43:18.975565Z","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":"2026-08-08T00:43:18.983958Z","title":"Neuweiler, H","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.983958Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:34159ffd74eb9e60e1a196f8ecc7ccb805052e459e78cc5888ffb1cfd7328ced","observation_id":"090507aa-ab59-44de-85e4-79a769641b7d","resolution":{"observed_at":"2026-08-08T00:43:18.983958Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2512.11032","last_updated":"2026-04-01T12:05:36Z","snapshot_observed_at":"2026-07-06T22:38:50.534580Z","submitted_at":"2025-12-11T19:00:02Z","title":"Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.11032","snapshot_observed_at":"2026-08-08T00:43:18.988679Z","title":"Magistrelli, S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.988679Z"},"links":{"cited_paper":"/paper/2512.11032","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:8def4e4aeb91dcb1dc8e33f3c99bedebb8f89dc3710453b41ba542ad2b62fb87","observation_id":"98313a13-410e-4b8d-a5c9-531a87f7869f","resolution":{"observed_at":"2026-08-08T00:43:18.988679Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5191","last_updated":"2013-09-08T12:12:06Z","snapshot_observed_at":"2026-07-06T03:18:39.319674Z","submitted_at":"2013-07-19T12:03:45Z","title":"Prompt merger collapse and the maximum mass of neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.5191","snapshot_observed_at":"2026-08-08T00:43:18.994207Z","title":"Bauswein, T","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.994207Z"},"links":{"cited_paper":"/paper/1307.5191","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:88f21e71c5b59b41dc020b959a7312b451b75ad257cdf09105de40e9f713ce11","observation_id":"bb761f38-cc6f-47dc-a78a-ca84a0ab3c7c","resolution":{"observed_at":"2026-08-08T00:43:18.994207Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.04621","last_updated":"2023-04-26T13:36:17Z","snapshot_observed_at":"2026-07-06T12:06:35.380847Z","submitted_at":"2021-11-08T16:48:57Z","title":"General-relativistic neutrino-radiation magnetohydrodynamic simulation of seconds-long black hole-neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.04621","snapshot_observed_at":"2026-08-08T00:43:19.001654Z","title":"Hayashi, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.001654Z"},"links":{"cited_paper":"/paper/2111.04621","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:4184a13d7209589c9d2cfc68496e22ac2c78aa0403f72a29980a7f29773898da","observation_id":"75427b5b-29a3-40ba-962f-3ab4182615e5","resolution":{"observed_at":"2026-08-08T00:43:19.001654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-08T00:43:19.007075Z","title":"Kiuchi, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.007075Z"},"links":{"cited_paper":"/paper/2306.15721","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:db6db305894b89873d3f748d00488d2fccb240be108d0f2f5b7579849e1a1172","observation_id":"a469e390-f80f-4f34-a5e4-35072b5ea4ca","resolution":{"observed_at":"2026-08-08T00:43:19.007075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.06253","last_updated":"2024-10-08T18:00:02Z","snapshot_observed_at":"2026-07-06T19:29:55.838200Z","submitted_at":"2024-10-08T18:00:02Z","title":"On the impact of neutrinos on the launching of relativistic jets from \"magnetars\" produced in neutron-star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.06253","snapshot_observed_at":"2026-08-08T00:43:19.013480Z","title":"Musolino, L","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.013480Z"},"links":{"cited_paper":"/paper/2410.06253","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:95aed90ebb4f9f9edd046935910a9e7832a8a1e7c1e6987c9f56fe9c82cf8dd4","observation_id":"414f9147-fd60-4c3a-9108-9c989b71b859","resolution":{"observed_at":"2026-08-08T00:43:19.013480Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.4662","last_updated":"2013-07-22T10:12:05Z","snapshot_observed_at":"2026-07-06T03:09:06.441862Z","submitted_at":"2013-03-19T16:57:33Z","title":"Equation of state and neutron star properties constrained by nuclear physics and observation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.4662","snapshot_observed_at":"2026-08-08T00:43:19.022818Z","title":"Hebeler, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.022818Z"},"links":{"cited_paper":"/paper/1303.4662","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:004a4beb2cacaf6f0f994e0608f0c51dfc0588b8f75ab4889b72a77d472681d9","observation_id":"fff90475-bd2e-4e29-833b-c8065df10bfd","resolution":{"observed_at":"2026-08-08T00:43:19.022818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.03470","last_updated":"2016-02-17T11:44:26Z","snapshot_observed_at":"2026-07-06T04:29:34.167550Z","submitted_at":"2015-09-11T12:13:42Z","title":"Chiral Three-Nucleon Interactions in Light Nuclei, Neutron-$\\alpha$ Scattering, and Neutron Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.03470","snapshot_observed_at":"2026-08-08T00:43:19.029265Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.029265Z"},"links":{"cited_paper":"/paper/1509.03470","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:afed8246cc24de4f753ab30c7340c68deea6126d54532b691734622386f9ae3f","observation_id":"18d0e8be-5c7a-4669-aa31-fec81220a2ba","resolution":{"observed_at":"2026-08-08T00:43:19.029265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.07232","last_updated":"2021-01-07T17:48:00Z","snapshot_observed_at":"2026-07-06T09:12:35.818953Z","submitted_at":"2020-04-15T17:45:51Z","title":"How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.07232","snapshot_observed_at":"2026-08-08T00:43:19.035637Z","title":"Drischler, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.035637Z"},"links":{"cited_paper":"/paper/2004.07232","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:ff03e21f8f1d4a76603c6330fc6df4c0d0f16daec83760d7a0c913fb13a61bce","observation_id":"e2f9b015-ef48-4890-8c80-0e2291423fd9","resolution":{"observed_at":"2026-08-08T00:43:19.035637Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.09411","last_updated":"2020-05-07T19:21:41Z","snapshot_observed_at":"2026-08-07T03:04:38.721983Z","submitted_at":"2019-12-19T17:28:08Z","title":"Nuclear and neutron-star matter from local chiral interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.09411","snapshot_observed_at":"2026-08-08T00:43:19.041108Z","title":"Lonardoni, I","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.041108Z"},"links":{"cited_paper":"/paper/1912.09411","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:3cf91d20b02f667298578bcca1db29f80c1f84fa9dc95a73e413fa8a578ddbc1","observation_id":"8e445af8-84ee-4938-b32c-8a645e6c643b","resolution":{"observed_at":"2026-08-08T00:43:19.041108Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.14016","last_updated":"2023-02-20T13:50:33Z","snapshot_observed_at":"2026-08-06T12:59:07.272128Z","submitted_at":"2022-04-29T11:04:31Z","title":"Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.14016","snapshot_observed_at":"2026-08-08T00:43:19.049978Z","title":"Keller, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.049978Z"},"links":{"cited_paper":"/paper/2204.14016","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:eccb53ab2220a430391f9246859341adfc6f626423740f137982be6de917b451","observation_id":"59130c88-8f4e-4d0f-bc98-3d152882893a","resolution":{"observed_at":"2026-08-08T00:43:19.049978Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2512.19593","last_updated":"2026-05-12T14:40:42Z","snapshot_observed_at":"2026-08-02T05:32:26.370206Z","submitted_at":"2025-12-22T17:25:18Z","title":"Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.19593","snapshot_observed_at":"2026-08-08T00:43:19.055710Z","title":"G¨ ottling, L","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.055710Z"},"links":{"cited_paper":"/paper/2512.19593","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:765fce109af3cfe3f1b688035216f7f9e205ed3b91fd38cc770a717ab45b9115","observation_id":"4b4bf6e0-80e6-4c00-8816-eb44bcfb45eb","resolution":{"observed_at":"2026-08-08T00:43:19.055710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.05350","last_updated":"2022-05-18T17:15:43Z","snapshot_observed_at":"2026-07-06T12:07:02.414603Z","submitted_at":"2021-11-09T19:00:03Z","title":"How perturbative QCD constrains the Equation of State at Neutron-Star densities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.05350","snapshot_observed_at":"2026-08-08T00:43:19.060431Z","title":"Komoltsev and A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.060431Z"},"links":{"cited_paper":"/paper/2111.05350","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:81ffff0886b300794d5b555650798f4b299c8621d31895201138b29f6c7fb4e5","observation_id":"7d6d9ecb-4c02-4a4d-8e62-79071d36bc4b","resolution":{"observed_at":"2026-08-08T00:43:19.060431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11877","last_updated":"2023-07-28T10:24:09Z","snapshot_observed_at":"2026-08-01T18:59:51.050777Z","submitted_at":"2022-04-25T18:00:03Z","title":"Ab-initio QCD calculations impact the inference of the neutron-star-matter equation of state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11877","snapshot_observed_at":"2026-08-08T00:43:19.065496Z","title":"Gorda, O","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.065496Z"},"links":{"cited_paper":"/paper/2204.11877","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:f9283ba09296e9d86725e8b23f34428d96ce25a31009b10886d3ff4f97e0112e","observation_id":"7ac63a30-7a47-4fb1-b383-135a977fc8e1","resolution":{"observed_at":"2026-08-08T00:43:19.065496Z","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":"2026-08-08T00:43:19.073371Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.073371Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:1d11adbb1cd3a651a8cc746ead7d2e68cc7dc41237440f2a67285faebf0c670c","observation_id":"5e95ff77-325c-4fea-be25-c921e8d03fd7","resolution":{"observed_at":"2026-08-08T00:43:19.073371Z","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":"2026-08-08T00:43:19.087206Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.087206Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:478aea4e1b64bf7b00ae13473c4b02e1beaa45d8a54e656558770ad8a96078b7","observation_id":"04a5b00b-e5cb-4f19-8baf-1dd8a309daec","resolution":{"observed_at":"2026-08-08T00:43:19.087206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11579","last_updated":"2019-01-22T19:56:03Z","snapshot_observed_at":"2026-07-06T06:41:51.126097Z","submitted_at":"2018-05-29T16:55:48Z","title":"Properties of the binary neutron star merger GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11579","snapshot_observed_at":"2026-08-08T00:43:19.092392Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.092392Z"},"links":{"cited_paper":"/paper/1805.11579","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:eb19799a6e1ddfe3c90a7b2cdcab73a50720ba4ef8d7b1fe7e02e6497908d316","observation_id":"cf5a9cbf-8ffd-417c-848b-e5dac32bd34c","resolution":{"observed_at":"2026-08-08T00:43:19.092392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05702","last_updated":"2019-12-12T00:04:38Z","snapshot_observed_at":"2026-07-06T08:43:55.093635Z","submitted_at":"2019-12-12T00:04:38Z","title":"A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05702","snapshot_observed_at":"2026-08-08T00:43:19.097129Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.097129Z"},"links":{"cited_paper":"/paper/1912.05702","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:310b9d3c8c30835853c6b2444f4f52aa7751c9e5ffda3cc6bb269579837233cd","observation_id":"21b48eb6-60a0-4611-be12-7162e8e5aaa6","resolution":{"observed_at":"2026-08-08T00:43:19.097129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05705","last_updated":"2019-12-12T00:04:41Z","snapshot_observed_at":"2026-07-31T21:20:48.579404Z","submitted_at":"2019-12-12T00:04:41Z","title":"PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05705","snapshot_observed_at":"2026-08-08T00:43:19.103441Z","title":"Miller, F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.103441Z"},"links":{"cited_paper":"/paper/1912.05705","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:5181c06766e77a51d9503b23c09b11f46b6a2a329576c0da0cf71872fc66a804","observation_id":"3c4622a8-1ce8-45f9-a3a6-74ed028bde2e","resolution":{"observed_at":"2026-08-08T00:43:19.103441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06980","last_updated":"2021-09-22T12:10:14Z","snapshot_observed_at":"2026-08-02T16:55:34.407604Z","submitted_at":"2021-05-14T17:33:33Z","title":"A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06980","snapshot_observed_at":"2026-08-08T00:43:19.116358Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.116358Z"},"links":{"cited_paper":"/paper/2105.06980","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:a0fb1bf9f9685d1c46f88467a1fab6fea61f8f294b9234e1184c0c242d5a9d4c","observation_id":"03f18dc7-3be5-41b5-b9e1-2f7043dd064e","resolution":{"observed_at":"2026-08-08T00:43:19.116358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06979","last_updated":"2021-05-14T17:33:32Z","snapshot_observed_at":"2026-08-07T18:52:26.425716Z","submitted_at":"2021-05-14T17:33:32Z","title":"The Radius of PSR J0740+6620 from NICER and XMM-Newton Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06979","snapshot_observed_at":"2026-08-08T00:43:19.123323Z","title":"Miller, F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.123323Z"},"links":{"cited_paper":"/paper/2105.06979","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:77eab9b6317696b8a97468d40f3c3a61bfc4de42fb5396cf9af4ef840fa73344","observation_id":"bd0698dd-35b6-471e-a89a-6982973bf815","resolution":{"observed_at":"2026-08-08T00:43:19.123323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.14466","last_updated":"2024-10-25T09:48:05Z","snapshot_observed_at":"2026-07-06T18:34:19.513528Z","submitted_at":"2024-06-20T16:30:01Z","title":"The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.14466","snapshot_observed_at":"2026-08-08T00:43:19.132730Z","title":"Salmi et al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.132730Z"},"links":{"cited_paper":"/paper/2406.14466","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:ec9c875d362e730c632f487b745cf7b13e061bdce22213b3f061a3a60d487ac5","observation_id":"c031f194-0423-4448-ad74-cca76de05a3f","resolution":{"observed_at":"2026-08-08T00:43:19.132730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.06789","last_updated":"2024-07-09T12:00:43Z","snapshot_observed_at":"2026-08-02T09:13:57.621070Z","submitted_at":"2024-07-09T12:00:43Z","title":"A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\\unicode{x2013}$4715","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.06789","snapshot_observed_at":"2026-08-08T00:43:19.144191Z","title":"Choudhury et al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.144191Z"},"links":{"cited_paper":"/paper/2407.06789","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:77b0442be7ded8ceaf72e1734a7e8b1e1d235fe50e9f37bcd6de3afc9272f11d","observation_id":"b4886441-3f05-42ac-bd82-89b1564191e3","resolution":{"observed_at":"2026-08-08T00:43:19.144191Z","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":"2026-08-08T00:43:19.151867Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.151867Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:e863889564a78d58a0cc01a724c04a0016eeaf2252d013bf1cd6574728576e6f","observation_id":"da23c8c3-2bd8-4662-a7c6-92e0c800ff64","resolution":{"observed_at":"2026-08-08T00:43:19.151867Z","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":"2026-08-08T00:43:19.156303Z","title":"Mauviard, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.156303Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:fbded256db063a715cce3a15a848b8f97d437039252aaf5eceae8a340b192899","observation_id":"9259dfee-6a44-487b-bcd7-711282957969","resolution":{"observed_at":"2026-08-08T00:43:19.156303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6875","last_updated":"2013-04-25T11:01:50Z","snapshot_observed_at":"2026-07-06T03:12:01.430759Z","submitted_at":"2013-04-25T11:01:50Z","title":"A Massive Pulsar in a Compact Relativistic Binary","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.6875","snapshot_observed_at":"2026-08-08T00:43:19.163964Z","title":"Antoniadis, P","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.163964Z"},"links":{"cited_paper":"/paper/1304.6875","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:18ec3cc2066a20867310f8926db1c39374c045b3ca76d3a99b42de3b9bf91780","observation_id":"f646bbf5-c7e6-4c99-971c-d902c9c9f5e0","resolution":{"observed_at":"2026-08-08T00:43:19.163964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.00880","last_updated":"2021-07-06T17:59:37Z","snapshot_observed_at":"2026-08-03T18:03:00.153543Z","submitted_at":"2021-04-02T04:26:41Z","title":"Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.00880","snapshot_observed_at":"2026-08-08T00:43:19.169166Z","title":"Fonseca et al., Astrophys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.169166Z"},"links":{"cited_paper":"/paper/2104.00880","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:8f7fb95f6fbace746c9a6818e6b9413f61f247f08f8ddf45ce774d733de8e91c","observation_id":"19460ced-0064-409e-acd8-757057851e09","resolution":{"observed_at":"2026-08-08T00:43:19.169166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.2163","last_updated":"2008-12-11T14:59:23Z","snapshot_observed_at":"2026-07-06T01:47:44.956336Z","submitted_at":"2008-12-11T14:59:23Z","title":"Constraints on a phenomenologically parameterized neutron-star equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.2163","snapshot_observed_at":"2026-08-08T00:43:19.189691Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.189691Z"},"links":{"cited_paper":"/paper/0812.2163","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:ef6096f86c9158f3975dce9aeae78da47bc712c04f6d4b5701e4fcadafbc16b6","observation_id":"3f7b3020-0b73-44a0-b14c-df7ffbb89f97","resolution":{"observed_at":"2026-08-08T00:43:19.189691Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01923","last_updated":"2018-06-25T20:56:27Z","snapshot_observed_at":"2026-07-06T06:17:24.959986Z","submitted_at":"2018-01-05T21:28:09Z","title":"Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01923","snapshot_observed_at":"2026-08-08T00:43:19.207336Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.207336Z"},"links":{"cited_paper":"/paper/1801.01923","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:aa239807b318bc5fae1a1bc8bbb711abadb6a5156539ecbb785bc324e201a008","observation_id":"93b18c37-04d2-487f-8cf0-5084ea171589","resolution":{"observed_at":"2026-08-08T00:43:19.207336Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.08188","last_updated":"2019-03-06T08:09:48Z","snapshot_observed_at":"2026-07-31T03:26:53.081341Z","submitted_at":"2018-12-19T19:00:19Z","title":"Equation of state sensitivities when inferring neutron star and dense matter properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.08188","snapshot_observed_at":"2026-08-08T00:43:19.222530Z","title":"Greif, G","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.222530Z"},"links":{"cited_paper":"/paper/1812.08188","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:dfab46eca517b91b3969feecae68c28bd4e1d78f8597a82a409776caa6a8efb0","observation_id":"53c08b6b-3d16-49ff-87c9-ea754b17d7b4","resolution":{"observed_at":"2026-08-08T00:43:19.222530Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12529","last_updated":"2018-12-05T18:19:00Z","snapshot_observed_at":"2026-07-06T07:18:06.398264Z","submitted_at":"2018-11-29T23:05:21Z","title":"Non-parametric inference of the neutron star equation of state from gravitational wave observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12529","snapshot_observed_at":"2026-08-08T00:43:19.236119Z","title":"Landry and R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.236119Z"},"links":{"cited_paper":"/paper/1811.12529","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:dc1e4307bf50fce56c98bcaf3e7c3dbbd281b990a170a42fcdfa3bf52883f5cf","observation_id":"37c8201f-8984-4ce6-9450-c4500a74a399","resolution":{"observed_at":"2026-08-08T00:43:19.236119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02644","last_updated":"2018-03-22T14:25:12Z","snapshot_observed_at":"2026-07-06T06:08:14.677196Z","submitted_at":"2017-11-07T18:06:28Z","title":"Gravitational-wave constraints on the neutron-star-matter Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02644","snapshot_observed_at":"2026-08-08T00:43:19.244697Z","title":"Annala, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.244697Z"},"links":{"cited_paper":"/paper/1711.02644","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:1f6984466b48c4e193d452bd5c3efd70e3e2e1b3cd40e52587af890f7ae985c8","observation_id":"e879f1b5-b8a8-4390-8b13-d02656e1f4a5","resolution":{"observed_at":"2026-08-08T00:43:19.244697Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.05313","last_updated":"2021-09-07T20:18:31Z","snapshot_observed_at":"2026-07-06T11:17:41.075986Z","submitted_at":"2021-06-09T18:08:05Z","title":"Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.05313","snapshot_observed_at":"2026-08-08T00:43:19.251386Z","title":"Legred, K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.251386Z"},"links":{"cited_paper":"/paper/2106.05313","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:cd091e167954dda100fcc126513bc49fcfde01cce236cf61848d5484910ac322","observation_id":"bdcaf0e9-af04-4850-a545-e64788374c67","resolution":{"observed_at":"2026-08-08T00:43:19.251386Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-08T00:43:19.258188Z","title":"Dietrich, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.258188Z"},"links":{"cited_paper":"/paper/2002.11355","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:bf139dc75b6828deae2247513e0d9b31a56673eb213370e9f5a8c1d7bba2ab3c","observation_id":"05446441-defc-43d0-b1db-b2df77547a4f","resolution":{"observed_at":"2026-08-08T00:43:19.258188Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06229","last_updated":"2022-06-24T14:44:52Z","snapshot_observed_at":"2026-08-06T00:47:36.743643Z","submitted_at":"2021-07-13T16:31:44Z","title":"Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06229","snapshot_observed_at":"2026-08-08T00:43:19.264856Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.264856Z"},"links":{"cited_paper":"/paper/2107.06229","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:765cfcf91e66b0c71536843f5572b6384a7ae2dfc09e4a996bbbee616d2dcd8b","observation_id":"ca349372-48c9-4d9b-ab5d-a247f1f37b3d","resolution":{"observed_at":"2026-08-08T00:43:19.264856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04172","last_updated":"2025-04-15T09:06:55Z","snapshot_observed_at":"2026-07-06T17:26:19.028623Z","submitted_at":"2024-02-06T17:27:09Z","title":"From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04172","snapshot_observed_at":"2026-08-08T00:43:19.270745Z","title":"Koehn, H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.270745Z"},"links":{"cited_paper":"/paper/2402.04172","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:871816799258671aded22121c4a99df2e396437c4a394a088f2639b1d882f1cc","observation_id":"b907bf0f-e113-48a7-b3f7-f8d75862f1ad","resolution":{"observed_at":"2026-08-08T00:43:19.270745Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.06790","last_updated":"2024-09-30T11:05:53Z","snapshot_observed_at":"2026-07-06T18:43:38.955120Z","submitted_at":"2024-07-09T12:00:44Z","title":"Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.06790","snapshot_observed_at":"2026-08-08T00:43:19.276392Z","title":"Rutherford et al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.276392Z"},"links":{"cited_paper":"/paper/2407.06790","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:ac6ffa748782e0e21f5d2c2f67357db3fc35f4cec594c98c126dfce151a3d515","observation_id":"85d1332e-0d2c-4c14-8dc8-c5ff33077288","resolution":{"observed_at":"2026-08-08T00:43:19.276392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.18560","last_updated":"2026-07-30T12:51:18Z","snapshot_observed_at":"2026-08-02T23:57:47.399690Z","submitted_at":"2026-05-18T15:40:59Z","title":"Astrophysics equation of state inference with Bayesian chiral effective field theory uncertainties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.18560","snapshot_observed_at":"2026-08-08T00:43:19.281610Z","title":"Mendes, H","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.281610Z"},"links":{"cited_paper":"/paper/2605.18560","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:b82bdc97cb6bbb011ac9cbe6aad3a823c6d8df81f6b0a1c0e4b0e37e720e53e7","observation_id":"558ff9cd-e38f-45ce-a0ab-cc6653218b14","resolution":{"observed_at":"2026-08-08T00:43:19.281610Z","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":"2026-08-08T00:43:18.887164Z","title":"Multimessenger Astronomy of 17 Neutron Star Mergers with Numerical Relativity","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:18.887164Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:a3d985285e6c442e5a422263ab8a74f1f1137954384bd2cfb0658013b1860053","observation_id":"1a9b81b1-97d5-4766-b19c-67eee5d700da","resolution":{"observed_at":"2026-08-08T00:43:18.887164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04063","last_updated":"2024-03-10T12:41:12Z","snapshot_observed_at":"2026-07-06T15:51:46.997267Z","submitted_at":"2023-07-08T23:56:25Z","title":"Symmetry energy and neutron star properties constrained by chiral effective field theory calculations","version":2},"cited_work":{"arxiv_id":"2307.04063","doi":null,"metadata_source":"pith","pith_arxiv_id":"2307.04063","snapshot_observed_at":"2026-08-08T00:43:22.454997Z","title":"Symmetry energy and neutron star properties constrained by chiral effective field theory calculations","venue":"nucl-th","work_id":"2b084701-33d0-4899-9be3-bc87529715c4","year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.303934Z"},"links":{"cited_paper":"/paper/2307.04063","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:704519067cfbe4701b443a8f8f2fe5a553d041d8545f05c51f8d4b5286694137","observation_id":"bb900ddf-237f-41ba-a75f-0a914213524b","resolution":{"observed_at":"2026-08-08T00:43:22.469761Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.02803","last_updated":"2018-07-18T17:56:20Z","snapshot_observed_at":"2026-07-06T06:27:07.831377Z","submitted_at":"2018-03-07T18:30:20Z","title":"Neutron star tidal deformabilities constrained by nuclear theory and experiment","version":2},"cited_work":{"arxiv_id":"1803.02803","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.02803","snapshot_observed_at":"2026-08-08T00:43:22.495604Z","title":"Neutron star tidal deformabilities constrained by nuclear theory and experiment","venue":"nucl-th","work_id":"94f63355-a9d1-44c3-ab80-8609908b7080","year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.297415Z"},"links":{"cited_paper":"/paper/1803.02803","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:8bcff29f2e2ed808304ee6037b307550e68f62a3ae533d06063f71eab7ec4819","observation_id":"78788fea-4175-4d7c-bb11-03a5019c2357","resolution":{"observed_at":"2026-08-08T00:43:22.502173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.19325","last_updated":"2024-08-21T09:22:06Z","snapshot_observed_at":"2026-08-07T20:17:40.935954Z","submitted_at":"2024-03-28T11:32:53Z","title":"Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.19325","snapshot_observed_at":"2026-08-08T00:43:19.315380Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.315380Z"},"links":{"cited_paper":"/paper/2403.19325","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:2233447453e9d1674f9c0a9f1ffae6503e6251e9585665c21e5bd0f021411fe8","observation_id":"7bc96916-ea7f-449b-b5b5-e24b74e42b5a","resolution":{"observed_at":"2026-08-08T00:43:19.315380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.15351","last_updated":"2024-02-27T09:00:45Z","snapshot_observed_at":"2026-07-06T16:11:51.259378Z","submitted_at":"2023-08-29T14:46:08Z","title":"Bayesian Survey of the Dense Matter Equation of State built upon Skyrme effective interactions","version":2},"cited_work":{"arxiv_id":"2308.15351","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.15351","snapshot_observed_at":"2026-08-08T00:43:22.418594Z","title":"Bayesian Survey of the Dense Matter Equation of State built upon Skyrme effective interactions","venue":"astro-ph.HE","work_id":"9f7a0ed3-7be6-4a95-b384-0f24ff5e2161","year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.309985Z"},"links":{"cited_paper":"/paper/2308.15351","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:d87c17a10f4f005c33efd5994b48a17b2c433d1346637b41215491bb54565e19","observation_id":"86d65e3f-6b18-40a2-961c-5fcfcaf93df8","resolution":{"observed_at":"2026-08-08T00:43:22.427229Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.06895","last_updated":"2018-01-11T01:53:22Z","snapshot_observed_at":"2026-08-06T03:48:37.494447Z","submitted_at":"2017-08-23T06:27:20Z","title":"The equation of state for dense nucleonic matter from a meta-modeling. II. Predictions for neutron stars properties","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.06895","snapshot_observed_at":"2026-08-08T00:43:19.344760Z","title":"Margueron, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.344760Z"},"links":{"cited_paper":"/paper/1708.06895","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:741eeb9d85c01e26c3c2871ad6483878708fcfe50a450e05bac95452df14030f","observation_id":"12a8ca26-7457-49d7-a92f-bf57d7b762af","resolution":{"observed_at":"2026-08-08T00:43:19.344760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.06894","last_updated":"2018-01-11T01:51:46Z","snapshot_observed_at":"2026-07-06T05:56:22.191336Z","submitted_at":"2017-08-23T06:18:33Z","title":"The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.06894","snapshot_observed_at":"2026-08-08T00:43:19.321418Z","title":"Margueron, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.321418Z"},"links":{"cited_paper":"/paper/1708.06894","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:f02884f1484a5515d96296897ea3c3a032ee9be1ddc9eb8fb509674f0182f307","observation_id":"6be31108-d670-4948-9cd1-c3da75e70482","resolution":{"observed_at":"2026-08-08T00:43:19.321418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.03790","last_updated":"2020-03-12T08:01:17Z","snapshot_observed_at":"2026-08-08T14:55:34.674512Z","submitted_at":"2019-07-08T18:05:46Z","title":"Sub-radian-accuracy gravitational waves from coalescing binary neutron stars II: Systematic study on the equation of state, binary mass, and mass ratio","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.03790","snapshot_observed_at":"2026-08-08T00:43:19.356367Z","title":"Kiuchi, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.356367Z"},"links":{"cited_paper":"/paper/1907.03790","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:6e4d01b801c591ebe6ea5dceb09f62cea2190dc27a4fe83b4cbfb803cba815ab","observation_id":"32fe65f6-c36e-4b41-9119-31dc491d46de","resolution":{"observed_at":"2026-08-08T00:43:19.356367Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-08T00:43:19.350676Z","title":"Radice, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.350676Z"},"links":{"cited_paper":"/paper/1809.11161","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:98d28e88f9d278524bd29d180eae4d3a8b92b58a447240e4d4038a4a3e71721b","observation_id":"1dd45bcf-6266-4137-aa9b-5c65e0f080f0","resolution":{"observed_at":"2026-08-08T00:43:19.350676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03361","last_updated":"2016-10-11T14:29:10Z","snapshot_observed_at":"2026-07-06T05:14:11.208979Z","submitted_at":"2016-10-11T14:29:10Z","title":"Equations of state for supernovae and compact stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.03361","snapshot_observed_at":"2026-08-08T00:43:19.377461Z","title":"Oertel, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.377461Z"},"links":{"cited_paper":"/paper/1610.03361","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:be8325d48423b8f63fcd28e30762d0e87cb4b0873b57e730d3a9bcd127834733","observation_id":"a60f36ba-cc03-401b-b029-43cdd572991d","resolution":{"observed_at":"2026-08-08T00:43:19.377461Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-08T00:43:19.362367Z","title":"Gonzalez, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.362367Z"},"links":{"cited_paper":"/paper/2210.16366","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:51fd8288c6bb4d1cf42f63a06f1cb09be78087a3c9a91ad6c9f3d9cdce6ad5d8","observation_id":"d5086450-07ec-4971-b8f7-65964c6bddb9","resolution":{"observed_at":"2026-08-08T00:43:19.362367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.01159","last_updated":"2016-11-03T20:00:02Z","snapshot_observed_at":"2026-07-06T05:17:18.667361Z","submitted_at":"2016-11-03T20:00:02Z","title":"Dynamical ejecta from precessing neutron star-black hole mergers with a hot, nuclear-theory based equation of state","version":1},"cited_work":{"arxiv_id":"1611.01159","doi":null,"metadata_source":"pith","pith_arxiv_id":"1611.01159","snapshot_observed_at":"2026-08-08T00:43:22.146416Z","title":"Dynamical ejecta from precessing neutron star-black hole mergers with a hot, nuclear-theory based equation of state","venue":"astro-ph.HE","work_id":"755ccd8d-f71c-43fa-a3db-e04eab5428d8","year":2016},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.397016Z"},"links":{"cited_paper":"/paper/1611.01159","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:6304f541834aafd1e5a8fed900a8bb61f5bf936ba62319127e97ae3a690d0cb2","observation_id":"5bdc28d6-4c93-4395-8e71-0fbdb4ff3c97","resolution":{"observed_at":"2026-08-08T00:43:22.156046Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5715","last_updated":"2013-07-22T14:02:32Z","snapshot_observed_at":"2026-08-01T22:18:46.384778Z","submitted_at":"2013-07-22T14:02:32Z","title":"CompOSE - CompStar Online Supernovae Equations of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.5715","snapshot_observed_at":"2026-08-08T00:43:19.383304Z","title":"Typel, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.383304Z"},"links":{"cited_paper":"/paper/1307.5715","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:4cd0da0ac9c2ce48df9d20d38d0c26b7c5fb4532ba970f6f414350bef33b0937","observation_id":"ed1a0110-7b79-4716-97b0-6dee5d573313","resolution":{"observed_at":"2026-08-08T00:43:19.383304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.3315","last_updated":"2010-10-15T17:54:46Z","snapshot_observed_at":"2026-07-06T02:11:51.145615Z","submitted_at":"2010-06-16T20:02:46Z","title":"Testing Approximations of Thermal Effects in Neutron Star Merger Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.3315","snapshot_observed_at":"2026-08-08T00:43:19.411068Z","title":"Bauswein, H.-T","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.411068Z"},"links":{"cited_paper":"/paper/1006.3315","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:31ec2995ae0b6fbf8f6a863a1a74fd465ae22b274de98d5b96f04fca2c3d8d98","observation_id":"5afff391-d4bd-4cc1-b510-73f13b7e9452","resolution":{"observed_at":"2026-08-08T00:43:19.411068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.02538","last_updated":"2023-03-15T20:49:05Z","snapshot_observed_at":"2026-08-08T07:35:15.285297Z","submitted_at":"2022-09-06T14:39:21Z","title":"Neutrino transport in general relativistic neutron star merger simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.02538","snapshot_observed_at":"2026-08-08T00:43:19.405049Z","title":"Foucart, Liv","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.405049Z"},"links":{"cited_paper":"/paper/2209.02538","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:c4b5e41794be6f982ccd8e628d2574700656349e6391209019e6757a2b9b92b0","observation_id":"d9cb32da-2a4b-46fe-a02a-7480ce59fa8c","resolution":{"observed_at":"2026-08-08T00:43:19.405049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.11359","last_updated":"2023-07-10T17:01:19Z","snapshot_observed_at":"2026-07-06T14:54:37.559648Z","submitted_at":"2023-02-22T13:14:26Z","title":"Thermal Effects in Binary Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.11359","snapshot_observed_at":"2026-08-08T00:43:19.423124Z","title":"Fields, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.423124Z"},"links":{"cited_paper":"/paper/2302.11359","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:542858908fd80e3c4f68fffafb08edb72cb8f2cafd4795f13334265f6f08531b","observation_id":"ecde60bf-50a5-4192-a353-a16105dd0092","resolution":{"observed_at":"2026-08-08T00:43:19.423124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.08691","last_updated":"2020-07-29T09:05:32Z","snapshot_observed_at":"2026-07-06T09:21:16.226310Z","submitted_at":"2020-05-18T13:16:09Z","title":"Hybrid equation of state approach in binary neutron-star merger simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.08691","snapshot_observed_at":"2026-08-08T00:43:19.417651Z","title":"Figura, J.-J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.417651Z"},"links":{"cited_paper":"/paper/2005.08691","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:5e1d80e56eca30b2c0d549f5d4648671bda07dbc6251044952d98d1bb29bd52f","observation_id":"5abd975b-84d2-4826-98dc-261f5d003b22","resolution":{"observed_at":"2026-08-08T00:43:19.417651Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06804","last_updated":"2021-07-14T16:04:29Z","snapshot_observed_at":"2026-08-06T08:06:41.139452Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06804","snapshot_observed_at":"2026-08-08T00:43:19.441566Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.441566Z"},"links":{"cited_paper":"/paper/2107.06804","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:42be2bda76a0be9cd84a55273ad0b23e466f32b6da88da32b96e640e52167ac6","observation_id":"e2ef3e4d-8d56-4185-90bb-cf8aed0dadac","resolution":{"observed_at":"2026-08-08T00:43:19.441566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10735","last_updated":"2019-02-27T19:10:13Z","snapshot_observed_at":"2026-08-08T16:40:11.313361Z","submitted_at":"2019-02-27T19:10:13Z","title":"Finite-temperature extension for cold neutron star equations of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10735","snapshot_observed_at":"2026-08-08T00:43:19.430350Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.430350Z"},"links":{"cited_paper":"/paper/1902.10735","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:742252b5b215653235016f1e129bae2b9a965a8b220a4afbfcd7a38e3fcbb4cd","observation_id":"bd94ab34-1624-4ff3-a9d1-cbc5c63f6afa","resolution":{"observed_at":"2026-08-08T00:43:19.430350Z","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":"2210.17509","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T00:43:21.896988Z","title":"Shankar, P","venue":null,"work_id":"af38cc09-4fdf-4abf-b2e2-d3c3494ee0fa","year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.452493Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:65bd47bbfc110899114d9d738d6bdaf3fb9e8105d738a44052dda1dfd8ca8bab","observation_id":"5d55fb5f-3904-477c-974e-74fa371f5ee8","resolution":{"observed_at":"2026-08-08T00:43:21.910776Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.10384","last_updated":"2024-11-22T20:02:55Z","snapshot_observed_at":"2026-08-08T01:12:02.534816Z","submitted_at":"2024-09-16T15:20:43Z","title":"Performance-Portable Binary Neutron Star Mergers with AthenaK","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.10384","snapshot_observed_at":"2026-08-08T00:43:19.446286Z","title":"Fields, H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.446286Z"},"links":{"cited_paper":"/paper/2409.10384","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:b2025a0044920482c100aa39b0263716aded9cbc8c1bde953302de91871b1bea","observation_id":"766e404a-7fb2-4737-a8d9-30c0b709ef4b","resolution":{"observed_at":"2026-08-08T00:43:19.446286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.09854","last_updated":"2026-07-10T18:00:01Z","snapshot_observed_at":"2026-08-07T21:16:16.355201Z","submitted_at":"2026-07-10T18:00:01Z","title":"GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity","version":1},"cited_work":{"arxiv_id":"2607.09854","doi":null,"metadata_source":"pith","pith_arxiv_id":"2607.09854","snapshot_observed_at":"2026-08-08T00:43:21.764690Z","title":"GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity","venue":"gr-qc","work_id":"a51871b5-898e-4ab2-9a8c-72805c4b5fa1","year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.471814Z"},"links":{"cited_paper":"/paper/2607.09854","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:d077b22d99aba401f5363b36cde939f87219fc75f77b66ec39be09c47041482c","observation_id":"031b00ef-a5ac-4b50-9b62-dea0f986c410","resolution":{"observed_at":"2026-08-08T00:43:21.771519Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.11669","last_updated":"2025-02-10T20:28:32Z","snapshot_observed_at":"2026-07-06T18:32:19.794373Z","submitted_at":"2024-06-17T15:51:35Z","title":"AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.11669","snapshot_observed_at":"2026-08-08T00:43:19.464877Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.464877Z"},"links":{"cited_paper":"/paper/2406.11669","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:ecd610408a7c9c4c4bd3ca198637d6adb2f791104f1911f1aed6444249417ef8","observation_id":"82dc268e-7cb1-4587-bcde-51fd5979bac7","resolution":{"observed_at":"2026-08-08T00:43:19.464877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.21725","last_updated":"2025-07-17T09:56:45Z","snapshot_observed_at":"2026-08-07T15:57:52.812787Z","submitted_at":"2025-04-30T15:11:02Z","title":"New {\\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain","version":2},"cited_work":{"arxiv_id":"2504.21725","doi":null,"metadata_source":"pith","pith_arxiv_id":"2504.21725","snapshot_observed_at":"2026-08-08T00:43:21.608920Z","title":"New {\\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain","venue":"nucl-th","work_id":"5816e277-c200-4c57-a7ad-b705ccdf434f","year":2025},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.482382Z"},"links":{"cited_paper":"/paper/2504.21725","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:4753a6689f7ea5eb60c6555fe884915289406111e7d1a2a131930d896dd95df1","observation_id":"33bd28b2-2e01-4a6f-8604-2bd03ed2d0e9","resolution":{"observed_at":"2026-08-08T00:43:21.614220Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2601.00976","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T00:43:21.724434Z","title":"Endeve, V","venue":null,"work_id":"54ea0b8b-a286-4fa0-a1cb-ca84a1752c52","year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.477515Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:13114ed169a5c2fe6c5761e5ce53d7c9a123166f1616dba172387f9202725523","observation_id":"a1d60de7-155c-4a82-8b3e-3f367538cd25","resolution":{"observed_at":"2026-08-08T00:43:21.737127Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06697","last_updated":"2021-07-14T13:37:17Z","snapshot_observed_at":"2026-07-06T11:29:04.092194Z","submitted_at":"2021-07-14T13:37:17Z","title":"Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06697","snapshot_observed_at":"2026-08-08T00:43:19.497246Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.497246Z"},"links":{"cited_paper":"/paper/2107.06697","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:bf687ef2a9b5e6166fabf7456c2fc8b4ccda19df854c26fdf89763ddba1d74e0","observation_id":"8a04f343-6c4a-4bc2-bd94-18d2ae2b1212","resolution":{"observed_at":"2026-08-08T00:43:19.497246Z","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":"2509.23910","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T00:43:21.563986Z","title":null,"venue":null,"work_id":"57126015-593c-45b5-83fe-fed27e2046f0","year":2026},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.489383Z"},"links":{"citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:cc6cdb750b459641d7095d53a7eac8dec75008ed14746760b82a5e355fac6a13","observation_id":"53fde5d1-eb78-4419-8cc4-98d8066ffbad","resolution":{"observed_at":"2026-08-08T00:43:21.577341Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.01527","last_updated":"2017-07-28T01:35:15Z","snapshot_observed_at":"2026-08-01T07:17:41.410923Z","submitted_at":"2017-07-05T18:27:02Z","title":"A New Open-Source Nuclear Equation of State Framework based on the Liquid-Drop Model with Skyrme Interaction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.01527","snapshot_observed_at":"2026-08-08T00:43:19.508454Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.508454Z"},"links":{"cited_paper":"/paper/1707.01527","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:f4ca7b6b69d24b171e99d496e28c8c3bf6cc730da39381c4396b2606f554339a","observation_id":"6d2d9c06-53f7-4e0a-acba-3724f6bbdeb1","resolution":{"observed_at":"2026-08-08T00:43:19.508454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.09499","last_updated":"2024-04-05T15:59:10Z","snapshot_observed_at":"2026-07-06T15:28:09.241288Z","submitted_at":"2023-05-16T14:52:54Z","title":"Energy and Angle Dependence of Neutrino Scattering Rates in Proto-Neutron Star and Supernova Matter within Skyrme RPA","version":3},"cited_work":{"arxiv_id":"2305.09499","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.09499","snapshot_observed_at":"2026-08-08T00:43:21.399710Z","title":"Energy and Angle Dependence of Neutrino Scattering Rates in Proto-Neutron Star and Supernova Matter within Skyrme RPA","venue":"nucl-th","work_id":"699d21fb-bc8d-4369-a253-bfbc5516f8d1","year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.502748Z"},"links":{"cited_paper":"/paper/2305.09499","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:2f83d3bb8a4666e67ee9b48a2bc4f0cf2211df72a8bc7deaa7f5d48f44216b84","observation_id":"703dc136-bdda-4215-a416-37aa0d48bb9b","resolution":{"observed_at":"2026-08-08T00:43:21.415721Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.02009","last_updated":"2019-06-05T13:02:15Z","snapshot_observed_at":"2026-08-08T14:39:19.032576Z","submitted_at":"2019-06-05T13:02:15Z","title":"Equation of state effects in the core collapse of a $20$-$M_\\odot$ star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.02009","snapshot_observed_at":"2026-08-08T00:43:19.523537Z","title":"Schneider, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.523537Z"},"links":{"cited_paper":"/paper/1906.02009","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:54873c383e65422277d406acc0483ccb5b2e50afceadb22c8ea1c3879083aa2c","observation_id":"85cb1bc0-da37-4ce1-8091-d6a1a75a6e27","resolution":{"observed_at":"2026-08-08T00:43:19.523537Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.02002","last_updated":"2020-03-12T08:02:28Z","snapshot_observed_at":"2026-08-08T14:37:02.833678Z","submitted_at":"2018-12-05T17:14:02Z","title":"Equation of state effects in core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.02002","snapshot_observed_at":"2026-08-08T00:43:19.513399Z","title":"Yasin, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.513399Z"},"links":{"cited_paper":"/paper/1812.02002","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:134ec1b3455a92addcaa161fb63bed9e0ec020e564efec1d5995ab7b4c318e81","observation_id":"fc3743a3-d0ab-4b85-998c-01be5079d76b","resolution":{"observed_at":"2026-08-08T00:43:19.513399Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00924","last_updated":"2019-08-22T13:30:48Z","snapshot_observed_at":"2026-07-06T07:43:06.427641Z","submitted_at":"2019-04-01T15:52:45Z","title":"${\\it Ab~initio}$ constraints on thermal effects of the nuclear equation of state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00924","snapshot_observed_at":"2026-08-08T00:43:19.539709Z","title":"Carbone and A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.539709Z"},"links":{"cited_paper":"/paper/1904.00924","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:be682b0c70d12542497118d6609ae0ee1c128b1914d3e088f7f75671d4d042f2","observation_id":"52940d6f-ea93-4803-99b6-6b3bdfe0cd8d","resolution":{"observed_at":"2026-08-08T00:43:19.539709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.05855","last_updated":"2021-05-17T14:54:59Z","snapshot_observed_at":"2026-07-06T10:13:41.694164Z","submitted_at":"2020-11-11T15:43:07Z","title":"Neutron matter at finite temperature based on chiral effective field theory interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.05855","snapshot_observed_at":"2026-08-08T00:43:19.529705Z","title":"Keller, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.529705Z"},"links":{"cited_paper":"/paper/2011.05855","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:204fb743b740689fbbbdaa7c74f263508836975aba88d0f84595d4b1e3c3b4a8","observation_id":"34768495-f525-4157-8a70-ce27601c4da6","resolution":{"observed_at":"2026-08-08T00:43:19.529705Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.08885","last_updated":"2021-02-12T15:35:51Z","snapshot_observed_at":"2026-07-06T09:56:50.303479Z","submitted_at":"2020-09-18T15:20:05Z","title":"New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.08885","snapshot_observed_at":"2026-08-08T00:43:19.555195Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.555195Z"},"links":{"cited_paper":"/paper/2009.08885","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:abd5abe60b03ee3a445933f616fc8311093e491733e08cd8c43a901adf91727a","observation_id":"9c52c370-2eab-467a-b487-429a4e1182c7","resolution":{"observed_at":"2026-08-08T00:43:19.555195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01213","last_updated":"2018-01-04T00:31:20Z","snapshot_observed_at":"2026-08-01T22:08:04.790508Z","submitted_at":"2018-01-04T00:31:20Z","title":"Nucleon Effective Masses in Neutron-Rich Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01213","snapshot_observed_at":"2026-08-08T00:43:19.544752Z","title":"Li, B.-J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.544752Z"},"links":{"cited_paper":"/paper/1801.01213","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:ca5f338968fe7b3bbbbce1586669ad9baa7807677de3b99f715a6031898ceffc","observation_id":"fc753846-ffd2-42f6-adbe-445f7d52f66e","resolution":{"observed_at":"2026-08-08T00:43:19.544752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.03672","last_updated":"2018-01-30T10:00:48Z","snapshot_observed_at":"2026-08-07T00:59:34.633125Z","submitted_at":"2018-01-11T08:57:02Z","title":"The Compression-Mode Giant Resonances and Nuclear Incompressibility","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.03672","snapshot_observed_at":"2026-08-08T00:43:19.570785Z","title":"Garg and G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.570785Z"},"links":{"cited_paper":"/paper/1801.03672","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:e58cee74ac281f52dd8f835d4689b022653a9f3553f300573b8f63f59be8a0ee","observation_id":"64b17c44-5726-4053-a9c2-3415fe49618c","resolution":{"observed_at":"2026-08-08T00:43:19.570785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.13175","last_updated":"2019-05-29T17:27:56Z","snapshot_observed_at":"2026-07-06T07:56:47.616437Z","submitted_at":"2019-05-29T17:27:56Z","title":"Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.13175","snapshot_observed_at":"2026-08-08T00:43:19.565614Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.565614Z"},"links":{"cited_paper":"/paper/1905.13175","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:37d2e4ff5e7ae8502b56ee9d14feb31375a4beee5e9af7f7e0fc3bec42deccfd","observation_id":"ab3e2f6b-c12e-405c-a193-1cc8acfb3518","resolution":{"observed_at":"2026-08-08T00:43:19.565614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.05246","last_updated":"2015-01-21T18:09:19Z","snapshot_observed_at":"2026-08-06T16:50:46.440965Z","submitted_at":"2015-01-21T18:09:19Z","title":"Constraining the nuclear matter equation of state around twice saturation density","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.05246","snapshot_observed_at":"2026-08-08T00:43:19.580233Z","title":"Le F` evre, Y","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.580233Z"},"links":{"cited_paper":"/paper/1501.05246","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:2ad15d01bff0de18378e5ad28cf16313725cc438364bc2262a5dd99dda14257f","observation_id":"93f3dc66-780e-42b5-8641-839701b75c9f","resolution":{"observed_at":"2026-08-08T00:43:19.580233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01264","last_updated":"2022-11-02T16:46:29Z","snapshot_observed_at":"2026-07-06T14:13:39.478174Z","submitted_at":"2022-11-02T16:46:29Z","title":"Towards a Unified Description of Isoscalar Giant Monopole Resonances in a Self-Consistent Quasiparticle-Vibration Coupling Approach","version":1},"cited_work":{"arxiv_id":"2211.01264","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.01264","snapshot_observed_at":"2026-08-08T00:43:21.145310Z","title":"Towards a Unified Description of Isoscalar Giant Monopole Resonances in a Self-Consistent Quasiparticle-Vibration Coupling Approach","venue":"nucl-th","work_id":"d690bb4d-53df-4379-8137-4d2e5722c0ef","year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.575475Z"},"links":{"cited_paper":"/paper/2211.01264","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:2791bbfd18f6d9cfaabac3b4d8a221ae63433c3541300c96786431e10b7030dc","observation_id":"770d70fa-ad9a-4fc1-8b3b-0186929eda8a","resolution":{"observed_at":"2026-08-08T00:43:21.152865Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.0744","last_updated":"2014-04-29T02:17:40Z","snapshot_observed_at":"2026-08-04T18:02:36.197360Z","submitted_at":"2014-04-03T01:07:53Z","title":"Incompressibility in finite nuclei and nuclear matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.0744","snapshot_observed_at":"2026-08-08T00:43:19.599813Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.599813Z"},"links":{"cited_paper":"/paper/1404.0744","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:470fdc4a3e680e0a1e5502b895dac8bcfe43fd74a75f46ce54d324d9e43e9b39","observation_id":"ef8c0a7e-514e-498d-a492-7da6189b57e1","resolution":{"observed_at":"2026-08-08T00:43:19.599813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.07805","last_updated":"2021-01-07T17:59:40Z","snapshot_observed_at":"2026-08-03T21:37:31.579349Z","submitted_at":"2020-04-16T17:52:14Z","title":"Quantifying uncertainties and correlations in the nuclear-matter equation of state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.07805","snapshot_observed_at":"2026-08-08T00:43:19.594760Z","title":"Drischler, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.594760Z"},"links":{"cited_paper":"/paper/2004.07805","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:0cde85953507c8c32384e32bbd016682add33bc847b3dc7dab886e983da5c3b2","observation_id":"38d3d8d2-e56d-4fe0-9922-4a1e0756711e","resolution":{"observed_at":"2026-08-08T00:43:19.594760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.03193","last_updated":"2021-03-31T18:26:09Z","snapshot_observed_at":"2026-07-06T10:31:05.724797Z","submitted_at":"2021-01-08T19:28:16Z","title":"Implications of PREX-II on the equation of state of neutron-rich matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.03193","snapshot_observed_at":"2026-08-08T00:43:19.625820Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.625820Z"},"links":{"cited_paper":"/paper/2101.03193","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:1763d42044fad205108e2a2f01d564b48b39cb132d7e40b4a64af9cf899c00b3","observation_id":"ab82635b-1469-46b2-a321-79a2398cd4e0","resolution":{"observed_at":"2026-08-08T00:43:19.625820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.01709","last_updated":"2021-05-26T13:42:52Z","snapshot_observed_at":"2026-08-07T09:31:39.613742Z","submitted_at":"2021-01-05T18:54:07Z","title":"Chiral Effective Field Theory and the High-Density Nuclear Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.01709","snapshot_observed_at":"2026-08-08T00:43:19.619509Z","title":"Drischler, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.619509Z"},"links":{"cited_paper":"/paper/2101.01709","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:54c5eaa4d7b8d5a5e2eed235d25454fdd261cb356d515be5b29fe7475928ed64","observation_id":"cecc0964-d8fc-41a9-a0fe-1aa1f60ccec4","resolution":{"observed_at":"2026-08-08T00:43:19.619509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03328","last_updated":"2023-08-14T10:18:24Z","snapshot_observed_at":"2026-07-06T13:28:50.323303Z","submitted_at":"2022-07-07T14:37:11Z","title":"Bayesian Inference of the Symmetry Energy and the Neutron Skin in $^{48}$Ca and $^{208}$Pb from CREX and PREX-2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03328","snapshot_observed_at":"2026-08-08T00:43:19.644749Z","title":"Zhang and L.-W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.644749Z"},"links":{"cited_paper":"/paper/2207.03328","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:3a453da0ecdcebf9c5fad3e5b2d6fa377496aabd64b9c66141da8178f228217d","observation_id":"8710c2d3-aeda-4454-96fc-509a2cdb4c69","resolution":{"observed_at":"2026-08-08T00:43:19.644749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.11593","last_updated":"2022-06-16T21:20:56Z","snapshot_observed_at":"2026-07-06T13:13:03.434894Z","submitted_at":"2022-05-23T19:46:18Z","title":"Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.11593","snapshot_observed_at":"2026-08-08T00:43:19.633685Z","title":"Adhikari et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.633685Z"},"links":{"cited_paper":"/paper/2205.11593","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:93070eef83e206bd9822b08a52c525243471195ae9f14b95e39dda69096398cb","observation_id":"711fe4c7-f74b-4848-a0fe-69baa24dfc1c","resolution":{"observed_at":"2026-08-08T00:43:19.633685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.4286","last_updated":"2013-05-15T13:52:30Z","snapshot_observed_at":"2026-07-06T02:44:50.967304Z","submitted_at":"2012-03-19T23:04:21Z","title":"Constraining the Symmetry Parameters of the Nuclear Interaction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.4286","snapshot_observed_at":"2026-08-08T00:43:19.654948Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.654948Z"},"links":{"cited_paper":"/paper/1203.4286","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:cb55b30eb422160c4bbcb98282d0fac9fbf3906d8c1f157c68ce3bf19cbe2090","observation_id":"eeaace47-4d24-4cd8-ab02-08ee6759742b","resolution":{"observed_at":"2026-08-08T00:43:19.654948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07133","last_updated":"2017-10-25T21:05:32Z","snapshot_observed_at":"2026-07-06T05:19:35.141404Z","submitted_at":"2016-11-22T03:03:09Z","title":"Symmetry Parameter Constraints From A Lower Bound On The Neutron-Matter Energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07133","snapshot_observed_at":"2026-08-08T00:43:19.650056Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.650056Z"},"links":{"cited_paper":"/paper/1611.07133","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:7efac90bac6dcde73fd486ab85f542928a5b6e116c02439fd6d03d8d2c62cd22","observation_id":"da2d6c13-65b0-4da1-afd1-dcc374470af4","resolution":{"observed_at":"2026-08-08T00:43:19.650056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.15050","last_updated":"2021-07-14T10:38:03Z","snapshot_observed_at":"2026-07-06T11:14:24.508408Z","submitted_at":"2021-05-31T15:33:32Z","title":"Information content of the parity-violating asymmetry in $^{208}$Pb","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.15050","snapshot_observed_at":"2026-08-08T00:43:19.666430Z","title":"Reinhard, X","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.666430Z"},"links":{"cited_paper":"/paper/2105.15050","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:44d34ff71cd30f4d7035ab2ec6c79da50222f842e9388d0ef78a6fc958739a06","observation_id":"6429e05c-b231-49bd-bc1e-6f2c61e9787f","resolution":{"observed_at":"2026-08-08T00:43:19.666430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03134","last_updated":"2023-01-02T17:51:19Z","snapshot_observed_at":"2026-07-06T13:18:09.946150Z","submitted_at":"2022-06-07T09:16:36Z","title":"Combined theoretical analysis of the parity-violating asymmetry for ${}^{48}$Ca and ${}^{208}Pb$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.03134","snapshot_observed_at":"2026-08-08T00:43:19.659638Z","title":"Reinhard, X","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.659638Z"},"links":{"cited_paper":"/paper/2206.03134","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:f1b40c37c773e8022c225f8022c5c2b782e2814b2a463be6b3f17ba3ecb334a1","observation_id":"c5c5e91e-3a7c-4498-bc69-60df30c26ecf","resolution":{"observed_at":"2026-08-08T00:43:19.659638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03666","last_updated":"2023-01-09T20:29:41Z","snapshot_observed_at":"2026-07-06T14:39:46.284351Z","submitted_at":"2023-01-09T20:29:41Z","title":"Constraints on Nuclear Symmetry Energy Parameters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03666","snapshot_observed_at":"2026-08-08T00:43:19.676262Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.676262Z"},"links":{"cited_paper":"/paper/2301.03666","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:d8e6973e2b6d94915856f566119cb1fcad9e980c25a8f4e1dc3baf3a97a070b4","observation_id":"9c1ed993-9e8e-4f12-80f6-46531819ef5e","resolution":{"observed_at":"2026-08-08T00:43:19.676262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.10074","last_updated":"2021-11-04T01:28:50Z","snapshot_observed_at":"2026-08-08T18:41:28.733001Z","submitted_at":"2021-02-19T18:14:59Z","title":"Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.10074","snapshot_observed_at":"2026-08-08T00:43:19.671183Z","title":"Essick, I","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.671183Z"},"links":{"cited_paper":"/paper/2102.10074","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:c01e3cf82fcfb5b4e6ce322f7010d7685e0cb9182c6132868077e8d729c86821","observation_id":"19e3a646-646c-449d-85e8-d3608dd17ec1","resolution":{"observed_at":"2026-08-08T00:43:19.671183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-08T19:11:12.965045Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":16,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":73,"verified_exact":11,"verified_fuzzy":0},"total_outbound_references":136},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 100 of 136 outbound references and 0 inbound Pith citation observations for arXiv:2608.04092."}