{"as_of":"2026-08-11T19:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a739bb1281832517c25734f10f2c1e4d565da267160d7c3e04bb4c0885d98e1e","coverage":[{"denominator":114,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T14:01:09.004267Z","state":"measured"},{"denominator":104,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":104,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:40:52.724580Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-11T08:30:57.586610Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15810","snapshot_observed_at":"2026-08-07T04:40:52.724580Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.10065","last_updated":"2025-06-11T18:00:00Z","snapshot_observed_at":"2026-08-10T23:18:40.560044Z","submitted_at":"2025-06-11T18:00:00Z","title":"Locating the QCD critical point with neutron-star observations","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T04:40:52.724580Z"},"links":{"cited_paper":"/paper/2501.15810","citing_paper":"/paper/2506.10065"},"observation_digest":"sha256:f2c8da25749f1365ce9c741af0d37d7e87c585eac59a86a3688a73d391423d58","observation_id":"c90e2d4f-5fe2-496a-b499-87705507fed8","resolution":{"observed_at":"2026-08-07T04:40:52.724580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15810","snapshot_observed_at":"2026-08-05T19:46:32.620313Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.11872","last_updated":"2026-05-23T02:23:15Z","snapshot_observed_at":"2026-08-11T01:55:31.847999Z","submitted_at":"2025-08-16T02:12:39Z","title":"Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-05T19:46:32.620313Z"},"links":{"cited_paper":"/paper/2501.15810","citing_paper":"/paper/2508.11872"},"observation_digest":"sha256:d682fe641d6ca3cdb720346ca62043271706aa0b0f7e72da481e9bc5fd1031c8","observation_id":"ddebaef4-588d-44c1-8e9e-ff853f74c089","resolution":{"observed_at":"2026-08-05T19:46:32.620313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15810","snapshot_observed_at":"2026-08-03T12:52:08.589474Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.01495","last_updated":"2026-06-16T10:49:44Z","snapshot_observed_at":"2026-08-08T17:56:57.753787Z","submitted_at":"2026-01-04T11:42:55Z","title":"Discovering the Gell-Mann-Okubo Formula with Kolmogorov-Arnold Networks","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-03T12:52:08.589474Z"},"links":{"cited_paper":"/paper/2501.15810","citing_paper":"/paper/2601.01495"},"observation_digest":"sha256:d4827063041912fd4eee1f66538761f44e9a0779741a655a320cf8f1d6be71cf","observation_id":"9100d342-30dc-472b-83de-aa0a4c485bf1","resolution":{"observed_at":"2026-08-03T12:52:08.589474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"cited_work":{"arxiv_id":"2501.15810","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15810","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"d49b43e2-1b88-48a1-aed0-0fe17b0c021b","year":2025},"citing_paper":{"arxiv_id":"2604.11046","last_updated":"2026-04-13T06:22:40Z","snapshot_observed_at":"2026-08-11T19:16:07.993373Z","submitted_at":"2026-04-13T06:22:40Z","title":"Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-10T16:35:52.640568Z"},"links":{"cited_paper":"/paper/2501.15810","citing_paper":"/paper/2604.11046"},"observation_digest":"sha256:5d0f509f506b85b8b8b70c7cc9188460f2248501b6a3f4ecf90bb4f8bb698c64","observation_id":"0ca17c0a-31b5-45b6-83c8-b3afb36c8dbf","resolution":{"observed_at":"2026-05-11T08:30:57.588131Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2501.15810/citation-record","integrity":"/paper/2501.15810/integrity","json":"/paper/2501.15810/citation-record.json","paper":"/paper/2501.15810"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T14:01:08.497012Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.497012Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:e805109d7e075901cad4cb0392ba73d4aab7825d7357115136b00ccdd2d4a231","observation_id":"6d2f91c0-1831-49b4-af1c-0619fea68513","resolution":{"observed_at":"2026-08-10T14:01:08.497012Z","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":"2026-08-10T14:01:08.502454Z","title":"Note that the change in the inverse sound speed squared is given by κs(ξ) → κs(ξ) + d∆ε(ξ) P dξ δε, correspondingly","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.502454Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:acc78fba56365207c743dd5ae99c344320aecc4e33e82f038a16e86727f64c50","observation_id":"04a93c1b-2fe5-4736-ae22-fe54554a9414","resolution":{"observed_at":"2026-08-10T14:01:08.502454Z","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":"2026-08-10T14:01:08.512448Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.512448Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:273fd269a2ba4ffdb39c92ba34fbc8924dc28beae6b20cad45f65ceed65bc460","observation_id":"ac369447-31b2-4c9c-894f-a371ed8c27df","resolution":{"observed_at":"2026-08-10T14:01:08.512448Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-10T14:01:08.517404Z","title":"observational values","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.517404Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:1326bb50b0cb9c2750c52569e2ee8e5ca5654075737b8bc4f9286a7661f51691","observation_id":"1fd40a87-7bf6-4000-b4d1-60383cd498ab","resolution":{"observed_at":"2026-08-10T14:01:08.517404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.13253","last_updated":"2024-01-25T19:51:49Z","snapshot_observed_at":"2026-08-07T18:34:24.476260Z","submitted_at":"2023-01-30T19:38:32Z","title":"Dense Nuclear Matter Equation of State from Heavy-Ion Collisions","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.13253","snapshot_observed_at":"2026-08-10T14:01:08.559709Z","title":"Sorensen et al., Prog","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.559709Z"},"links":{"cited_paper":"/paper/2301.13253","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:85ee196eb8ccf1a80943a23cddc5ec5f6f0355879855c27d96f7948c7ad67950","observation_id":"81745a54-ad1f-4364-8631-96abb0c9cbde","resolution":{"observed_at":"2026-08-10T14:01:08.559709Z","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":"2026-08-10T14:01:08.523582Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.523582Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:ee0ee2f897344a6f459ea45bb694f5e396dfc02aac0f408d575a00705bfa2d94","observation_id":"9d817593-98de-40f2-a415-335761eff800","resolution":{"observed_at":"2026-08-10T14:01:08.523582Z","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":"2026-08-10T14:01:08.528590Z","title":"In MCMC, the parameter ensemble is sampled one after another as a chain","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.528590Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:4bb06a773251b109a54e5aa18157e07e409240de73f60df46e486c2650615ca6","observation_id":"19b53d55-3193-429f-9cf6-4df72dc029d4","resolution":{"observed_at":"2026-08-10T14:01:08.528590Z","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":"2026-08-10T14:01:08.532756Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.532756Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:99b68ee7973033191acb5b14dbd3df06fe1829ced8c0229578281a15261afef5","observation_id":"812d38eb-67bd-4f06-8e78-9cb5d15da588","resolution":{"observed_at":"2026-08-10T14:01:08.532756Z","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":"2026-08-10T14:01:08.536882Z","title":"It should be noted that the overall posterior is normalized, 1 = R P(ϑ)dN −2 ˆϑ dξPT d∆ε, so that the marginal one is also normalized, R P(ξPT, ∆ε) dξPT d∆ε","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.536882Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:0c8de02ebddb12f7cf3df432be8a6bb7d9ec5107d009f60c1014df8d980c0edb","observation_id":"da216733-cf62-4518-8298-51301a207e4c","resolution":{"observed_at":"2026-08-10T14:01:08.536882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.05145","last_updated":"2015-12-16T12:26:56Z","snapshot_observed_at":"2026-08-10T07:31:46.140889Z","submitted_at":"2015-12-16T12:26:56Z","title":"Introductory lectures on lattice QCD at nonzero baryon number","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.05145","snapshot_observed_at":"2026-08-10T14:01:08.541152Z","title":"Aarts, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.541152Z"},"links":{"cited_paper":"/paper/1512.05145","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:9dad0d4cdecf23978cf3410dfccb806e330f235d74001732168e0e0c59c47397","observation_id":"e22500dc-d474-41cf-b677-bc39367b3926","resolution":{"observed_at":"2026-08-10T14:01:08.541152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.0539","last_updated":"2010-06-01T14:39:07Z","snapshot_observed_at":"2026-08-08T14:53:38.265649Z","submitted_at":"2010-05-04T14:27:36Z","title":"Simulating QCD at finite density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.0539","snapshot_observed_at":"2026-08-10T14:01:08.545990Z","title":"de Forcrand, PoS LA T2009, 010 (2009), arXiv:1005.0539 [hep-lat]","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.545990Z"},"links":{"cited_paper":"/paper/1005.0539","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:0be3e42ec877b158c2096c99a1726f67f5bb6744b2ad79639fa0ff21b2c2b75e","observation_id":"070aeaf2-ffe5-4e3a-a9eb-75d97fd94a12","resolution":{"observed_at":"2026-08-10T14:01:08.545990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.08834","last_updated":"2020-10-17T17:52:19Z","snapshot_observed_at":"2026-08-10T22:10:12.325391Z","submitted_at":"2020-10-17T17:52:19Z","title":"Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.08834","snapshot_observed_at":"2026-08-10T14:01:08.550753Z","title":"Dexheimer, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.550753Z"},"links":{"cited_paper":"/paper/2010.08834","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:4ae90a5602b8141d54ae68bbfcff77237d73eecea7ffeab4129ebdfefe0bc625","observation_id":"388e69fc-b08a-4db2-ae41-0171aa6e8f0d","resolution":{"observed_at":"2026-08-10T14:01:08.550753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.03006","last_updated":"2020-09-07T10:45:54Z","snapshot_observed_at":"2026-08-04T09:17:56.519403Z","submitted_at":"2020-09-07T10:45:54Z","title":"Little-Bang and Femto-Nova in Nucleus-Nucleus Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.03006","snapshot_observed_at":"2026-08-10T14:01:08.555251Z","title":"Fukushima, B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.555251Z"},"links":{"cited_paper":"/paper/2009.03006","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:8171fc2327b0b25a32744c8a339da343a4f9d69a53260339b2f6d3ca8d87df03","observation_id":"9ca77ad8-702e-453b-971c-80aebd76f4ca","resolution":{"observed_at":"2026-08-10T14:01:08.555251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06980","last_updated":"2021-09-22T12:10:14Z","snapshot_observed_at":"2026-08-09T17:30:18.423607Z","submitted_at":"2021-05-14T17:33:33Z","title":"A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06980","snapshot_observed_at":"2026-08-10T14:01:08.603564Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.603564Z"},"links":{"cited_paper":"/paper/2105.06980","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:4c32a98ae2106c45065239aaee54f25fd635c37284fcc3910ed1ad33c7a27c30","observation_id":"ffc23014-6d92-42bd-9b57-2dc00ee4a7ca","resolution":{"observed_at":"2026-08-10T14:01:08.603564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.3510","last_updated":"2013-05-15T14:59:02Z","snapshot_observed_at":"2026-07-06T03:13:27.638618Z","submitted_at":"2013-05-15T14:59:02Z","title":"The Nuclear Equation of State and Neutron Star Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.3510","snapshot_observed_at":"2026-08-10T14:01:08.564475Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.564475Z"},"links":{"cited_paper":"/paper/1305.3510","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:f3e8cef951428decddfef997b3cd6d2dff2890375ae6133652a39c84e5b1a824","observation_id":"7e070d1c-5a66-466f-b177-fc66ceb39970","resolution":{"observed_at":"2026-08-10T14:01:08.564475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.04966","last_updated":"2017-12-17T00:07:47Z","snapshot_observed_at":"2026-08-07T05:50:14.787661Z","submitted_at":"2017-07-17T00:23:41Z","title":"From hadrons to quarks in neutron stars: a review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.04966","snapshot_observed_at":"2026-08-10T14:01:08.569604Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.569604Z"},"links":{"cited_paper":"/paper/1707.04966","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:01dca2b3a8ea1d241ab5bbd74a58a3661f57b844d88b44f2a2f33a8cb252b278","observation_id":"74fb2e2f-f171-4692-a017-faad72c47cd6","resolution":{"observed_at":"2026-08-10T14:01:08.569604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-07T22:20:24.299342Z","submitted_at":"2018-05-29T16:56:13Z","title":"GW170817: Measurements of Neutron Star Radii and Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11581","snapshot_observed_at":"2026-08-10T14:01:08.574130Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.574130Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:c495e6e898373aa147e17780abd02f0fe92c49647c7f585a90420419412c1fec","observation_id":"5d0c5076-94cc-4810-bc3a-f886b1c038a3","resolution":{"observed_at":"2026-08-10T14:01:08.574130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-10T14:01:08.578707Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.578707Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:e92d048ddab8fc385abada2a7eda07a9f31f57598e55fb1c2c68a376577d906a","observation_id":"e1d14656-3be6-4d2f-a013-bd3fbb0c02c4","resolution":{"observed_at":"2026-08-10T14:01:08.578707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01761","last_updated":"2020-04-07T09:39:44Z","snapshot_observed_at":"2026-08-10T13:59:44.754944Z","submitted_at":"2020-01-06T19:54:55Z","title":"GW190425: Observation of a Compact Binary Coalescence with Total Mass $\\sim 3.4 M_{\\odot}$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.01761","snapshot_observed_at":"2026-08-10T14:01:08.583457Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.583457Z"},"links":{"cited_paper":"/paper/2001.01761","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:c5cdae2839b50265cabfb7d8707b787a2d3277db754b9413e41c8f06156134e5","observation_id":"95f4c98b-d67e-4db9-a39a-44da67ce1de1","resolution":{"observed_at":"2026-08-10T14:01:08.583457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.12611","last_updated":"2020-06-22T20:56:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-06-22T20:56:34Z","title":"GW190814: Gravitational Waves from the Coalescence of a 23 M$_\\odot$ Black Hole with a 2.6 M$_\\odot$ Compact Object","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.12611","snapshot_observed_at":"2026-08-10T14:01:08.587921Z","title":"Abbott et al.(LIGO Scientific, Virgo), Astrophys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.587921Z"},"links":{"cited_paper":"/paper/2006.12611","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:0fdcd0ca9f95d278686f2d5217323db685c61f61034e04e3d6b8fff20a1a5794","observation_id":"b4ef4aba-ae65-4c42-b2cf-514002cd2dcb","resolution":{"observed_at":"2026-08-10T14:01:08.587921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05705","last_updated":"2019-12-12T00:04:41Z","snapshot_observed_at":"2026-07-31T21:20:48.579404Z","submitted_at":"2019-12-12T00:04:41Z","title":"PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05705","snapshot_observed_at":"2026-08-10T14:01:08.593344Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.593344Z"},"links":{"cited_paper":"/paper/1912.05705","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:e2a1f487840b213954edcf7d5d3042f2b8e32f5c292ab9461cba69cdcc360a71","observation_id":"e4b00419-04a1-439c-9d8c-d0caa6860710","resolution":{"observed_at":"2026-08-10T14:01:08.593344Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05702","last_updated":"2019-12-12T00:04:38Z","snapshot_observed_at":"2026-08-10T10:33:26.457624Z","submitted_at":"2019-12-12T00:04:38Z","title":"A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05702","snapshot_observed_at":"2026-08-10T14:01:08.598485Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.598485Z"},"links":{"cited_paper":"/paper/1912.05702","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:472680103ad01609cd75c655edcd9150cab743d39847cd6f80ecb34ce0f15a29","observation_id":"9d5cd7c7-8f8a-4a9a-93de-96fddec78af2","resolution":{"observed_at":"2026-08-10T14:01:08.598485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14645","last_updated":"2025-04-14T05:43:34Z","snapshot_observed_at":"2026-08-11T12:00:54.527779Z","submitted_at":"2024-12-19T08:54:23Z","title":"Correlations between the Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.14645","snapshot_observed_at":"2026-08-10T14:01:08.644211Z","title":"Sun and J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.644211Z"},"links":{"cited_paper":"/paper/2412.14645","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:147b04223e3f02ca185b6a57816c4aa1a882a2f3a1363ea03369386cdc776a9c","observation_id":"d1813951-e600-4ae9-8507-2be625ce315d","resolution":{"observed_at":"2026-08-10T14:01:08.644211Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06979","last_updated":"2021-05-14T17:33:32Z","snapshot_observed_at":"2026-08-08T20:42:33.884209Z","submitted_at":"2021-05-14T17:33:32Z","title":"The Radius of PSR J0740+6620 from NICER and XMM-Newton Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06979","snapshot_observed_at":"2026-08-10T14:01:08.608052Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.608052Z"},"links":{"cited_paper":"/paper/2105.06979","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:f9e6c4c614a512e14c81835a9e9cd04a9598276d1dbd924a26ee5965b87870f9","observation_id":"c505077b-ac71-4beb-947b-f73b4676158e","resolution":{"observed_at":"2026-08-10T14:01:08.608052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.04434","last_updated":"2015-10-15T08:00:01Z","snapshot_observed_at":"2026-07-06T04:33:10.141578Z","submitted_at":"2015-10-15T08:00:01Z","title":"Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.04434","snapshot_observed_at":"2026-08-10T14:01:08.612641Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.612641Z"},"links":{"cited_paper":"/paper/1510.04434","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:40c7f5f35cc86b4e513dfa1a28d0bf12c7608b20122b3186338e56206bf5c922","observation_id":"7bc1bba6-ad16-4404-9bcb-16e46d1dcec5","resolution":{"observed_at":"2026-08-10T14:01:08.612641Z","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":"2026-08-10T14:01:08.507015Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.507015Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:29c8eefe9539f155fb2899541ec1bb52e7199bde2d09ac6e0b363c7c16ab7f1a","observation_id":"da2ee11d-e3ad-4f7f-ada2-9457baaf1b46","resolution":{"observed_at":"2026-08-10T14:01:08.507015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04117","last_updated":"2022-02-08T19:40:20Z","snapshot_observed_at":"2026-08-11T08:56:40.228198Z","submitted_at":"2022-02-08T19:40:20Z","title":"Gravitational-Wave and X-ray Probes of the Neutron Star Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04117","snapshot_observed_at":"2026-08-10T14:01:08.617056Z","title":"Yunes, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.617056Z"},"links":{"cited_paper":"/paper/2202.04117","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:e99c9cd33e452dc808573c4b736e65dc08d9c1dbb860d474d22b9ec33562c6b3","observation_id":"e3ae7813-1419-4d46-b854-14029f9f6252","resolution":{"observed_at":"2026-08-10T14:01:08.617056Z","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":"2026-08-10T14:01:08.621669Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.621669Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:134938d4a12aa8c53583f5253c369974309551d03353c8f3db1935a46bb6f8a4","observation_id":"32993db4-c190-421f-95cd-78917f3aa2d4","resolution":{"observed_at":"2026-08-10T14:01:08.621669Z","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":"2026-08-10T14:01:08.626528Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.626528Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:bb17f6acf4685919dc7936bb26350e8007fc884db998b43bb3bf3d14f307dfc1","observation_id":"ea36b99e-6907-4f43-b479-dc3865b57593","resolution":{"observed_at":"2026-08-10T14:01:08.626528Z","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":"2026-08-10T14:01:08.630707Z","title":"Lindblom, Astrophys","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.630707Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:9bba57f33fb7b29e6f4ac0ea047fefdc66d7ef552c2c55988956210793135762","observation_id":"03848d54-bfb5-44cb-9605-0e749a6d38b9","resolution":{"observed_at":"2026-08-10T14:01:08.630707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16847","last_updated":"2024-02-26T14:20:21Z","snapshot_observed_at":"2026-07-06T16:38:29.188225Z","submitted_at":"2023-10-23T03:23:07Z","title":"Maximal Mass Neutron Star as a Key to Superdense Matter Physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16847","snapshot_observed_at":"2026-08-10T14:01:08.634642Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.634642Z"},"links":{"cited_paper":"/paper/2310.16847","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:fc88b527d0e99d9d22f1bfd273d1b8ba88c8c2934a78c73edaa566949010e36c","observation_id":"086f5b44-344d-4ac8-8089-2228e65e1711","resolution":{"observed_at":"2026-08-10T14:01:08.634642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00843","last_updated":"2024-05-04T04:45:25Z","snapshot_observed_at":"2026-08-03T14:22:02.388362Z","submitted_at":"2023-11-01T20:47:48Z","title":"Compiled Properties of Nucleonic Matter and Nuclear and Neutron Star Models from Non-Relativistic and Relativistic Interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00843","snapshot_observed_at":"2026-08-10T14:01:08.639671Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.639671Z"},"links":{"cited_paper":"/paper/2311.00843","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:771eed37b5aed13f0130362bb5f8dc3ba2f87b4d6f52f8a7b2d8244a8a997574","observation_id":"93eee501-26a9-4312-acb9-13c7aa7def74","resolution":{"observed_at":"2026-08-10T14:01:08.639671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.08885","last_updated":"2021-02-12T15:35:51Z","snapshot_observed_at":"2026-08-10T08:43:45.291453Z","submitted_at":"2020-09-18T15:20:05Z","title":"New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.08885","snapshot_observed_at":"2026-08-10T14:01:08.648659Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.648659Z"},"links":{"cited_paper":"/paper/2009.08885","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:f8e4f841aab2dde03c6129a35d8f1f825afcc789d86267ea51253a6e11608cf4","observation_id":"9f70be78-6a00-4376-ae8f-2d2c55c7ae07","resolution":{"observed_at":"2026-08-10T14:01:08.648659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06229","last_updated":"2022-06-24T14:44:52Z","snapshot_observed_at":"2026-08-06T00:47:36.743643Z","submitted_at":"2021-07-13T16:31:44Z","title":"Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06229","snapshot_observed_at":"2026-08-10T14:01:08.653054Z","title":"Huth et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.653054Z"},"links":{"cited_paper":"/paper/2107.06229","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:812c88c31c86a1c1d85fcf19f0c6f923896c20105355ab15cc56df1057596f08","observation_id":"b06c62a2-6192-498b-b04d-c7d3f77a3ba8","resolution":{"observed_at":"2026-08-10T14:01:08.653054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","snapshot_observed_at":"2026-07-06T11:10:37.017160Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08688","snapshot_observed_at":"2026-08-10T14:01:08.658261Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.658261Z"},"links":{"cited_paper":"/paper/2105.08688","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:965968ba60d833e1222bb31b9b902d7da90ec32a80a2bafe89d9c4e7e3c393c5","observation_id":"5fed7279-2d06-4adf-92b4-7a80e34fb192","resolution":{"observed_at":"2026-08-10T14:01:08.658261Z","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":"2026-08-10T14:01:08.663439Z","title":"Chatziioannou, H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.663439Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:f61d177dd0e794f232fbb9be24c358dcb52326ed2b11fc29ffa9ea625d06f3cf","observation_id":"023d1bc1-b293-47e2-948d-762290885260","resolution":{"observed_at":"2026-08-10T14:01:08.663439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.12817","last_updated":"2020-11-17T05:21:41Z","snapshot_observed_at":"2026-08-11T19:09:18.274036Z","submitted_at":"2020-08-28T19:06:33Z","title":"Combining Electromagnetic and Gravitational-Wave Constraints on Neutron-Star Masses and Radii","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.12817","snapshot_observed_at":"2026-08-10T14:01:08.668525Z","title":"Al-Mamun, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.668525Z"},"links":{"cited_paper":"/paper/2008.12817","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:50407301d3b63ed8e85760c08419738f075cc3ce8a599ac14f769915539f233f","observation_id":"8c1b1637-6f0c-4252-9430-03458e34a79b","resolution":{"observed_at":"2026-08-10T14:01:08.668525Z","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":"2026-08-10T14:01:08.672775Z","title":"Baym and C","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.672775Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:27b45fc948fa4ac0d21dc167573d9d92a2227e0ce0bd9876d90a3b2ff8629017","observation_id":"738e67b6-b33c-4ddc-b732-4a2cf90f5494","resolution":{"observed_at":"2026-08-10T14:01:08.672775Z","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":"2026-08-10T14:01:08.676969Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.676969Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:683010e0be9d817a68f967af2a1aecb94eb1f16fc672e93b214276b8c2d724b3","observation_id":"7eb3ca90-a6a6-48c0-bcc8-f8fe3353879e","resolution":{"observed_at":"2026-08-10T14:01:08.676969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111092","last_updated":"2001-11-12T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2001-11-05T17:05:33Z","title":"A unified equation of state of dense matter and neutron star structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111092","snapshot_observed_at":"2026-08-10T14:01:08.681979Z","title":"Douchin and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.681979Z"},"links":{"cited_paper":"/paper/astro-ph/0111092","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:00ee25875e8bb04f8cce844d1c6e3cab0a63ec6b85de4ef4520dab28439f5a8e","observation_id":"a79ec1d5-5ec0-4f70-a38a-50eee81c1261","resolution":{"observed_at":"2026-08-10T14:01:08.681979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.3791","last_updated":"2008-01-24T16:17:09Z","snapshot_observed_at":"2026-07-06T01:34:45.604137Z","submitted_at":"2008-01-24T16:17:09Z","title":"Hypernuclear Physics for Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.3791","snapshot_observed_at":"2026-08-10T14:01:08.686474Z","title":"Schaffner-Bielich, Nucl","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.686474Z"},"links":{"cited_paper":"/paper/0801.3791","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:d99c44a97a58b9173fdc6ebbcc81055d00ff50027900c194a6761c6b088b442b","observation_id":"a6bfcae7-8ab3-41f6-98bd-4f1ce12edf04","resolution":{"observed_at":"2026-08-10T14:01:08.686474Z","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":"2026-08-10T14:01:08.690932Z","title":"Vida˜ na, Nucl","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.690932Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:83f42cea97f23c0174c807a0f784656d7e4ef46747c559eb6f64d45724f7ec16","observation_id":"ddc71fe8-d3b1-491f-a6eb-181c19649547","resolution":{"observed_at":"2026-08-10T14:01:08.690932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005490","last_updated":"2002-09-19T21:10:48Z","snapshot_observed_at":"2026-08-10T10:14:01.862496Z","submitted_at":"2000-05-24T17:24:54Z","title":"Phase Transition to Hyperon Matter in Neutron Stars","version":3},"cited_work":{"arxiv_id":"astro-ph/0005490","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0005490","snapshot_observed_at":"2026-08-10T14:01:10.024451Z","title":"Phase Transition to Hyperon Matter in Neutron Stars","venue":"astro-ph","work_id":"ce985d42-2994-4e5b-a95c-7352d8cc81b6","year":2000},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.694862Z"},"links":{"cited_paper":"/paper/astro-ph/0005490","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:1adc0e040b9bd3ac1d4fc322ef3f1bb7a85b01feb828e9c87d80824c3f95892b","observation_id":"0786cbdc-455e-4d06-bd60-6a1c0d02b3a2","resolution":{"observed_at":"2026-08-10T14:01:10.029328Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-lat/0701002","last_updated":"2006-12-31T23:10:55Z","snapshot_observed_at":"2026-07-07T03:43:43.283130Z","submitted_at":"2006-12-31T23:10:55Z","title":"QCD phase diagram: an overview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-lat/0701002","snapshot_observed_at":"2026-08-10T14:01:08.699279Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.699279Z"},"links":{"cited_paper":"/paper/hep-lat/0701002","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:d728c866d76c93b5bc0891eea2ff0736f69a5ae2e20973408d3f2d09e4a09401","observation_id":"933d2397-ed0c-4c80-984d-b9e910113635","resolution":{"observed_at":"2026-08-10T14:01:08.699279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.09121","last_updated":"2021-07-27T11:45:07Z","snapshot_observed_at":"2026-08-09T14:31:41.802114Z","submitted_at":"2019-03-21T17:30:37Z","title":"Evidence for quark-matter cores in massive neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.09121","snapshot_observed_at":"2026-08-10T14:01:08.703576Z","title":"Annala, T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.703576Z"},"links":{"cited_paper":"/paper/1903.09121","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:1eb0e3b11446caf2f85e6861d124333d968309072bb5f191141163741b7dea22","observation_id":"3516d2ab-8445-45e4-b5fe-c33aa9d7cf87","resolution":{"observed_at":"2026-08-10T14:01:08.703576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.00936","last_updated":"2020-04-16T15:47:10Z","snapshot_observed_at":"2026-07-30T16:44:03.301968Z","submitted_at":"2019-06-03T17:29:52Z","title":"Mapping the Phases of Quantum Chromodynamics with Beam Energy Scan","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.00936","snapshot_observed_at":"2026-08-10T14:01:08.720033Z","title":"Bzdak, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.720033Z"},"links":{"cited_paper":"/paper/1906.00936","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:47fd1b10fc2494b91ef7c7e7e2c0e6e9913d834cb09a3812ac5165ba21e635e2","observation_id":"1b100a4d-5467-43cf-b693-16f9ff25f83d","resolution":{"observed_at":"2026-08-10T14:01:08.720033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.11356","last_updated":"2024-01-12T08:46:31Z","snapshot_observed_at":"2026-08-11T01:55:00.194030Z","submitted_at":"2023-03-20T18:00:04Z","title":"Strongly interacting matter exhibits deconfined behavior in massive neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.11356","snapshot_observed_at":"2026-08-10T14:01:08.726043Z","title":"Annala, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.726043Z"},"links":{"cited_paper":"/paper/2303.11356","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:e0c92208cb99d127e15e685b80ef9c57fd2e3c7856a14e7a8d1b8e4acb501195","observation_id":"d21bd702-83a3-49f3-9419-f912dd4b3fcb","resolution":{"observed_at":"2026-08-10T14:01:08.726043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07411","last_updated":"2023-06-08T13:17:42Z","snapshot_observed_at":"2026-07-06T15:26:27.123805Z","submitted_at":"2023-05-12T12:27:24Z","title":"Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.07411","snapshot_observed_at":"2026-08-10T14:01:08.732181Z","title":"Essick, I","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.732181Z"},"links":{"cited_paper":"/paper/2305.07411","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:5e2ef366a1eb211664a25763b20c58b42559659f1687a174dec464a1dfb29520","observation_id":"94e8f598-4a07-4062-a754-f6eb6ee13a1d","resolution":{"observed_at":"2026-08-10T14:01:08.732181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.01619","last_updated":"2024-09-23T02:04:01Z","snapshot_observed_at":"2026-08-05T07:32:00.996875Z","submitted_at":"2023-10-02T20:28:12Z","title":"Indication of Sharp and Strong Phase-Transitions from NICER Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.01619","snapshot_observed_at":"2026-08-10T14:01:08.737577Z","title":"Lin and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.737577Z"},"links":{"cited_paper":"/paper/2310.01619","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:40905bfa3c004a2ac21441ae413712ad50f671b868a1ec8a2e9654571a36a50c","observation_id":"58e825a6-c8b7-4417-bd30-9b41f4fcf474","resolution":{"observed_at":"2026-08-10T14:01:08.737577Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.01756","last_updated":"2022-09-02T11:26:41Z","snapshot_observed_at":"2026-08-07T03:42:44.264174Z","submitted_at":"2022-01-05T18:40:42Z","title":"Neural network reconstruction of the dense matter equation of state from neutron star observables","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.01756","snapshot_observed_at":"2026-08-10T14:01:08.743345Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.743345Z"},"links":{"cited_paper":"/paper/2201.01756","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:4d31c78a6677eec673ada21ddafccb13a96b7755e6e41be11973331054f2dee9","observation_id":"f00afc0b-d033-43e7-8a8f-5b275a5f4b9b","resolution":{"observed_at":"2026-08-10T14:01:08.743345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.08883","last_updated":"2022-12-22T15:41:47Z","snapshot_observed_at":"2026-08-04T01:49:12.243924Z","submitted_at":"2022-09-19T09:38:33Z","title":"Reconstructing the neutron star equation of state from observational data via automatic differentiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.08883","snapshot_observed_at":"2026-08-10T14:01:08.750066Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.750066Z"},"links":{"cited_paper":"/paper/2209.08883","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:383def0b0f983f5c9a1b53657b86b8077e40e91db16d653e1eebe7e12a2ff328","observation_id":"78b346f3-3752-4144-84b3-a03d6054448d","resolution":{"observed_at":"2026-08-10T14:01:08.750066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.05408","last_updated":"2019-01-16T17:46:36Z","snapshot_observed_at":"2026-08-09T19:43:56.397674Z","submitted_at":"2019-01-16T17:46:36Z","title":"Reconstructing parton distribution functions from Ioffe time data: from Bayesian methods to Neural Networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.05408","snapshot_observed_at":"2026-08-10T14:01:08.756028Z","title":"Karpie, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.756028Z"},"links":{"cited_paper":"/paper/1901.05408","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:107deeeb6a2a5cd9d1823e5de97cf54a64bebd9c790b78ea2edab0f31462a486","observation_id":"75a1a466-5fe1-4aa2-824c-a9202493bace","resolution":{"observed_at":"2026-08-10T14:01:08.756028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.02671","last_updated":"2021-09-06T18:00:06Z","snapshot_observed_at":"2026-08-11T10:56:25.567053Z","submitted_at":"2021-09-06T18:00:06Z","title":"An open-source machine learning framework for global analyses of parton distributions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.02671","snapshot_observed_at":"2026-08-10T14:01:08.761977Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.761977Z"},"links":{"cited_paper":"/paper/2109.02671","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:2e6d88195365e94a307f81f9212dfbe0dea1e985fa260dfc5a745af9293f39b1","observation_id":"8c352e64-25f2-40b9-9dcb-275f68a56f5e","resolution":{"observed_at":"2026-08-10T14:01:08.761977Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.02297","last_updated":"2022-12-28T03:30:06Z","snapshot_observed_at":"2026-08-09T04:53:41.234814Z","submitted_at":"2022-08-03T18:28:48Z","title":"Continuum-extrapolated NNLO Valence PDF of Pion at the Physical Point","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.02297","snapshot_observed_at":"2026-08-10T14:01:08.767215Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.767215Z"},"links":{"cited_paper":"/paper/2208.02297","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:6d817d73793c3313b66c0b6b2a4c90c7fc6de560bd012746c17e94e024166e7f","observation_id":"6bbc58fe-f1ac-4832-a210-96de3165d10a","resolution":{"observed_at":"2026-08-10T14:01:08.767215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.07862","last_updated":"2022-01-14T18:36:17Z","snapshot_observed_at":"2026-08-10T20:19:01.193868Z","submitted_at":"2021-05-17T14:00:35Z","title":"Heavy quark potential in quark-gluon Plasma: Deep neural network meets lattice quantum chromodynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.07862","snapshot_observed_at":"2026-08-10T14:01:08.773325Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.773325Z"},"links":{"cited_paper":"/paper/2105.07862","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:e1bd9af4b4dd9dd009304f6f3b4bc10c95567dc21c71ab5b4a17497ef5021907","observation_id":"f21e40e3-d1d1-4c2f-9b9e-6c3cd57c9212","resolution":{"observed_at":"2026-08-10T14:01:08.773325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14760","last_updated":"2022-09-20T18:59:18Z","snapshot_observed_at":"2026-08-10T06:27:24.779424Z","submitted_at":"2021-11-29T18:09:49Z","title":"Reconstructing spectral functions via automatic differentiation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.14760","snapshot_observed_at":"2026-08-10T14:01:08.779356Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.779356Z"},"links":{"cited_paper":"/paper/2111.14760","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:3551119e9e637e6faaf12bb054a279b5efc4d5002e3342a91eaf3ead3e038674","observation_id":"e556db8c-1ff1-43ef-b6be-ffe25e227803","resolution":{"observed_at":"2026-08-10T14:01:08.779356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02564","last_updated":"2022-09-20T15:51:32Z","snapshot_observed_at":"2026-07-06T12:25:30.741916Z","submitted_at":"2022-01-07T17:48:49Z","title":"Rethinking the ill-posedness of the spectral function reconstruction -- why is it fundamentally hard and how Artificial Neural Networks can help","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.02564","snapshot_observed_at":"2026-08-10T14:01:08.784703Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.784703Z"},"links":{"cited_paper":"/paper/2201.02564","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:784ea558147d27ddc09ccaddff14d09231e4ac745b878532a126be7162e61de6","observation_id":"d618992a-b70e-4d64-9b0f-ba3757ea7e26","resolution":{"observed_at":"2026-08-10T14:01:08.784703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07994","last_updated":"2022-11-15T09:03:21Z","snapshot_observed_at":"2026-08-10T20:17:46.597309Z","submitted_at":"2022-11-15T09:03:21Z","title":"Deep-learning quasi-particle masses from QCD equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07994","snapshot_observed_at":"2026-08-10T14:01:08.791337Z","title":"Li, H.-L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.791337Z"},"links":{"cited_paper":"/paper/2211.07994","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:6f68197f81d27f9457906bb9a105396b4d82a6bb0d9082625ad1f355a48f79c7","observation_id":"f5d7adc8-d158-4bf9-8e87-a72337b74fa1","resolution":{"observed_at":"2026-08-10T14:01:08.791337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.10012","last_updated":"2025-01-17T07:48:42Z","snapshot_observed_at":"2026-08-10T19:21:37.402979Z","submitted_at":"2025-01-17T07:48:42Z","title":"Nuclear equation of state at finite $\\mu_B$ using deep learning assisted quasi-parton model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.10012","snapshot_observed_at":"2026-08-10T14:01:08.796833Z","title":"Li, L.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.796833Z"},"links":{"cited_paper":"/paper/2501.10012","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:792e9542c471d4d44ee9bc1164bf1a341d5c0b454e00dc931e216e5c9b13011b","observation_id":"5c2df666-25e2-4371-98c7-85194405540e","resolution":{"observed_at":"2026-08-10T14:01:08.796833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.03784","last_updated":"2024-12-03T09:29:36Z","snapshot_observed_at":"2026-08-10T13:03:19.799079Z","submitted_at":"2024-08-07T14:09:25Z","title":"Neural Network Modeling of Heavy-Quark Potential from Holography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.03784","snapshot_observed_at":"2026-08-10T14:01:08.802513Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.802513Z"},"links":{"cited_paper":"/paper/2408.03784","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:337f9825fd3e2d3ea3c0d7fa0b1fe1ce5bad2fae1d00ed7374ae9b6ea5e1a88a","observation_id":"96c1e11c-a681-41ea-8cfb-40afbc081bc9","resolution":{"observed_at":"2026-08-10T14:01:08.802513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.03082","last_updated":"2024-10-04T02:05:32Z","snapshot_observed_at":"2026-08-09T20:10:57.434467Z","submitted_at":"2024-10-04T02:05:32Z","title":"Building Hadron Potentials from Lattice QCD with Deep Neural Networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.03082","snapshot_observed_at":"2026-08-10T14:01:08.807964Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.807964Z"},"links":{"cited_paper":"/paper/2410.03082","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:313efb491ed3db3d5578434e18bc2f993ff0b49175f4b0bb2f7f575ea4d3c10d","observation_id":"34cfb874-4ab9-4be9-b0f3-69fc1b9b9287","resolution":{"observed_at":"2026-08-10T14:01:08.807964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.00374","last_updated":"2024-12-31T09:55:21Z","snapshot_observed_at":"2026-08-10T22:50:26.289188Z","submitted_at":"2024-12-31T09:55:21Z","title":"Deep learning for exploring hadron-hadron interactions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.00374","snapshot_observed_at":"2026-08-10T14:01:08.814028Z","title":"Wang (2024) arXiv:2501.00374 [nucl-th]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.814028Z"},"links":{"cited_paper":"/paper/2501.00374","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:cfd12e21d29a97e306b5328dc08197bbeea3cf1fb40fff1a8ba965d3f9e9f9b3","observation_id":"273be7ff-b606-4394-8dc8-213f7849726a","resolution":{"observed_at":"2026-08-10T14:01:08.814028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.16343","last_updated":"2025-01-07T21:16:35Z","snapshot_observed_at":"2026-08-09T19:01:20.132247Z","submitted_at":"2024-11-25T12:43:22Z","title":"Learning Hadron Emitting Sources with Deep Neural Networks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.16343","snapshot_observed_at":"2026-08-10T14:01:08.820309Z","title":"Wang and J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.820309Z"},"links":{"cited_paper":"/paper/2411.16343","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:6fcf4393762fc66df4e09f0b7a695556e23b59dd164542e02b5088ce0d843fa5","observation_id":"1e5edac0-a93d-49b8-a355-0236d645775f","resolution":{"observed_at":"2026-08-10T14:01:08.820309Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15136","last_updated":"2023-12-01T23:47:32Z","snapshot_observed_at":"2026-08-10T20:17:03.031865Z","submitted_at":"2023-03-27T12:10:42Z","title":"Exploring QCD matter in extreme conditions with Machine Learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15136","snapshot_observed_at":"2026-08-10T14:01:08.826289Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.826289Z"},"links":{"cited_paper":"/paper/2303.15136","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:3990f9a8e9cb583243ae578d25584edffc85e0deedd5e0160a65fa0aca338d70","observation_id":"e847c34c-5d65-4889-ad7e-753e89544d78","resolution":{"observed_at":"2026-08-10T14:01:08.826289Z","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":"2026-08-10T14:01:08.831757Z","title":"Aarts, K","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.831757Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:caecbbf46974641a5cb50e8f9e24245798e7a2c3ade51b3c05c3d38db1291a82","observation_id":"5683db42-87e6-4335-9806-fba13411c777","resolution":{"observed_at":"2026-08-10T14:01:08.831757Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-10T14:01:08.836838Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.836838Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:8b25c0ab76d5b2fe652ab9555f72e73152856979c032964479cab2ee7c4c4047","observation_id":"56531664-c620-41f4-b6b6-7fcbae87e4e9","resolution":{"observed_at":"2026-08-10T14:01:08.836838Z","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":"2026-08-10T14:01:08.842991Z","title":"¨Ozel and P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.842991Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:82b64d5b0948771e0817b479ea3ae7fbff5d27b2d6f14fbcc9e28262bb8fefd8","observation_id":"74068eba-43a3-487e-a67e-d29e815eb90b","resolution":{"observed_at":"2026-08-10T14:01:08.842991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.03954","last_updated":"2016-08-19T17:41:49Z","snapshot_observed_at":"2026-08-03T18:29:21.691415Z","submitted_at":"2016-05-12T19:55:33Z","title":"Applying Bayesian parameter estimation to relativistic heavy-ion collisions: simultaneous characterization of the initial state and quark-gluon plasma medium","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.03954","snapshot_observed_at":"2026-08-10T14:01:08.848097Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.848097Z"},"links":{"cited_paper":"/paper/1605.03954","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:7334578ba5c599c10b9c73f2087ba0c9e2a6b5f4b190bd34344f5a78a2f6a2ca","observation_id":"c5a4cccf-97e6-4fd2-a3ed-b042d88954f1","resolution":{"observed_at":"2026-08-10T14:01:08.848097Z","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":"2026-08-10T14:01:08.853552Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.853552Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:fa9b9abb5ae5842136bcabd507f6a0d4c7b28826e3a84cfe9c3e10f17d83e4a8","observation_id":"cd9ff43d-669c-4fe0-a3c7-199bd2593357","resolution":{"observed_at":"2026-08-10T14:01:08.853552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.03928","last_updated":"2020-10-08T12:26:16Z","snapshot_observed_at":"2026-08-11T03:25:04.209512Z","submitted_at":"2020-10-08T12:26:16Z","title":"Phenomenological constraints on the transport properties of QCD matter with data-driven model averaging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.03928","snapshot_observed_at":"2026-08-10T14:01:08.858461Z","title":"Everett et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.858461Z"},"links":{"cited_paper":"/paper/2010.03928","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:045b94a79cc64911057de420f2ababfdabd71e7057fb84cec9afab296697e3e2","observation_id":"7f583fa7-2717-4d46-bdcf-7bd6aa323c09","resolution":{"observed_at":"2026-08-10T14:01:08.858461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01430","last_updated":"2020-11-06T20:33:35Z","snapshot_observed_at":"2026-07-06T10:11:08.648093Z","submitted_at":"2020-11-03T02:32:56Z","title":"Multi-system Bayesian constraints on the transport coefficients of QCD matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01430","snapshot_observed_at":"2026-08-10T14:01:08.864305Z","title":"Everett et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.864305Z"},"links":{"cited_paper":"/paper/2011.01430","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:531fb20674fc3fce6409962e8099c88cfe74e614fcf280808414f5242a36f911","observation_id":"699a8a06-2ec9-4d02-ac58-0720394bbae7","resolution":{"observed_at":"2026-08-10T14:01:08.864305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.11337","last_updated":"2021-07-29T00:49:53Z","snapshot_observed_at":"2026-08-09T07:54:28.754473Z","submitted_at":"2021-02-22T20:12:48Z","title":"Determining the jet transport coefficient $\\hat{q}$ from inclusive hadron suppression measurements using Bayesian parameter estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.11337","snapshot_observed_at":"2026-08-10T14:01:08.869016Z","title":"Cao et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.869016Z"},"links":{"cited_paper":"/paper/2102.11337","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:a9cf00763d24e3f676eff698f5996d1dafa4febb53c60f01255a1605a3d3ed34","observation_id":"c03d5e79-7b77-4cba-97df-5510ccb5caaf","resolution":{"observed_at":"2026-08-10T14:01:08.869016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.09619","last_updated":"2023-07-01T00:47:42Z","snapshot_observed_at":"2026-08-11T03:25:32.233242Z","submitted_at":"2023-06-16T04:22:57Z","title":"Early-times Yang-Mills dynamics and the characterization of strongly interacting matter with statistical learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.09619","snapshot_observed_at":"2026-08-10T14:01:08.874971Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.874971Z"},"links":{"cited_paper":"/paper/2306.09619","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:9f3ccfbc6473103c29532d6d2e6800474c5bb0cc839f0e7ec312610185c7339a","observation_id":"dfdf0b7e-b322-43ef-b979-e7a67798ce2b","resolution":{"observed_at":"2026-08-10T14:01:08.874971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09478","last_updated":"2024-05-27T21:27:18Z","snapshot_observed_at":"2026-08-03T15:47:35.229692Z","submitted_at":"2023-02-19T04:47:57Z","title":"Bayesian quantification of strongly-interacting matter with color glass condensate initial conditions","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09478","snapshot_observed_at":"2026-08-10T14:01:08.879678Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.879678Z"},"links":{"cited_paper":"/paper/2302.09478","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:152a2ed80b9346a06b15e2135d6f77a216a55e9d71f8ddb68c121aebed83a4cc","observation_id":"74d9b03b-d1f6-4127-87a4-64141dd47ef6","resolution":{"observed_at":"2026-08-10T14:01:08.879678Z","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":"2026-08-10T14:01:08.885095Z","title":"Andrieu, N","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.885095Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:42301b333c3b070657386f375a7c44afb3de0787b5c008ae4f94c56412115cef","observation_id":"734192d4-7525-4c7f-bf04-ad9947350ae1","resolution":{"observed_at":"2026-08-10T14:01:08.885095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.1268","last_updated":"2009-01-09T16:33:52Z","snapshot_observed_at":"2026-07-06T01:49:42.552755Z","submitted_at":"2009-01-09T16:33:52Z","title":"Keplerian frequency of uniformly rotating neutron stars and quark stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.1268","snapshot_observed_at":"2026-08-10T14:01:08.890253Z","title":"Haensel, J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.890253Z"},"links":{"cited_paper":"/paper/0901.1268","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:57f56022c39a7e9ff50d6feb5ceef4272773304579159cdcd4cf525d6e64a277","observation_id":"f7ec54c7-d217-490e-b7a6-bf86174fb369","resolution":{"observed_at":"2026-08-10T14:01:08.890253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05368","last_updated":"2016-03-29T12:54:07Z","snapshot_observed_at":"2026-07-06T04:43:30.139132Z","submitted_at":"2016-01-20T18:38:44Z","title":"Rotating neutron stars with exotic cores: masses, radii, stability","version":2},"cited_work":{"arxiv_id":"1601.05368","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05368","snapshot_observed_at":"2026-08-10T14:01:09.623127Z","title":"Rotating neutron stars with exotic cores: masses, radii, stability","venue":"astro-ph.HE","work_id":"75bbe792-3205-41c3-900d-f2f879eecba3","year":2016},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.895737Z"},"links":{"cited_paper":"/paper/1601.05368","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:a75e28e9d366b743a1ae0268de554dff434a0c467f41fda008b24bd6f9a7badf","observation_id":"a60ac8d3-b38f-47d2-ba2d-dec5771a07a7","resolution":{"observed_at":"2026-08-10T14:01:09.628234Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.09759","last_updated":"2020-05-19T21:16:40Z","snapshot_observed_at":"2026-07-06T09:21:47.619259Z","submitted_at":"2020-05-19T21:16:40Z","title":"Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination","version":1},"cited_work":{"arxiv_id":"2005.09759","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.09759","snapshot_observed_at":"2026-08-10T14:01:09.602851Z","title":"Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination","venue":"astro-ph.HE","work_id":"773e9bc3-0bec-47f1-947a-a500ff76129e","year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.901035Z"},"links":{"cited_paper":"/paper/2005.09759","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:f87572e32ec2e2de833cba6f8aa09ee4a95bd74848be722c19fc7a670c5fd360","observation_id":"e4737bfb-71db-4ee7-a6e1-d9dd0d41d0af","resolution":{"observed_at":"2026-08-10T14:01:09.607809Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.02106","last_updated":"2022-10-26T15:54:46Z","snapshot_observed_at":"2026-08-11T01:51:56.722372Z","submitted_at":"2022-06-05T06:39:56Z","title":"Do we need dense matter equation of state in curved spacetime for neutron stars?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.02106","snapshot_observed_at":"2026-08-10T14:01:08.906947Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.906947Z"},"links":{"cited_paper":"/paper/2206.02106","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:7fe36db82cec2b3d53ecadeb607eb5cfcd9f778f94a5599360618955633a4b3c","observation_id":"87428b75-93fe-406f-9768-174b2a5ca99f","resolution":{"observed_at":"2026-08-10T14:01:08.906947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1915","last_updated":"2007-12-07T21:22:23Z","snapshot_observed_at":"2026-07-06T01:33:47.610408Z","submitted_at":"2007-09-12T15:46:16Z","title":"Constraining neutron star tidal Love numbers with gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.1915","snapshot_observed_at":"2026-08-10T14:01:08.912252Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.912252Z"},"links":{"cited_paper":"/paper/0709.1915","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:0b7c6e71459b68016e66765b8d3fa963ac4b0461291a9fd71627e5957ee5b0a4","observation_id":"d9762ba1-a718-413f-a04a-74634b8f3f38","resolution":{"observed_at":"2026-08-10T14:01:08.912252Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.0096","last_updated":"2009-12-03T14:45:12Z","snapshot_observed_at":"2026-08-05T01:49:37.499461Z","submitted_at":"2009-05-30T17:22:37Z","title":"Relativistic tidal properties of neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.0096","snapshot_observed_at":"2026-08-10T14:01:08.916797Z","title":"Damour and A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.916797Z"},"links":{"cited_paper":"/paper/0906.0096","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:1689d26fc7e91753ef919011f20030f6af2a5ae61c53c62403d643af1cdddec1","observation_id":"d2f7b07e-8411-47c5-a7ad-72cde9ccad7f","resolution":{"observed_at":"2026-08-10T14:01:08.916797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2420","last_updated":"2009-03-07T02:10:36Z","snapshot_observed_at":"2026-08-03T22:44:29.548949Z","submitted_at":"2007-11-15T14:44:17Z","title":"Tidal Love numbers of neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.2420","snapshot_observed_at":"2026-08-10T14:01:08.921481Z","title":"Hinderer, Astrophys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.921481Z"},"links":{"cited_paper":"/paper/0711.2420","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:91d07eac2dcb9f9015d16c6272c09308ae7992c5fde020f11da062adfb25276f","observation_id":"ae565f63-d436-477f-9a70-92d12307530e","resolution":{"observed_at":"2026-08-10T14:01:08.921481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.5098","last_updated":"2010-04-28T18:05:11Z","snapshot_observed_at":"2026-07-06T02:09:46.923631Z","submitted_at":"2010-04-28T18:05:11Z","title":"Tidal Love Numbers of Neutron and Self-Bound Quark Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.5098","snapshot_observed_at":"2026-08-10T14:01:08.926308Z","title":"Postnikov, M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.926308Z"},"links":{"cited_paper":"/paper/1004.5098","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:d2023288081cae63dbe8a25184f4e4dce7ff577cb1210d02c9260f42b2e9c0f6","observation_id":"40c2e161-cb11-40b4-87bd-4b31bce16663","resolution":{"observed_at":"2026-08-10T14:01:08.926308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.01139","last_updated":"2020-10-13T11:13:37Z","snapshot_observed_at":"2026-08-08T00:52:32.514511Z","submitted_at":"2020-06-30T07:45:56Z","title":"Comment on \"Tidal Love numbers of neutron and self-bound quark stars\"","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.01139","snapshot_observed_at":"2026-08-10T14:01:08.931571Z","title":"Tak´ atsy and P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.931571Z"},"links":{"cited_paper":"/paper/2007.01139","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:9418a3ece9d453daaffc5b893cb1da76f02f6896da866e8f994e32e30d9a3112","observation_id":"ff58e36b-b171-4073-bbc7-8b0c4e504a57","resolution":{"observed_at":"2026-08-10T14:01:08.931571Z","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":"2026-08-10T06:35:57.906968Z","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":"2026-08-10T14:01:08.936097Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.936097Z"},"links":{"cited_paper":"/paper/1207.2184","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:d95e7ba504130fa297273283affacf85294139dca990866b643cf00288eba756","observation_id":"a8d0512a-fd33-4fec-899c-50a0b2d6223e","resolution":{"observed_at":"2026-08-10T14:01:08.936097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.6980","last_updated":"2017-01-30T01:27:54Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-12-22T13:54:29Z","title":"Adam: A Method for Stochastic Optimization","version":9},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.6980","snapshot_observed_at":"2026-08-10T14:01:08.940886Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.940886Z"},"links":{"cited_paper":"/paper/1412.6980","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:b6d9dc6f1bac814688ff07c0fd45319622fee1aa7ab25fb4ea5e32da457edd3b","observation_id":"c2f41a8b-3134-4f82-838c-2bd6889a388f","resolution":{"observed_at":"2026-08-10T14:01:08.940886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.08823","last_updated":"2019-05-27T16:51:57Z","snapshot_observed_at":"2026-08-04T18:35:05.807969Z","submitted_at":"2018-03-23T14:53:05Z","title":"A high-bias, low-variance introduction to Machine Learning for physicists","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.08823","snapshot_observed_at":"2026-08-10T14:01:08.945350Z","title":"Mehta, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.945350Z"},"links":{"cited_paper":"/paper/1803.08823","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:d558ca6db76e3a06e8f8722bdb7a2a3321737e70edddba3ea5ccdbe377814022","observation_id":"412748df-2f35-4a18-8d47-94b7be715fee","resolution":{"observed_at":"2026-08-10T14:01:08.945350Z","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":"2026-08-10T14:01:08.950218Z","title":"Kahn and A","venue":null,"work_id":null,"year":1953},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.950218Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:80c4557d9ee70a6fc5a40c0a5ed3d7e3f3b7f753d82c71753a716061e8dee3e4","observation_id":"f04d37c0-05dd-4f82-b06b-99eaac32c51b","resolution":{"observed_at":"2026-08-10T14:01:08.950218Z","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":"2026-08-10T14:01:08.954529Z","title":"Leshno and S","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.954529Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:a7fac55429d6fe7474cb6d0e5cf888fd80d981b3c6b094daa277f558a253c61a","observation_id":"157fc0e1-b555-4ebf-86b3-a129ad5701ae","resolution":{"observed_at":"2026-08-10T14:01:08.954529Z","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":"10.1007/s10472-020-09723-1","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T14:01:09.099854Z","title":"Kratsios, Annals of Mathematics and Artificial In- telligence (2021), 10.1007/s10472-020-09723-1","venue":null,"work_id":"fdc36de4-5270-43bb-bbdf-4943bcd3bd6c","year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.959016Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:4b3e8ef2d122f6e8a4fe3b38e92af98b125f4b92d19e3aed2fac93b9ec94378d","observation_id":"0aa3b49a-fce4-4277-863e-fa4ed1147491","resolution":{"observed_at":"2026-08-10T14:01:09.106281Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T14:01:08.963460Z","title":"LeCun, Y","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.963460Z"},"links":{"citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:7bf20eee16b50891ba23b0d43d0e39169894eaa6ff936d28158d2484f8cf261b","observation_id":"6642f92d-2bf0-4e78-af8e-5460f4ca9cbe","resolution":{"observed_at":"2026-08-10T14:01:08.963460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.04262","last_updated":"2017-08-02T01:50:06Z","snapshot_observed_at":"2026-07-06T05:22:31.301365Z","submitted_at":"2016-12-13T16:19:00Z","title":"An equation-of-state-meter of QCD transition from deep learning","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.04262","snapshot_observed_at":"2026-08-10T14:01:08.967967Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.967967Z"},"links":{"cited_paper":"/paper/1612.04262","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:54dd86fb3dc318e7558d8b8916fa7f2682fcd2d7e319ba4c3bb360fcc213e5fb","observation_id":"e8acddb9-ae00-49e6-b03e-d958d6d399eb","resolution":{"observed_at":"2026-08-10T14:01:08.967967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.05590","last_updated":"2021-10-25T11:26:31Z","snapshot_observed_at":"2026-07-06T11:28:24.094754Z","submitted_at":"2021-07-12T17:11:53Z","title":"An equation-of-state-meter for CBM using PointNet","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.05590","snapshot_observed_at":"2026-08-10T14:01:08.972482Z","title":"Omana Kuttan, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.972482Z"},"links":{"cited_paper":"/paper/2107.05590","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:f9267f446b467a366d8d740e170ca88a1f54d2503de606cbda487de497fbef09","observation_id":"0e52a289-8e89-4d0c-8574-b9a1c38597bc","resolution":{"observed_at":"2026-08-10T14:01:08.972482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.04090","last_updated":"2021-03-06T10:29:58Z","snapshot_observed_at":"2026-08-10T03:29:41.155852Z","submitted_at":"2021-03-06T10:29:58Z","title":"Deep learning stochastic processes with QCD phase transition","version":1},"cited_work":{"arxiv_id":"2103.04090","doi":null,"metadata_source":"pith","pith_arxiv_id":"2103.04090","snapshot_observed_at":"2026-08-10T14:01:09.429641Z","title":"Deep learning stochastic processes with QCD phase transition","venue":"nucl-th","work_id":"c832a003-70d1-482c-8b47-92d6b96f399f","year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.976999Z"},"links":{"cited_paper":"/paper/2103.04090","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:d1bd721bd2e4ce8878d5ef4700dbaec00dbb7a7b968e124b2b27360313946e25","observation_id":"d9057d0d-3654-44b8-8f78-e9cf9f572448","resolution":{"observed_at":"2026-08-10T14:01:09.434495Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.12879","last_updated":"2019-03-15T09:18:40Z","snapshot_observed_at":"2026-08-07T20:12:57.045299Z","submitted_at":"2018-10-30T17:22:57Z","title":"Regressive and generative neural networks for scalar field theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.12879","snapshot_observed_at":"2026-08-10T14:01:08.981415Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.981415Z"},"links":{"cited_paper":"/paper/1810.12879","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:529e1061bb2d476caf2fe6aa2a334cf8bd6ec729171c0c7d3aa88a00bc20d21c","observation_id":"2d2ea6f3-c12b-43bd-a4a0-a6956ae43a0f","resolution":{"observed_at":"2026-08-10T14:01:08.981415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.14830","last_updated":"2025-07-12T21:27:19Z","snapshot_observed_at":"2026-08-09T04:56:20.312140Z","submitted_at":"2024-05-23T17:46:49Z","title":"Deep learning lattice gauge theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.14830","snapshot_observed_at":"2026-08-10T14:01:08.986051Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.986051Z"},"links":{"cited_paper":"/paper/2405.14830","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:eebdd31ae10b76f2da1a2965291c41265e4f421fdeb2d6b61ae2d551360c930f","observation_id":"4d76bb9f-805a-4a2e-bf9a-07edca14b2d6","resolution":{"observed_at":"2026-08-10T14:01:08.986051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.04305","last_updated":"2021-02-01T12:34:20Z","snapshot_observed_at":"2026-07-06T07:52:13.448801Z","submitted_at":"2019-05-10T16:51:45Z","title":"Spectral Reconstruction with Deep Neural Networks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.04305","snapshot_observed_at":"2026-08-10T14:01:08.990511Z","title":"Kades, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.990511Z"},"links":{"cited_paper":"/paper/1905.04305","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:580ff8ef4966ede3aef296f6611bea9008d10c9f76d2528f3c768900ea25c9ee","observation_id":"2e53c087-b9e2-4d5d-b89f-08f986fb887c","resolution":{"observed_at":"2026-08-10T14:01:08.990511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14282","last_updated":"2021-04-13T21:41:42Z","snapshot_observed_at":"2026-08-06T18:57:14.940816Z","submitted_at":"2020-07-28T14:52:28Z","title":"Variational Monte Carlo calculations of $\\mathbf{A\\leq 4}$ nuclei with an artificial neural-network correlator ansatz","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.14282","snapshot_observed_at":"2026-08-10T14:01:08.994963Z","title":"Adams, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.994963Z"},"links":{"cited_paper":"/paper/2007.14282","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:8d7cef34664336d26fa28b636c5b37d34b586d1bd4fe0a821505cf06b01a9c61","observation_id":"e14dd706-06b4-47f5-aa3c-f03d0d93761c","resolution":{"observed_at":"2026-08-10T14:01:08.994963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.04436","last_updated":"2022-12-08T17:55:25Z","snapshot_observed_at":"2026-08-01T17:57:43.304722Z","submitted_at":"2022-12-08T17:55:25Z","title":"Dilute neutron star matter from neural-network quantum states","version":1},"cited_work":{"arxiv_id":"2212.04436","doi":null,"metadata_source":"pith","pith_arxiv_id":"2212.04436","snapshot_observed_at":"2026-08-10T14:01:09.351253Z","title":"Dilute neutron star matter from neural-network quantum states","venue":"nucl-th","work_id":"b81da01d-5f74-44eb-93c2-11c77bc481e0","year":2022},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.999481Z"},"links":{"cited_paper":"/paper/2212.04436","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:c7543a259794d02a74e9b2b095b093daaf810e761231763f2340843b8445ed1a","observation_id":"5699ff61-b3ef-41c2-a88c-d4a580bb7d6d","resolution":{"observed_at":"2026-08-10T14:01:09.356349Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03090","last_updated":"2025-07-16T05:50:16Z","snapshot_observed_at":"2026-07-06T20:01:23.373458Z","submitted_at":"2024-12-04T07:38:34Z","title":"A deep neural network approach to solve the Dirac equation","version":2},"cited_work":{"arxiv_id":"2412.03090","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03090","snapshot_observed_at":"2026-08-10T14:01:09.330033Z","title":"A deep neural network approach to solve the Dirac equation","venue":"quant-ph","work_id":"890ef8e9-4cf4-4e07-a7a1-348f0c1af8b1","year":2024},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:09.004267Z"},"links":{"cited_paper":"/paper/2412.03090","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:14871eb5908967d8238bf92e24af9b27606eeceb4d016a11abe3ec1c400cee42","observation_id":"7ded3147-a9e6-4c0b-8bbc-58dd0712b58f","resolution":{"observed_at":"2026-08-10T14:01:09.335117Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-11T09:25:50.152384Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":2,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":91,"verified_exact":6,"verified_fuzzy":0},"total_outbound_references":114},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 114 outbound references and 4 inbound Pith citation observations for arXiv:2501.15810."}