{"as_of":"2026-08-22T16:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1fb07948a49669d59d9ae3c18d09fcf7b9e0ebe2f4bc91e88c0788c18fcdead9","coverage":[{"denominator":104,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T05:43:33.431803Z","state":"measured"},{"denominator":103,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":103,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-10T22:27:16.157204Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T22:27:36.581783Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"cited_work":{"arxiv_id":"2603.27680","doi":null,"metadata_source":"pith","pith_arxiv_id":"2603.27680","snapshot_observed_at":"2026-07-10T22:27:36.581783Z","title":"Akhmetali, Y","venue":"astro-ph.HE","work_id":"bc42f10e-533a-4d25-a438-024cca8b54e9","year":2026},"citing_paper":{"arxiv_id":"2605.04896","last_updated":"2026-08-17T10:43:20Z","snapshot_observed_at":"2026-08-20T23:15:53.104386Z","submitted_at":"2026-05-06T13:27:04Z","title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-08T15:59:11.556246Z"},"links":{"cited_paper":"/paper/2603.27680","citing_paper":"/paper/2605.04896"},"observation_digest":"sha256:90fd44a46a888bd9f8fa7efb9c91a31bc966d60bfa59541dd1e61956c852c612","observation_id":"a9cfe0e0-9bfc-44ac-9d96-f3db7e10c30e","resolution":{"observed_at":"2026-06-24T02:14:49.089585Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"cited_work":{"arxiv_id":"2603.27680","doi":null,"metadata_source":"pith","pith_arxiv_id":"2603.27680","snapshot_observed_at":"2026-07-10T22:27:36.581783Z","title":"Akhmetali, Y","venue":"astro-ph.HE","work_id":"bc42f10e-533a-4d25-a438-024cca8b54e9","year":2026},"citing_paper":{"arxiv_id":"2605.21310","last_updated":"2026-05-20T15:37:58Z","snapshot_observed_at":"2026-08-17T02:55:31.042897Z","submitted_at":"2026-05-20T15:37:58Z","title":"Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection","version":1},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-05-21T03:33:53.198336Z"},"links":{"cited_paper":"/paper/2603.27680","citing_paper":"/paper/2605.21310"},"observation_digest":"sha256:0f0a54d230ec34d961481bd42512882a722dabfa69f459c3b949ecb20b2f524e","observation_id":"2df88077-abb2-453a-8d6e-280f46350080","resolution":{"observed_at":"2026-06-24T02:14:49.089585Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"cited_work":{"arxiv_id":"2603.27680","doi":null,"metadata_source":"pith","pith_arxiv_id":"2603.27680","snapshot_observed_at":"2026-07-10T22:27:36.581783Z","title":"Akhmetali, Y","venue":"astro-ph.HE","work_id":"bc42f10e-533a-4d25-a438-024cca8b54e9","year":2026},"citing_paper":{"arxiv_id":"2607.06736","last_updated":"2026-07-09T15:38:32Z","snapshot_observed_at":"2026-08-18T22:27:29.999946Z","submitted_at":"2026-07-07T19:00:28Z","title":"The Generalization Gap in Machine Learning EoS Inference from Core-Collapse Supernova Gravitational Waves","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-10T22:27:16.157204Z"},"links":{"cited_paper":"/paper/2603.27680","citing_paper":"/paper/2607.06736"},"observation_digest":"sha256:3cd24a9e8c981b5d435461db749b428ea902caf684b2ac3c5d4d520607191f4c","observation_id":"bec93817-358a-4da7-95a2-c191d25e95ca","resolution":{"observed_at":"2026-07-10T22:27:36.597352Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2603.27680/citation-record","integrity":"/paper/2603.27680/integrity","json":"/paper/2603.27680/citation-record.json","paper":"/paper/2603.27680"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2508.18082","last_updated":"2026-06-26T11:38:00Z","snapshot_observed_at":"2026-08-17T00:03:22.576608Z","submitted_at":"2025-08-25T14:46:09Z","title":"GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18082","snapshot_observed_at":"2026-08-04T05:43:22.994740Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:22.994740Z"},"links":{"cited_paper":"/paper/2508.18082","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:cef8863d85967cc9de7a43c5c777175195e2b61d79a3edb2ed5f67d47ebf398a","observation_id":"97b91106-4ad7-43c0-911a-06f21f6b0217","resolution":{"observed_at":"2026-08-04T05:43:22.994740Z","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":"2026-08-04T05:43:23.075197Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.075197Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:dd0e326f35c1bf6a5c4b4d44ca6f8353761e77c0d3b8fc9b51845b5f5692596c","observation_id":"cfcb9e69-4cce-4b4a-981a-ebeb64bfabc2","resolution":{"observed_at":"2026-08-04T05:43:23.075197Z","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":"2026-08-04T05:43:23.206160Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.206160Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:2b578aedf1440e7ce2f14ea07b5c9945910414c049f2fb404faa73e25b90e442","observation_id":"91fcefc4-28e9-4a08-bd76-b043e5c36519","resolution":{"observed_at":"2026-08-04T05:43:23.206160Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.01397","last_updated":"2022-03-03T00:00:04Z","snapshot_observed_at":"2026-08-21T08:33:21.355815Z","submitted_at":"2022-01-05T00:50:00Z","title":"Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.01397","snapshot_observed_at":"2026-08-04T05:43:23.290918Z","title":"Powell and B","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.290918Z"},"links":{"cited_paper":"/paper/2201.01397","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:ec1610466ee2271211646191d6315066d4a3ac4bcfeababf7274293d433595b5","observation_id":"04c66f55-711c-4592-9e0a-e15f48b3590a","resolution":{"observed_at":"2026-08-04T05:43:23.290918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.02836","last_updated":"2016-07-07T20:06:20Z","snapshot_observed_at":"2026-08-15T01:08:53.534371Z","submitted_at":"2015-11-09T20:44:37Z","title":"Observing Gravitational Waves from Core-Collapse Supernovae in the Advanced Detector Era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.02836","snapshot_observed_at":"2026-08-04T05:43:23.384738Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.384738Z"},"links":{"cited_paper":"/paper/1511.02836","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:a1b756c8ece5300b2d6404a11631011c6224dcbcc1e1b23f75c68ce88eb2f28e","observation_id":"b0a43e79-3b4a-4699-ae09-116078b71025","resolution":{"observed_at":"2026-08-04T05:43:23.384738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06462","last_updated":"2021-04-13T19:09:48Z","snapshot_observed_at":"2026-08-17T12:48:50.059345Z","submitted_at":"2021-04-13T19:09:48Z","title":"Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06462","snapshot_observed_at":"2026-08-04T05:43:23.461293Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.461293Z"},"links":{"cited_paper":"/paper/2104.06462","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:45eb4bfc60106526a68220f0d8d93a1cc1fbe267792fc26ca480c7eddf14b34a","observation_id":"0ff44c3e-e2ee-48fd-b6c9-523c74d97d35","resolution":{"observed_at":"2026-08-04T05:43:23.461293Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.00084","last_updated":"2019-05-31T21:16:15Z","snapshot_observed_at":"2026-08-19T23:58:54.322444Z","submitted_at":"2019-05-31T21:16:15Z","title":"Detection Prospects of Core-Collapse Supernovae with Supernova-Optimized Third-Generation Gravitational-wave Detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.00084","snapshot_observed_at":"2026-08-04T05:43:23.540463Z","title":"Srivastava, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.540463Z"},"links":{"cited_paper":"/paper/1906.00084","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:f017c6cf58c8ad56a0b0592090d58501231233b919f8ee5d3b60efaa3a1eeea7","observation_id":"f2962a95-c284-4f66-a74c-c574c7dcfe80","resolution":{"observed_at":"2026-08-04T05:43:23.540463Z","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":"2026-08-04T05:43:23.605141Z","title":"Abdikamalov, G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.605141Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:3cdc73a2adfd0795c549d756de70c3bea0e70bd815fce1b97581cd25b521c0c6","observation_id":"e46a1bf3-5478-4036-9826-41972de130da","resolution":{"observed_at":"2026-08-04T05:43:23.605141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.11635","last_updated":"2024-01-22T00:18:28Z","snapshot_observed_at":"2026-08-21T10:48:53.771925Z","submitted_at":"2024-01-22T00:18:28Z","title":"Gravitational Waves from Neutrino-Driven Core Collapse Supernovae: Predictions, Detection, and Parameter Estimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.11635","snapshot_observed_at":"2026-08-04T05:43:23.681626Z","title":"Mezzacappa and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.681626Z"},"links":{"cited_paper":"/paper/2401.11635","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:e69f31529bf90689eee51015d948ffd89aff530caf6a16a5bd20dbf0a04eb7eb","observation_id":"c0531fe2-4d75-4ad7-92bc-78f2909d3eee","resolution":{"observed_at":"2026-08-04T05:43:23.681626Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.24243","last_updated":"2026-07-15T03:34:44Z","snapshot_observed_at":"2026-08-16T16:19:15.742081Z","submitted_at":"2026-03-25T12:29:39Z","title":"Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.24243","snapshot_observed_at":"2026-08-04T05:43:23.823697Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.823697Z"},"links":{"cited_paper":"/paper/2603.24243","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:eb105d72ee5aa15fb3acf6c099bdf1e5a370c847ca0a82a6b8a4a7a4f4c3e675","observation_id":"255b4799-adae-4c6a-b8c5-a583a71a3422","resolution":{"observed_at":"2026-08-04T05:43:23.823697Z","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":"2026-08-04T05:43:23.934032Z","title":"Burrows and J","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.934032Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:794d4aaa89437d14e978275ee7008f268df41bf612feffa7d40fb40406115b74","observation_id":"3187b4a8-108a-415f-bad3-5a4b7973aeac","resolution":{"observed_at":"2026-08-04T05:43:23.934032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0008432","last_updated":"2001-01-03T20:50:39Z","snapshot_observed_at":"2026-08-19T11:55:08.956794Z","submitted_at":"2000-08-28T19:20:21Z","title":"Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0008432","snapshot_observed_at":"2026-08-04T05:43:23.994894Z","title":"Janka, Conditions for shock revival by neutrino heating in core-collapse supernovae, A&A368, 527 (2001), arXiv:astro-ph/0008432 [astro-ph]","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:23.994894Z"},"links":{"cited_paper":"/paper/astro-ph/0008432","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:d35f90e8214f9fa96a538cd4cb57bc29be617e3e6daf7b95b3970c10d6af1307","observation_id":"1e4aa790-0713-4460-b7e0-7272a6750742","resolution":{"observed_at":"2026-08-04T05:43:23.994894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.05083","last_updated":"2020-06-09T07:23:00Z","snapshot_observed_at":"2026-08-10T05:45:07.617277Z","submitted_at":"2020-06-09T07:23:00Z","title":"Hydrodynamics of core-collapse supernovae and their progenitors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.05083","snapshot_observed_at":"2026-08-04T05:43:24.075224Z","title":"M¨ uller, Hydrodynamics of core-collapse supernovae and their progenitors, Living Reviews in Computa- 9 tional Astrophysics6, 3 (2020), arXiv:2006.05083 [astro- ph.SR]","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.075224Z"},"links":{"cited_paper":"/paper/2006.05083","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:99b91521f5beda3dcace0fdc5f4119dbf8f65b77220123011e5665151ccc7419","observation_id":"eb207bb0-fa47-4a9c-92e0-eb346c40dbb1","resolution":{"observed_at":"2026-08-04T05:43:24.075224Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005438","last_updated":"2000-06-30T16:38:15Z","snapshot_observed_at":"2026-07-07T00:11:27.453055Z","submitted_at":"2000-05-22T18:52:27Z","title":"Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005438","snapshot_observed_at":"2026-08-04T05:43:24.184827Z","title":"Rampp and H.-T","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.184827Z"},"links":{"cited_paper":"/paper/astro-ph/0005438","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:ca2fbaf1c58e75b152755af7b08118d68988b82099fe1fa53ee1bd9dead87642","observation_id":"b9d85577-772d-46c3-a879-35dc4c674481","resolution":{"observed_at":"2026-08-04T05:43:24.184827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.1100","last_updated":"2013-01-30T01:58:56Z","snapshot_observed_at":"2026-08-15T00:54:19.877159Z","submitted_at":"2012-07-04T20:00:00Z","title":"The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.1100","snapshot_observed_at":"2026-08-04T05:43:24.220740Z","title":"O’Connor and C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.220740Z"},"links":{"cited_paper":"/paper/1207.1100","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:6f73433667ef3484df9daab38e66ca2ae1d035355383031fdf51e1e167eec0ee","observation_id":"a07c9f5f-9885-47c2-bfa2-88a534d48c34","resolution":{"observed_at":"2026-08-04T05:43:24.220740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512189","last_updated":"2006-07-10T18:27:48Z","snapshot_observed_at":"2026-07-07T00:56:44.301086Z","submitted_at":"2005-12-07T17:30:52Z","title":"Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512189","snapshot_observed_at":"2026-08-04T05:43:24.299575Z","title":"Buras, H.-T","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.299575Z"},"links":{"cited_paper":"/paper/astro-ph/0512189","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:9aae2ffcfb6e20f4d0ffab8a1afe8915d4c8076404d5e7aa76944b149b0d3605","observation_id":"e4af6eb2-cbdf-491a-a03d-4ef19bcb0d5e","resolution":{"observed_at":"2026-08-04T05:43:24.299575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.5779","last_updated":"2015-11-03T19:46:43Z","snapshot_observed_at":"2026-08-14T23:18:47.989413Z","submitted_at":"2014-09-19T19:42:16Z","title":"The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_\\odot$ Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.5779","snapshot_observed_at":"2026-08-04T05:43:24.414233Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.414233Z"},"links":{"cited_paper":"/paper/1409.5779","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:b414608eff33eaf8b9aea2c2c3245af27a1821ea19f963651c6bef4381ff4911","observation_id":"76c7b2a4-ea39-489c-994b-467387081a8c","resolution":{"observed_at":"2026-08-04T05:43:24.414233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.02703","last_updated":"2018-02-07T07:58:01Z","snapshot_observed_at":"2026-08-14T19:56:54.349875Z","submitted_at":"2018-01-08T22:34:48Z","title":"Impact of Neutrino Opacities on Core-Collapse Supernova Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.02703","snapshot_observed_at":"2026-08-04T05:43:24.558823Z","title":"Kotake, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.558823Z"},"links":{"cited_paper":"/paper/1801.02703","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:34d05595669a377bd8938c102b60373b1bc2ec97ca4e696b813e3306f552efee","observation_id":"788970ff-a125-42e1-b008-2bbc64ffceea","resolution":{"observed_at":"2026-08-04T05:43:24.558823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210634","last_updated":"2002-10-29T18:33:40Z","snapshot_observed_at":"2026-08-18T18:40:25.482550Z","submitted_at":"2002-10-29T18:33:40Z","title":"Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0210634","snapshot_observed_at":"2026-08-04T05:43:24.627462Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.627462Z"},"links":{"cited_paper":"/paper/astro-ph/0210634","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:c0582bcd1485950be545f3a0099a93b97177cdb75df9b14700e3087e710780f8","observation_id":"3a957f71-04f0-448a-87e8-7765cbb67eaf","resolution":{"observed_at":"2026-08-04T05:43:24.627462Z","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":"2026-08-04T05:43:24.708638Z","title":"Foglizzo, L","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.708638Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:497eb76721ee2be75de1c9b826b98df538c3d2f266af328a416b96b8be1c4776","observation_id":"3e35f896-3a0b-4809-a9cb-1378443cf079","resolution":{"observed_at":"2026-08-04T05:43:24.708638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.7078","last_updated":"2012-10-25T10:47:14Z","snapshot_observed_at":"2026-08-15T00:58:20.485988Z","submitted_at":"2012-05-31T19:20:05Z","title":"New Two-Dimensional Models of Supernova Explosions by the Neutrino-Heating Mechanism: Evidence for Different Instability Regimes in Collapsing Stellar Cores","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.7078","snapshot_observed_at":"2026-08-04T05:43:24.777545Z","title":"M¨ uller, H.-T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.777545Z"},"links":{"cited_paper":"/paper/1205.7078","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:cd1205607ffc9db7c484690cbf72da5ec68c74e01c02f6313d5d87e3815d58c0","observation_id":"36b88309-5769-4a5b-bcad-4b6d24bdaae1","resolution":{"observed_at":"2026-08-04T05:43:24.777545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02199","last_updated":"2015-06-22T19:27:20Z","snapshot_observed_at":"2026-08-16T18:59:53.520704Z","submitted_at":"2015-03-07T18:31:13Z","title":"The Three Dimensional Evolution to Core Collapse of a Massive Star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.02199","snapshot_observed_at":"2026-08-04T05:43:24.916390Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.916390Z"},"links":{"cited_paper":"/paper/1503.02199","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:cf76930b4a5b3103138b7ed9a661730ff3fe195f714a82903ab728a534a5db86","observation_id":"59cc2657-bf18-4ede-87bf-3be520bb1e77","resolution":{"observed_at":"2026-08-04T05:43:24.916390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.00620","last_updated":"2017-07-28T14:30:16Z","snapshot_observed_at":"2026-08-17T14:16:05.145258Z","submitted_at":"2017-05-01T18:00:01Z","title":"Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.00620","snapshot_observed_at":"2026-08-04T05:43:24.980845Z","title":"M¨ uller, T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:24.980845Z"},"links":{"cited_paper":"/paper/1705.00620","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:f4c6bde8c6635ee88c05ecbfd93f5f2c1b91f02abe42f59c054d2d53b5f427c6","observation_id":"ecfabff5-443d-4e31-a7d6-d690d766f370","resolution":{"observed_at":"2026-08-04T05:43:24.980845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.08819","last_updated":"2020-06-23T15:01:35Z","snapshot_observed_at":"2026-08-19T07:45:42.809191Z","submitted_at":"2019-11-20T11:00:22Z","title":"The impact of progenitor asymmetries on the neutrino-driven convection in core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.08819","snapshot_observed_at":"2026-08-04T05:43:25.089001Z","title":"Kazeroni and E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.089001Z"},"links":{"cited_paper":"/paper/1911.08819","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:797f34915b025fc7eef63b86bb8aa180866ae63ce99e72067e0bffa8fb641db7","observation_id":"573d8073-9fc5-4b62-a2fb-3de0752a11a1","resolution":{"observed_at":"2026-08-04T05:43:25.089001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.17737","last_updated":"2024-09-26T11:11:14Z","snapshot_observed_at":"2026-08-16T13:15:10.676444Z","submitted_at":"2024-09-26T11:11:14Z","title":"Convective vortices in collapsing stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.17737","snapshot_observed_at":"2026-08-04T05:43:25.189057Z","title":"Telman, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.189057Z"},"links":{"cited_paper":"/paper/2409.17737","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:aa53a23239a7ceb43da14ed6a22ab29f338ffb773a5273d3849fb5a42c0af04b","observation_id":"9b5ef347-dfa9-4410-8a8e-7062ff921f82","resolution":{"observed_at":"2026-08-04T05:43:25.189057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409422","last_updated":"2004-09-17T03:35:22Z","snapshot_observed_at":"2026-08-20T18:46:17.099304Z","submitted_at":"2004-09-17T03:35:22Z","title":"Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409422","snapshot_observed_at":"2026-08-04T05:43:25.255139Z","title":"Heger, S","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.255139Z"},"links":{"cited_paper":"/paper/astro-ph/0409422","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:8995120753feb47dd7ab38b13f8c5cd572222c09239eded76220242590a7fd80","observation_id":"af6315d0-ea3d-43c8-a5ee-d952248e68b6","resolution":{"observed_at":"2026-08-04T05:43:25.255139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.0632","last_updated":"2012-04-03T09:24:09Z","snapshot_observed_at":"2026-08-15T04:14:10.148599Z","submitted_at":"2012-04-03T09:24:09Z","title":"Initial spin periods of neutron stars in supernova remnants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.0632","snapshot_observed_at":"2026-08-04T05:43:25.295483Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.295483Z"},"links":{"cited_paper":"/paper/1204.0632","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:e35aed037190159d7d386ad7ea1d93e4823b49cde1cc54b1a483e3d4ca735c5f","observation_id":"0f51f098-d63a-42a3-bb96-122e86b4128a","resolution":{"observed_at":"2026-08-04T05:43:25.295483Z","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":"2026-08-04T05:43:25.366773Z","title":"Burrows, L","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.366773Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:c11fb401a632d1ab8bbb993b484d1ddf8244970233c09512111217499d39d4ba","observation_id":"d4dc9dd7-cb9d-444e-a081-480a05ff3782","resolution":{"observed_at":"2026-08-04T05:43:25.366773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.1230","last_updated":"2014-03-05T19:13:50Z","snapshot_observed_at":"2026-08-14T23:42:20.587112Z","submitted_at":"2014-03-05T19:13:50Z","title":"Magnetorotational Core-Collapse Supernovae in Three Dimensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.1230","snapshot_observed_at":"2026-08-04T05:43:25.425840Z","title":"M¨ osta, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.425840Z"},"links":{"cited_paper":"/paper/1403.1230","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:4f97b2c779624b8b523a240c1efe1661193c1c34aa928b49b4172eb6ea3e45f1","observation_id":"f7f8f244-9e58-4f52-80a9-0150e361cdf8","resolution":{"observed_at":"2026-08-04T05:43:25.425840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.02004","last_updated":"2020-05-12T13:59:19Z","snapshot_observed_at":"2026-08-17T10:18:40.783632Z","submitted_at":"2020-03-04T11:11:05Z","title":"Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.02004","snapshot_observed_at":"2026-08-04T05:43:25.477383Z","title":"Kuroda, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.477383Z"},"links":{"cited_paper":"/paper/2003.02004","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:25c6d11f6025212fa4e87f9b7563abb4dfd2528933b04811c3269d0fe1ccd16c","observation_id":"2935e291-39da-4fb5-9c8f-0472f329248c","resolution":{"observed_at":"2026-08-04T05:43:25.477383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.01105","last_updated":"2020-01-11T11:21:44Z","snapshot_observed_at":"2026-08-15T17:39:09.389277Z","submitted_at":"2019-09-03T12:02:35Z","title":"Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.01105","snapshot_observed_at":"2026-08-04T05:43:25.576579Z","title":"Obergaulinger and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.576579Z"},"links":{"cited_paper":"/paper/1909.01105","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:a4d830e0be61da66739970d4e721456fc6539bd1d05003e63660e12836e0d490","observation_id":"87d1a991-470b-464a-b4ab-ac3c8debe526","resolution":{"observed_at":"2026-08-04T05:43:25.576579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.00665","last_updated":"2021-07-23T15:01:44Z","snapshot_observed_at":"2026-08-16T18:27:29.671359Z","submitted_at":"2021-05-03T07:44:34Z","title":"Three-dimensional core-collapse supernovae with complex magnetic structures: I. Explosion dynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.00665","snapshot_observed_at":"2026-08-04T05:43:25.681873Z","title":"Bugli, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.681873Z"},"links":{"cited_paper":"/paper/2105.00665","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:8a3f61c651a401df9a1d85bec128458878ff182b5cc52ed3d1e6bebb29eed766","observation_id":"2ca2a82c-1098-4e4b-b679-17912bca97c1","resolution":{"observed_at":"2026-08-04T05:43:25.681873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.08432","last_updated":"2022-01-20T19:59:39Z","snapshot_observed_at":"2026-08-16T17:26:58.871523Z","submitted_at":"2022-01-20T19:59:39Z","title":"Observational signatures of stellar explosions driven by relativistic jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.08432","snapshot_observed_at":"2026-08-04T05:43:25.799171Z","title":"Eisenberg, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.799171Z"},"links":{"cited_paper":"/paper/2201.08432","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:3a1d6e685b6885aaa67b12b0a635aca9c3711cf9bfec3ebf59088a7a635732d9","observation_id":"5da63084-4d7a-44b8-bef4-b27752f803ea","resolution":{"observed_at":"2026-08-04T05:43:25.799171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14459","last_updated":"2022-12-08T12:13:01Z","snapshot_observed_at":"2026-08-16T16:35:51.951888Z","submitted_at":"2022-08-30T18:00:02Z","title":"The velocity distribution of outflows driven by choked jets in stellar envelopes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14459","snapshot_observed_at":"2026-08-04T05:43:25.889321Z","title":null,"venue":null,"work_id":null,"year":1941},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.889321Z"},"links":{"cited_paper":"/paper/2208.14459","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:71620cc6471c966a41ae7f749711a9ca09364f5d992392ab1e6e11281b30e131","observation_id":"170debac-a4f5-4458-a026-4150e0ca3e8a","resolution":{"observed_at":"2026-08-04T05:43:25.889321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.06759","last_updated":"2016-05-19T10:02:03Z","snapshot_observed_at":"2026-08-14T22:09:20.882939Z","submitted_at":"2016-02-22T13:11:05Z","title":"Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.06759","snapshot_observed_at":"2026-08-04T05:43:25.993074Z","title":"Takiwaki, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:25.993074Z"},"links":{"cited_paper":"/paper/1602.06759","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:2e1054c4f001cdd1bba4f334c60a2a7fa89a22ac633ee0bbfecc1f2d9a9102ed","observation_id":"d7c1eae7-1fd5-4c83-87f8-822746f82989","resolution":{"observed_at":"2026-08-04T05:43:25.993074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.04154","last_updated":"2017-11-22T08:17:23Z","snapshot_observed_at":"2026-08-14T20:41:30.777619Z","submitted_at":"2017-08-14T14:43:14Z","title":"Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.04154","snapshot_observed_at":"2026-08-04T05:43:26.089923Z","title":"Summa, H.-T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.089923Z"},"links":{"cited_paper":"/paper/1708.04154","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:1f84fb0de22b396c34683144440d25a32c41dc3cd5de615bc5af3b8d840305fe","observation_id":"4bc14d9e-c5c8-4c4d-8b31-5b4d02f2f8c5","resolution":{"observed_at":"2026-08-04T05:43:26.089923Z","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":"2026-08-04T05:43:26.171078Z","title":"Abdikamalov, T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.171078Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:1def105a4a9d1feaf54fc99da1ade767a0e8d3f33c5745ff0ad91db94e849a56","observation_id":"910cb508-3076-4310-85c6-f8c2265edd43","resolution":{"observed_at":"2026-08-04T05:43:26.171078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.01962","last_updated":"2023-04-27T09:18:28Z","snapshot_observed_at":"2026-08-17T09:14:12.938078Z","submitted_at":"2023-01-05T08:59:02Z","title":"Effect of stellar rotation on the development of post-shock instabilities during core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.01962","snapshot_observed_at":"2026-08-04T05:43:26.267463Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.267463Z"},"links":{"cited_paper":"/paper/2301.01962","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:fd5d2a1d510e510cd3812b61d81da4c15341dbea01a2563350ed4d2b82bd17cf","observation_id":"59dd4da2-8229-4052-ab57-ca86c262ade1","resolution":{"observed_at":"2026-08-04T05:43:26.267463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.09691","last_updated":"2024-07-23T01:33:37Z","snapshot_observed_at":"2026-08-16T13:43:07.465680Z","submitted_at":"2024-06-14T03:28:38Z","title":"The gravitational-wave emission from the explosion of a 15 solar mass star with rotation and magnetic fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.09691","snapshot_observed_at":"2026-08-04T05:43:26.438347Z","title":"Powell and B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.438347Z"},"links":{"cited_paper":"/paper/2406.09691","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:8e42135bc19e0d2c01d605923ad673737391c68951d73a562eeac92a482d47c1","observation_id":"9a240099-5fb4-4b80-801f-5f0264cb841e","resolution":{"observed_at":"2026-08-04T05:43:26.438347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.4762","last_updated":"2009-12-02T01:55:26Z","snapshot_observed_at":"2026-08-19T16:10:01.384793Z","submitted_at":"2009-07-27T20:18:07Z","title":"A Model for Gravitational Wave Emission from Neutrino-Driven Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.4762","snapshot_observed_at":"2026-08-04T05:43:26.568062Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.568062Z"},"links":{"cited_paper":"/paper/0907.4762","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:c3afa0ddd96dbd83faec2d959c0791904cc481149dc895e817035b4d6002de93","observation_id":"b00643ca-806b-4564-86e0-56dd1bc90942","resolution":{"observed_at":"2026-08-04T05:43:26.568062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01914","last_updated":"2018-05-19T01:57:46Z","snapshot_observed_at":"2026-08-17T06:50:18.539576Z","submitted_at":"2018-01-05T20:50:36Z","title":"The gravitational wave signal from core-collapse supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01914","snapshot_observed_at":"2026-08-04T05:43:26.738012Z","title":"Morozova, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.738012Z"},"links":{"cited_paper":"/paper/1801.01914","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:b0d03adf002bf12b3b31e4d7dc37bf145a11ddcb106487a0b3ce1dd5399a8ce0","observation_id":"47d70c4f-c42a-4564-9521-edff0ee27b7d","resolution":{"observed_at":"2026-08-04T05:43:26.738012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.6674","last_updated":"2013-03-25T06:07:46Z","snapshot_observed_at":"2026-08-18T08:39:39.598570Z","submitted_at":"2012-10-24T20:29:10Z","title":"General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.6674","snapshot_observed_at":"2026-08-04T05:43:26.916692Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:26.916692Z"},"links":{"cited_paper":"/paper/1210.6674","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:3c8e28209abea17bfb6c7903026b10c8f19eb7974697adcc44979e234a4a1008","observation_id":"2e42c984-289c-435a-b04b-0b609f78ede0","resolution":{"observed_at":"2026-08-04T05:43:26.916692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05824","last_updated":"2015-05-21T18:21:18Z","snapshot_observed_at":"2026-08-19T23:27:14.033424Z","submitted_at":"2015-05-21T18:21:18Z","title":"Gravitational Wave Signatures of Ab Initio Two-Dimensional Core Collapse Supernova Explosion Models for 12-25 Solar Masses Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.05824","snapshot_observed_at":"2026-08-04T05:43:27.012164Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.012164Z"},"links":{"cited_paper":"/paper/1505.05824","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:b1dd1d5f832756a71497d6aa9a00188be401b3f0b8c4e0c4cb1abdcd4a36597e","observation_id":"8202f05a-8af8-4654-8fb5-496ba4db7c99","resolution":{"observed_at":"2026-08-04T05:43:27.012164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09215","last_updated":"2016-08-24T11:29:25Z","snapshot_observed_at":"2026-08-19T03:11:01.377843Z","submitted_at":"2016-05-30T13:09:44Z","title":"A New Gravitational-Wave Signature from Standing Accretion Shock Instabilities in Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.09215","snapshot_observed_at":"2026-08-04T05:43:27.077675Z","title":"Kuroda, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.077675Z"},"links":{"cited_paper":"/paper/1605.09215","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:803129db3f606c58f3b7906ff006eae2675238cb31e45cfdf14ad668c848c5d1","observation_id":"a02e46af-42c1-4177-9a1f-0bdbf2b41a81","resolution":{"observed_at":"2026-08-04T05:43:27.077675Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-21T11:01:47.810958Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-04T05:43:27.157799Z","title":"Torres-Forn´ e, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.157799Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:7254b4a6859b9d60c90291e3a459af31e6416b83e96eb8774142f04c00e5de39","observation_id":"63927295-4987-4ff7-ab58-19556030b97d","resolution":{"observed_at":"2026-08-04T05:43:27.157799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.10643","last_updated":"2022-08-22T23:02:39Z","snapshot_observed_at":"2026-08-22T00:48:31.550337Z","submitted_at":"2022-08-22T23:02:39Z","title":"Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.10643","snapshot_observed_at":"2026-08-04T05:43:27.232217Z","title":"Mezzacappa, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.232217Z"},"links":{"cited_paper":"/paper/2208.10643","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:07ddc06414dff8b9e9dbd8da40aaeb4d85ca651183b496ce23abb0dfc543245b","observation_id":"8c7bfd43-6a85-466f-993d-512acc68ce79","resolution":{"observed_at":"2026-08-04T05:43:27.232217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.07092","last_updated":"2023-05-30T18:00:08Z","snapshot_observed_at":"2026-08-19T17:49:26.076980Z","submitted_at":"2023-02-06T19:00:01Z","title":"The Gravitational-Wave Signature of Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.07092","snapshot_observed_at":"2026-08-04T05:43:27.316042Z","title":"Vartanyan, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.316042Z"},"links":{"cited_paper":"/paper/2302.07092","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:a815285082e8d9c2b5bd9fcd3d8560ba386b01914ed4fd1895fc5a75c412493e","observation_id":"5ef11e6d-03db-460c-b28d-71a792ee67ec","resolution":{"observed_at":"2026-08-04T05:43:27.316042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.09030","last_updated":"2024-05-15T01:55:46Z","snapshot_observed_at":"2026-08-16T13:52:38.600579Z","submitted_at":"2024-05-15T01:55:46Z","title":"Universality in supernova gravitational waves with proto-neutron star properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.09030","snapshot_observed_at":"2026-08-04T05:43:27.448355Z","title":"Sotani, B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.448355Z"},"links":{"cited_paper":"/paper/2405.09030","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:97a61c62f6781c693196416848988b16d38b5119188d22a629188a1b5eb3b387","observation_id":"dccfbb5b-7104-4c15-9ca2-7871916ebd0f","resolution":{"observed_at":"2026-08-04T05:43:27.448355Z","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":"2026-08-04T05:43:27.691028Z","title":"Ehring, S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.691028Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:cad79500dd22eecc9ac7d98fe5e828adf9313a48ce6d0ce588a27efd124bed94","observation_id":"2ef69268-ecd1-4f51-941d-74ddb7505a6d","resolution":{"observed_at":"2026-08-04T05:43:27.691028Z","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":"2026-08-04T05:43:27.763200Z","title":"Lella, G","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.763200Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:98940d4fee72e1057f76ab41218884573befd031b315ab694dc015b70bc925d2","observation_id":"00af0e29-177c-472b-94fd-5d64c2e6dd7d","resolution":{"observed_at":"2026-08-04T05:43:27.763200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.0512","last_updated":"2013-03-25T06:12:03Z","snapshot_observed_at":"2026-08-15T04:14:14.428196Z","submitted_at":"2012-04-02T20:00:00Z","title":"Correlated Gravitational Wave and Neutrino Signals from General-Relativistic Rapidly Rotating Iron Core Collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.0512","snapshot_observed_at":"2026-08-04T05:43:27.875760Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.875760Z"},"links":{"cited_paper":"/paper/1204.0512","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:d47c39b3b5065e291b6a05b227e359ecfdb2c2c68fbc53e1e4a52294fbe033b1","observation_id":"830d083e-d084-4ee1-9878-b6b5e83cf897","resolution":{"observed_at":"2026-08-04T05:43:27.875760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.06951","last_updated":"2015-04-29T19:23:32Z","snapshot_observed_at":"2026-08-14T23:02:27.173646Z","submitted_at":"2015-01-27T22:51:31Z","title":"Supernova Seismology: Gravitational Wave Signatures of Rapidly Rotating Core Collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.06951","snapshot_observed_at":"2026-08-04T05:43:28.006274Z","title":"Fuller, H","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.006274Z"},"links":{"cited_paper":"/paper/1501.06951","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:46859c696506d90bdef114c5b3a966afac3b004e39a069c06102f709bb3e1d66","observation_id":"97c90e9d-045f-42c3-b7ee-849942ea0e80","resolution":{"observed_at":"2026-08-04T05:43:28.006274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0168","last_updated":"2008-07-07T15:34:05Z","snapshot_observed_at":"2026-08-15T10:33:08.833620Z","submitted_at":"2007-09-03T08:54:59Z","title":"Gravitational waves from 3D MHD core collapse simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0168","snapshot_observed_at":"2026-08-04T05:43:28.088011Z","title":"Scheidegger, T","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.088011Z"},"links":{"cited_paper":"/paper/0709.0168","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:410930ba176439c282ff1696940473a914597069d3b5b792c71a4693ec5f9c6c","observation_id":"b570bd15-ce15-4b54-b500-f3f94e59e0e8","resolution":{"observed_at":"2026-08-04T05:43:28.088011Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.09730","last_updated":"2020-02-06T07:18:56Z","snapshot_observed_at":"2026-08-13T22:26:54.134754Z","submitted_at":"2019-09-20T21:59:31Z","title":"A New Gravitational Wave Signature of Low-$T/|W|$ Instability in Rapidly Rotating Stellar Core Collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.09730","snapshot_observed_at":"2026-08-04T05:43:28.301320Z","title":"Shibagaki, T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.301320Z"},"links":{"cited_paper":"/paper/1909.09730","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:e83cdb5d2ecd384ac6c8bbee3bd5497d0c8187abe05e883adac30f4d1228bd3d","observation_id":"85a98deb-0157-421c-9a1a-74e5b601b8e4","resolution":{"observed_at":"2026-08-04T05:43:28.301320Z","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":"2026-08-04T05:43:28.421506Z","title":"Mueller and H","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.421506Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:d0c2d13b1fea7a1b6afbd93078c857887d7bbb925750392a90c8255b7cd407e1","observation_id":"31d49506-6c1b-4a56-a320-406cb902cd9a","resolution":{"observed_at":"2026-08-04T05:43:28.421506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.01525","last_updated":"2025-05-06T16:11:21Z","snapshot_observed_at":"2026-08-19T23:57:57.998245Z","submitted_at":"2024-08-02T18:35:58Z","title":"Gravitational-Wave and Gravitational-Wave Memory Signatures of Core-Collapse Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.01525","snapshot_observed_at":"2026-08-04T05:43:28.510263Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.510263Z"},"links":{"cited_paper":"/paper/2408.01525","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:90d01cca22b1c673346080f3cf1414b1c520373a5606ce7efa21ebeeb088caec","observation_id":"a6cc6696-2fb2-4ef0-94e3-35c7d77fc561","resolution":{"observed_at":"2026-08-04T05:43:28.510263Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.6301","last_updated":"2011-12-05T13:05:34Z","snapshot_observed_at":"2026-08-15T04:42:24.646990Z","submitted_at":"2011-06-30T16:49:58Z","title":"Parametrized 3D models of neutrino-driven supernova explosions: Neutrino emission asymmetries and gravitational-wave signals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.6301","snapshot_observed_at":"2026-08-04T05:43:28.629001Z","title":"M¨ uller, H.-T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.629001Z"},"links":{"cited_paper":"/paper/1106.6301","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:96f639876d38377d491e71067962423c9d09f08f16ca9acfaa6b6ccd3a9ce488","observation_id":"b5c9a761-9e7c-4fce-948c-93d0ab542b61","resolution":{"observed_at":"2026-08-04T05:43:28.629001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.07703","last_updated":"2019-04-23T17:20:22Z","snapshot_observed_at":"2026-08-14T17:41:32.429585Z","submitted_at":"2018-12-18T23:58:08Z","title":"Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.07703","snapshot_observed_at":"2026-08-04T05:43:28.759776Z","title":"Radice, V","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.759776Z"},"links":{"cited_paper":"/paper/1812.07703","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:87f0518d45e38dc3d210e1b6a36fef3a45e8b6905db7ec232b3d6178fc91280b","observation_id":"9183eacd-2b91-4c40-8e83-ad95f1813049","resolution":{"observed_at":"2026-08-04T05:43:28.759776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.5713","last_updated":"2013-06-18T17:06:09Z","snapshot_observed_at":"2026-08-17T09:40:49.115593Z","submitted_at":"2013-02-22T21:15:11Z","title":"Gravitational Wave Memory from Gamma Ray Bursts' Jets","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.5713","snapshot_observed_at":"2026-08-04T05:43:28.888694Z","title":"Birnholtz and T","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:28.888694Z"},"links":{"cited_paper":"/paper/1302.5713","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:a7707537e8edfc7581c40b252eb92cea83dd57ff871cb246aef72e623aeb9bd3","observation_id":"1e44230c-8694-481c-b0a7-39b278bac00f","resolution":{"observed_at":"2026-08-04T05:43:28.888694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.09256","last_updated":"2023-06-21T01:28:08Z","snapshot_observed_at":"2026-08-16T16:31:24.609857Z","submitted_at":"2022-09-19T18:00:01Z","title":"Jetted and Turbulent Stellar Deaths: New LVK-Detectable Gravitational Wave Sources","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.09256","snapshot_observed_at":"2026-08-04T05:43:29.068939Z","title":"Gottlieb, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.068939Z"},"links":{"cited_paper":"/paper/2209.09256","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:e13316be46ab91e136a32b4bff5abfea78364216f638a11a6ded2e676effaa6b","observation_id":"dc7f39f9-05f4-4dee-b0fa-38eb4a08511c","resolution":{"observed_at":"2026-08-04T05:43:29.068939Z","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":"2026-08-04T05:43:29.143125Z","title":"Cusinato, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.143125Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:1605413df121ad80777e84d9ec1f3012882ddd7191d44a2635de27da457b0dd8","observation_id":"5da45ebe-a55f-4974-b709-1598416f7449","resolution":{"observed_at":"2026-08-04T05:43:29.143125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.3678","last_updated":"2013-11-14T21:24:03Z","snapshot_observed_at":"2026-08-14T23:55:14.523922Z","submitted_at":"2013-11-14T21:24:03Z","title":"Measuring the Angular Momentum Distribution in Core-Collapse Supernova Progenitors with Gravitational Waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.3678","snapshot_observed_at":"2026-08-04T05:43:29.194786Z","title":"Abdikamalov, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.194786Z"},"links":{"cited_paper":"/paper/1311.3678","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:3e7b1b1f98f948cc98f607036d99025176e8bf2611bf21d3f856987c6321972b","observation_id":"0ab82dcd-ae44-4609-b813-f730a3025880","resolution":{"observed_at":"2026-08-04T05:43:29.194786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09055","last_updated":"2019-06-30T01:51:09Z","snapshot_observed_at":"2026-08-14T17:25:45.608114Z","submitted_at":"2019-01-25T19:15:44Z","title":"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.09055","snapshot_observed_at":"2026-08-04T05:43:29.262089Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.262089Z"},"links":{"cited_paper":"/paper/1901.09055","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:de498fec1d8cbfdde404bd35ddf19d267cf992f2817bace1762536c0a67fd732","observation_id":"8519bacb-5aea-4027-a9c5-cb56cf59d429","resolution":{"observed_at":"2026-08-04T05:43:29.262089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3256","last_updated":"2012-02-23T11:02:09Z","snapshot_observed_at":"2026-08-16T11:10:41.999145Z","submitted_at":"2012-02-15T10:08:35Z","title":"Inferring Core-Collapse Supernova Physics with Gravitational Waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3256","snapshot_observed_at":"2026-08-04T05:43:29.395073Z","title":"Logue, C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.395073Z"},"links":{"cited_paper":"/paper/1202.3256","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:166a4fd211108021ac829d75ef7ddce59a69598d2c1207a6cdf36eba8e2341af","observation_id":"ded7b7f0-81ce-40a8-89a8-0a1cce1078d6","resolution":{"observed_at":"2026-08-04T05:43:29.395073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.18221","last_updated":"2024-02-28T23:00:04Z","snapshot_observed_at":"2026-08-18T05:21:38.252175Z","submitted_at":"2023-11-30T03:31:52Z","title":"Determining the core-collapse supernova explosion mechanism with current and future gravitational-wave observatories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.18221","snapshot_observed_at":"2026-08-04T05:43:29.497575Z","title":"Powell, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.497575Z"},"links":{"cited_paper":"/paper/2311.18221","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:87c62b468b253b2fa33ecce6b25ebebff776d8776be378f34202b8f2c6913d61","observation_id":"62e529d1-a47e-49b9-bfcb-feef40b6528f","resolution":{"observed_at":"2026-08-04T05:43:29.497575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.00846","last_updated":"2021-11-15T15:13:31Z","snapshot_observed_at":"2026-08-19T23:57:23.727177Z","submitted_at":"2020-12-01T21:34:25Z","title":"Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.00846","snapshot_observed_at":"2026-08-04T05:43:29.621210Z","title":"Bizouard, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.621210Z"},"links":{"cited_paper":"/paper/2012.00846","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:36371b2c28a37f08c80d36be13b6c72b382686cf99d70fc3cc783d4712c6561c","observation_id":"cebe4adf-ab22-4618-9702-01ce055e368f","resolution":{"observed_at":"2026-08-04T05:43:29.621210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.03131","last_updated":"2021-11-25T15:09:33Z","snapshot_observed_at":"2026-08-16T17:51:17.407637Z","submitted_at":"2021-10-07T01:07:33Z","title":"Universal relation for supernova gravitational waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.03131","snapshot_observed_at":"2026-08-04T05:43:29.705140Z","title":"Sotani, T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.705140Z"},"links":{"cited_paper":"/paper/2110.03131","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:7778f7fa2e0929a63e6dab4de8523e19ee5eb387869aa35e1543c57598161a4e","observation_id":"f9c3c182-5918-44ab-8909-c6657471974b","resolution":{"observed_at":"2026-08-04T05:43:29.705140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.10019","last_updated":"2023-07-06T09:24:57Z","snapshot_observed_at":"2026-08-16T16:00:29.525280Z","submitted_at":"2023-01-24T14:05:58Z","title":"Inference of proto-neutron star properties in core-collapse supernovae from a gravitational-wave detector network","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.10019","snapshot_observed_at":"2026-08-04T05:43:29.765576Z","title":"Bruel, M.-A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.765576Z"},"links":{"cited_paper":"/paper/2301.10019","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:026f10646a0c6f79671413140f4957d3268a91be022032daea6bc343c800d109","observation_id":"678aa698-3959-4264-8fe4-bda96d1d12fc","resolution":{"observed_at":"2026-08-04T05:43:29.765576Z","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":"2026-08-04T05:43:29.830317Z","title":"Casallas-Lagos, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.830317Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:c6697d8786eff88d6a57a125627a2f15fac1722e062351323f117798371613b9","observation_id":"1343bcc4-56e2-4204-9ad5-6395faf43569","resolution":{"observed_at":"2026-08-04T05:43:29.830317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.02752","last_updated":"2017-03-03T18:51:23Z","snapshot_observed_at":"2026-08-14T21:21:45.691835Z","submitted_at":"2017-01-10T19:01:10Z","title":"Equation of State Effects on Gravitational Waves from Rotating Core Collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.02752","snapshot_observed_at":"2026-08-04T05:43:29.966582Z","title":"Richers, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:29.966582Z"},"links":{"cited_paper":"/paper/1701.02752","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:3ec4f51e93806a37247e37b3dc744e26cbdfa9d284766f3c9812fa5dfe820bed","observation_id":"9ccf992c-bcc7-4c39-a1a4-910e32995055","resolution":{"observed_at":"2026-08-04T05:43:29.966582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.07367","last_updated":"2021-01-17T06:28:03Z","snapshot_observed_at":"2026-08-07T06:35:34.217217Z","submitted_at":"2020-09-15T22:04:59Z","title":"Classifying the Equation of State from Rotating Core Collapse Gravitational Waves with Deep Learning","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.07367","snapshot_observed_at":"2026-08-04T05:43:30.090230Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.090230Z"},"links":{"cited_paper":"/paper/2009.07367","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:b35e2099fc99bdb7153f401aea60c9fb8a04ce6bf60d56d01a88dc9ceba0aa79","observation_id":"3c759a69-9635-45f0-ac51-f899d2f1bf66","resolution":{"observed_at":"2026-08-04T05:43:30.090230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.10089","last_updated":"2022-09-21T03:46:15Z","snapshot_observed_at":"2026-08-16T16:31:02.472761Z","submitted_at":"2022-09-21T03:46:15Z","title":"Determine the Core Structure and Nuclear Equation of State of Rotating Core-Collapse Supernovae with Gravitational Waves by Convolutional Neural Networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.10089","snapshot_observed_at":"2026-08-04T05:43:30.172630Z","title":"Chao, C.-Z","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.172630Z"},"links":{"cited_paper":"/paper/2209.10089","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:57d16e4e8b8f1af4c5abebd7c46ba6029e52a49175cbc60a5757e2b6ce93c8fd","observation_id":"944fdfb7-b35a-494f-85b7-18c3b548f96f","resolution":{"observed_at":"2026-08-04T05:43:30.172630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.16962","last_updated":"2023-03-29T18:50:05Z","snapshot_observed_at":"2026-08-21T17:28:57.929318Z","submitted_at":"2023-03-29T18:50:05Z","title":"Gravitational Wave Eigenfrequencies from Neutrino-Driven Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.16962","snapshot_observed_at":"2026-08-04T05:43:30.298187Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.298187Z"},"links":{"cited_paper":"/paper/2303.16962","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:4b3f638c7b02169a087364a8d18df8cd4cc5e9bba63c582e5e0fe30dfcb379f8","observation_id":"a89408be-2af0-4658-a1d3-c5b917875620","resolution":{"observed_at":"2026-08-04T05:43:30.298187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01784","last_updated":"2024-07-30T16:56:52Z","snapshot_observed_at":"2026-08-16T13:46:32.414952Z","submitted_at":"2024-06-03T21:03:16Z","title":"Dependence of the Reconstructed Core-Collapse Supernova Gravitational Wave High-Frequency Feature on the Nuclear Equation of State, in Real Interferometric Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.01784","snapshot_observed_at":"2026-08-04T05:43:30.383343Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.383343Z"},"links":{"cited_paper":"/paper/2406.01784","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:f411aa1ff066455b6dff41923151efc5d56544fbfcadafd1dc29b7a476b89c87","observation_id":"9dc22440-398f-46d2-af67-d458a16198f6","resolution":{"observed_at":"2026-08-04T05:43:30.383343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.15649","last_updated":"2024-03-07T20:54:49Z","snapshot_observed_at":"2026-08-20T12:12:31.922217Z","submitted_at":"2023-10-24T09:08:22Z","title":"Probing nuclear physics with supernova gravitational waves and machine learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.15649","snapshot_observed_at":"2026-08-04T05:43:30.459028Z","title":"Mitra, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.459028Z"},"links":{"cited_paper":"/paper/2310.15649","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:83e78e26eadd66d8ab5a87de5a9e4db7657b7983028a0737e6e8f539d93ddd1f","observation_id":"8cb1193c-4c5d-4d99-af69-1caa14d221d8","resolution":{"observed_at":"2026-08-04T05:43:30.459028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.14508","last_updated":"2025-01-06T17:25:17Z","snapshot_observed_at":"2026-08-16T13:16:29.027203Z","submitted_at":"2024-09-22T16:11:25Z","title":"Evaluating Machine Learning Models for Supernova Gravitational Wave Signal Classification","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.14508","snapshot_observed_at":"2026-08-04T05:43:30.543822Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.543822Z"},"links":{"cited_paper":"/paper/2409.14508","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:4c2a91e0d2881aa46d12e1acac06e8e24c32f9596cac85307814695739b1f4ba","observation_id":"cb7395fa-613f-4cd5-a519-b3166d2ec917","resolution":{"observed_at":"2026-08-04T05:43:30.543822Z","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":"2026-08-04T05:43:30.643803Z","title":"Sultan Abylkairov, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.643803Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:bc289f3fbd6d88aeebe7014f229b64c24b1d4ab0175701f468cea7e61250dd06","observation_id":"79b83acd-59f5-4c38-9025-387a59e53291","resolution":{"observed_at":"2026-08-04T05:43:30.643803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.18080","last_updated":"2026-06-26T11:37:39Z","snapshot_observed_at":"2026-08-16T08:27:09.645325Z","submitted_at":"2025-08-25T14:46:07Z","title":"GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18080","snapshot_observed_at":"2026-08-04T05:43:30.756046Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.756046Z"},"links":{"cited_paper":"/paper/2508.18080","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:f4c4045a472d7dc88fc37ad7b965773c91f66f8850c3ecdb3110fc122be2c0bc","observation_id":"be82ea40-a6c6-4b74-9403-9478b02f6a92","resolution":{"observed_at":"2026-08-04T05:43:30.756046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0700","last_updated":"2009-10-27T17:24:19Z","snapshot_observed_at":"2026-08-17T16:35:22.476848Z","submitted_at":"2009-08-05T16:40:22Z","title":"Progenitors of core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0700","snapshot_observed_at":"2026-08-04T05:43:30.836035Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.836035Z"},"links":{"cited_paper":"/paper/0908.0700","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:f5bf8676f3f3a30e328af11da6d31f5eb3d1d3abce008ef5ab0209d0eca3c4d2","observation_id":"06788279-6617-425d-ac35-3c022aa1553d","resolution":{"observed_at":"2026-08-04T05:43:30.836035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.03243","last_updated":"2018-03-22T20:11:06Z","snapshot_observed_at":"2026-08-14T20:25:29.855421Z","submitted_at":"2017-10-09T18:00:08Z","title":"High Resolution Study of Presupernova Compactness","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.03243","snapshot_observed_at":"2026-08-04T05:43:30.932260Z","title":"Sukhbold, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:30.932260Z"},"links":{"cited_paper":"/paper/1710.03243","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:24a767c5648941ed16a2810400f499a1fd2b15369736e0504e3dc1c8adb3b3aa","observation_id":"f3194d96-8031-4762-8bf0-8de7b84acd20","resolution":{"observed_at":"2026-08-04T05:43:30.932260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.1191","last_updated":"2009-03-06T12:02:48Z","snapshot_observed_at":"2026-08-15T05:53:30.100800Z","submitted_at":"2009-03-06T12:02:48Z","title":"Neutrinos from Supernovae as a Trigger for Gravitational Wave Search","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.1191","snapshot_observed_at":"2026-08-04T05:43:31.015164Z","title":"Pagliaroli, F","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.015164Z"},"links":{"cited_paper":"/paper/0903.1191","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:0db74e0d9d1fb4d3670cabe6fa1c48a09b67ab776ffaf0fdf0008e7e9eb7ee1b","observation_id":"93d6d535-1dda-446b-b7b9-18a5085452b6","resolution":{"observed_at":"2026-08-04T05:43:31.015164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.2317","last_updated":"2009-10-16T10:17:30Z","snapshot_observed_at":"2026-08-15T05:41:24.533675Z","submitted_at":"2009-08-17T09:56:06Z","title":"Reconstructing the supernova bounce time with neutrinos in IceCube","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.2317","snapshot_observed_at":"2026-08-04T05:43:31.172200Z","title":"Halzen and G","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.172200Z"},"links":{"cited_paper":"/paper/0908.2317","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:3ecf9a8be9092b7e0ea09bad0ea2cbe7904fd75b921f4f9c5f54cc3dbe6559c7","observation_id":"bad2fcbc-d82d-44cf-9cd0-f55aff16b1e9","resolution":{"observed_at":"2026-08-04T05:43:31.172200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0204288","last_updated":"2002-04-17T18:19:36Z","snapshot_observed_at":"2026-07-07T00:26:01.431611Z","submitted_at":"2002-04-17T18:19:36Z","title":"Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0204288","snapshot_observed_at":"2026-08-04T05:43:31.303572Z","title":"Dimmelmeier, J","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.303572Z"},"links":{"cited_paper":"/paper/astro-ph/0204288","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:5673887306d01e43d740b50b0e8abfeadffa76a0cd037a757c9a462e94250d29","observation_id":"9c9b64ea-97cd-4a29-a04d-5da3cdd83735","resolution":{"observed_at":"2026-08-04T05:43:31.303572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0407174","last_updated":"2005-03-02T09:51:00Z","snapshot_observed_at":"2026-08-15T03:37:42.614043Z","submitted_at":"2004-07-08T18:04:00Z","title":"\"Mariage des Maillages\": A new numerical approach for 3D relativistic core collapse simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0407174","snapshot_observed_at":"2026-08-04T05:43:31.449091Z","title":"Dimmelmeier, J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.449091Z"},"links":{"cited_paper":"/paper/astro-ph/0407174","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:d0c3503178ab8f6d49893443acbf6127a850779287bdcccc87dc97761269b997","observation_id":"518cba2e-fe4f-46fe-8f65-f0d88e912b4e","resolution":{"observed_at":"2026-08-04T05:43:31.449091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14542","last_updated":"2023-01-11T22:16:30Z","snapshot_observed_at":"2026-08-16T16:28:17.295170Z","submitted_at":"2022-09-29T04:16:50Z","title":"Exploring Supernova Gravitational Waves with Machine Learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14542","snapshot_observed_at":"2026-08-04T05:43:31.579074Z","title":"Mitra, B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.579074Z"},"links":{"cited_paper":"/paper/2209.14542","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:684f7971273073e81845d12a4b460e5e11e3a32ab647881488d402e525c41da5","observation_id":"d9d9397d-2211-4190-8d2c-ad23257162ca","resolution":{"observed_at":"2026-08-04T05:43:31.579074Z","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":"2026-08-04T05:43:31.681632Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.681632Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:48f87047e96fcdcd0d86351ffac09ff6fff1a0cde14428312867edb7289daef4","observation_id":"e0d4549d-78e4-4578-bd20-68fac5457d10","resolution":{"observed_at":"2026-08-04T05:43:31.681632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504072","last_updated":"2005-07-16T21:25:50Z","snapshot_observed_at":"2026-08-21T09:46:29.381448Z","submitted_at":"2005-04-04T15:44:42Z","title":"A simple parameterization of the consequences of deleptonization for simulations of stellar core collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504072","snapshot_observed_at":"2026-08-04T05:43:31.704306Z","title":"Liebend¨ orfer, A Simple Parameterization of the Con- sequences of Deleptonization for Simulations of Stel- lar Core Collapse, Astrophys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.704306Z"},"links":{"cited_paper":"/paper/astro-ph/0504072","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:8dee552f3754f797adfb141e5101b658d309b3d24719e87cb937dcf287b0657a","observation_id":"4d5f5a99-0c5c-4a8b-b101-5c6d6ea4d138","resolution":{"observed_at":"2026-08-04T05:43:31.704306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702176","last_updated":"2007-02-06T23:50:55Z","snapshot_observed_at":"2026-08-20T00:48:37.315091Z","submitted_at":"2007-02-06T23:50:55Z","title":"Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0702176","snapshot_observed_at":"2026-08-04T05:43:31.821530Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.821530Z"},"links":{"cited_paper":"/paper/astro-ph/0702176","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:4f3fd205ff4c39c996c7b5c4610388231cc55dfd17868cbb9e3dea0aa33cc252","observation_id":"67ae4465-fe6a-4312-b257-0472e9dbdbb8","resolution":{"observed_at":"2026-08-04T05:43:31.821530Z","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":"2026-08-04T05:43:31.967419Z","title":"Heger, S","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:31.967419Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:7781128148f5f13dfe1ed69192b44f4eadd197ab469cee3a86ada4953a792169","observation_id":"45aecae4-f3ff-4fed-b650-de161712b2d0","resolution":{"observed_at":"2026-08-04T05:43:31.967419Z","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":"2026-08-04T05:43:32.121595Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.121595Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:7a3e3d8a65297c4cd15823ccb9c96f5d0ce4d736fe290dca09bb3b28a98baa84","observation_id":"9105b3b1-9817-4196-ba08-a3171351a975","resolution":{"observed_at":"2026-08-04T05:43:32.121595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.2184","last_updated":"2012-07-09T21:00:43Z","snapshot_observed_at":"2026-08-15T00:53:51.994483Z","submitted_at":"2012-07-09T21:00:43Z","title":"Core-collapse supernova equations of state based on neutron star observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.2184","snapshot_observed_at":"2026-08-04T05:43:32.181148Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.181148Z"},"links":{"cited_paper":"/paper/1207.2184","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:ea20e1fc8eb392cac6c330b60fd68dcb1ca9e3867caeb71de19a8330a09ff349","observation_id":"400b100c-1bc2-43d9-beb3-2a515b7920d1","resolution":{"observed_at":"2026-08-04T05:43:32.181148Z","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":"2026-08-04T05:43:32.323332Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.323332Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:b1006b4d80c303b65528b0437717bf8943ccfae5e2c7f8f907695ac441ff0592","observation_id":"f223b9db-bef2-44dd-b3db-e1e381a5e479","resolution":{"observed_at":"2026-08-04T05:43:32.323332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.4073","last_updated":"2009-11-20T18:41:34Z","snapshot_observed_at":"2026-08-16T17:45:23.823475Z","submitted_at":"2009-11-20T18:41:34Z","title":"Statistical Model for a Complete Supernova Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.4073","snapshot_observed_at":"2026-08-04T05:43:32.541137Z","title":"Hempel and J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.541137Z"},"links":{"cited_paper":"/paper/0911.4073","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:67c87782a4af337a4b36ad22b3774c03d4330f45751d1b47d69af581360271da","observation_id":"a58e6522-06d4-448f-a697-409207a966e3","resolution":{"observed_at":"2026-08-04T05:43:32.541137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0848","last_updated":"2012-11-22T15:11:18Z","snapshot_observed_at":"2026-08-18T13:49:02.027374Z","submitted_at":"2011-08-03T14:08:54Z","title":"New Equations of State in Simulations of Core-Collapse Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0848","snapshot_observed_at":"2026-08-04T05:43:32.649282Z","title":"Hempel, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.649282Z"},"links":{"cited_paper":"/paper/1108.0848","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:f1e57ce914f424c1b7c0d8dde6762256af1a619d62c1721dc0ae239e798494d2","observation_id":"83e8dc52-c93b-4150-8531-967474b51bd8","resolution":{"observed_at":"2026-08-04T05:43:32.649282Z","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":"2026-08-04T05:43:32.755446Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.755446Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:7e759acbcbb6242bfc3e341ca80377de26f6a25c6bc380d0d16b9be18c8b8625","observation_id":"53a998c4-8c74-4aa7-b1ae-8d8c017abebe","resolution":{"observed_at":"2026-08-04T05:43:32.755446Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.5241","last_updated":"2012-10-18T20:00:00Z","snapshot_observed_at":"2026-08-20T13:01:43.776827Z","submitted_at":"2012-10-18T20:00:00Z","title":"Dimensional Dependence of the Hydrodynamics of Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.5241","snapshot_observed_at":"2026-08-04T05:43:32.840764Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.840764Z"},"links":{"cited_paper":"/paper/1210.5241","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:fb81d30687271ab60543d4f93eb67df3eda96cbcbab79d14db4a68a176ab1012","observation_id":"e8ebd647-dda4-4f65-9d0a-a2b997d9a6f7","resolution":{"observed_at":"2026-08-04T05:43:32.840764Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.05139","last_updated":"2015-07-16T04:14:17Z","snapshot_observed_at":"2026-08-16T23:37:41.462991Z","submitted_at":"2015-06-16T20:24:28Z","title":"The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.05139","snapshot_observed_at":"2026-08-04T05:43:32.940636Z","title":"M¨ uller, The dynamics of neutrino-driven supernova explosions after shock revival in 2D and 3D, MNRAS 453, 287 (2015), arXiv:1506.05139 [astro-ph.SR]","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:32.940636Z"},"links":{"cited_paper":"/paper/1506.05139","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:b02fce37489c2bb54df907c4d7347320cd53d008987b2a076a8232ae5d7e11a5","observation_id":"905a6b12-d3a3-42a5-b034-8b140d58d628","resolution":{"observed_at":"2026-08-04T05:43:32.940636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.06662","last_updated":"2020-03-14T15:55:35Z","snapshot_observed_at":"2026-08-09T06:13:31.834327Z","submitted_at":"2020-03-14T15:55:35Z","title":"Magnetar formation through a convective dynamo in protoneutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.06662","snapshot_observed_at":"2026-08-04T05:43:33.144601Z","title":"Raynaud, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:33.144601Z"},"links":{"cited_paper":"/paper/2003.06662","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:170af11534366529bae615d4fdfc3df309087e725c114f10936b59ffb27c68f3","observation_id":"abe7701f-c27a-4c24-832f-245094cb6bf5","resolution":{"observed_at":"2026-08-04T05:43:33.144601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.05022","last_updated":"2016-03-22T22:10:32Z","snapshot_observed_at":"2026-08-14T22:27:29.080575Z","submitted_at":"2015-10-16T20:47:09Z","title":"Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.05022","snapshot_observed_at":"2026-08-04T05:43:33.330844Z","title":"Radice, C","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:33.330844Z"},"links":{"cited_paper":"/paper/1510.05022","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:2bfbea2735238e7c293c550baf7a9b5f3a2c711220b1ae978a6347558917f472","observation_id":"803c2638-55cf-4a24-b20d-d4bcbfe7441c","resolution":{"observed_at":"2026-08-04T05:43:33.330844Z","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":"2026-08-04T05:43:33.431803Z","title":null,"venue":null,"work_id":null,"year":1967},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:33.431803Z"},"links":{"citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:23557e478b2b9bd4028ef6897f4e9abe304da66e5b149924e0997690f74e4851","observation_id":"a1419f60-0ab3-4541-99ac-b462c1ff441f","resolution":{"observed_at":"2026-08-04T05:43:33.431803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T16:16:34.560805Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":104},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 3 inbound Pith citation observations for arXiv:2603.27680."}