{"as_of":"2026-08-16T17:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:af7b8116da8e576ff4efa5eee6733103caeb03bc02fbd954a7d5159e78cc838e","coverage":[{"denominator":296,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T00:09:06.040583Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.12632/citation-record","integrity":"/paper/2608.12632/integrity","json":"/paper/2608.12632/citation-record.json","paper":"/paper/2608.12632"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2607.18124","last_updated":"2026-08-13T16:32:16Z","snapshot_observed_at":"2026-08-16T17:11:48.377572Z","submitted_at":"2026-07-20T16:19:21Z","title":"Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.18124","snapshot_observed_at":"2026-08-16T00:09:03.894527Z","title":"Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:03.894527Z"},"links":{"cited_paper":"/paper/2607.18124","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:22102ea803d37d00470d0185c481799f69854db57db9b2c66b392897edf63413","observation_id":"a9efdcac-b0ce-4183-9d2d-3432b14171cb","resolution":{"observed_at":"2026-08-16T00:09:03.894527Z","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":"2026-08-16T00:09:03.991527Z","title":"Investigating Twin Star Equation of States in Light of Recent Astrophysical Observations","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:03.991527Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:2d47bbd15d63a2141c55f6ee6c71d4c2cd0e438deb8fc3ca9725072ed53812f8","observation_id":"e86d38b1-77af-4c5c-a129-b7a98b11defb","resolution":{"observed_at":"2026-08-16T00:09:03.991527Z","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":"10.1103/99c1-2p2y","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:09:08.824577Z","title":null,"venue":null,"work_id":"fda527b0-15ab-4f92-a5fd-03b4ed3a07bd","year":2026},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:03.997223Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:97624d402ae6568f26c4571257e5a6053f5166b7ac072f44b8dbd087accfb517","observation_id":"1d8595d7-63b6-43d0-a939-f3bae6fbbe14","resolution":{"observed_at":"2026-08-16T00:09:08.829802Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07524","last_updated":"2017-07-24T12:49:14Z","snapshot_observed_at":"2026-08-14T20:45:44.220911Z","submitted_at":"2017-07-24T12:49:14Z","title":"Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.07524","snapshot_observed_at":"2026-08-16T00:09:04.002877Z","title":"Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.002877Z"},"links":{"cited_paper":"/paper/1707.07524","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:62fe6957bf50b05933adf0894b977e41f47fda6aa411eb8dae2ee5ba5f85e624","observation_id":"4c4e31b8-4823-402c-94de-f8d840b44f36","resolution":{"observed_at":"2026-08-16T00:09:04.002877Z","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":"2026-08-16T00:09:04.009615Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.009615Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:c222dd4d3738b2d7643ce96baba3bd8302abe8e0850fb960f68f0e363e233b0c","observation_id":"500e6159-9b6e-46d8-ac15-2ae1e174103f","resolution":{"observed_at":"2026-08-16T00:09:04.009615Z","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":"2026-08-16T00:09:04.015996Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.015996Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:ef26ee85c48129e5b627a7054ede3f9353941dc5d96d96d321aaef074444abe2","observation_id":"eef706a4-cda3-4cec-bef9-91ad4841621a","resolution":{"observed_at":"2026-08-16T00:09:04.015996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.05287","last_updated":"2025-02-20T17:55:00Z","snapshot_observed_at":"2026-08-16T13:27:23.300127Z","submitted_at":"2024-08-09T18:16:47Z","title":"Constraining twin stars with cold neutron star cooling data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05287","snapshot_observed_at":"2026-08-16T00:09:04.022624Z","title":"urgen , title =","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.022624Z"},"links":{"cited_paper":"/paper/2408.05287","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:d6c863b5d4ac21b4f1a59678e06a8f9e9063f13876e181a54c6b2fe8b509125a","observation_id":"ff299539-979b-43ad-9366-3482682ac79c","resolution":{"observed_at":"2026-08-16T00:09:04.022624Z","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":"2026-08-16T00:09:04.080168Z","title":"Hybrid stars with large quark cores within the parity doublet model and modified NJL model","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.080168Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:001dec75786e34854c6d877b0a86d0d5482a24d8b3767e4a29fbef7358444079","observation_id":"6ae90bbb-21c9-4d6c-8fd4-b06390ae8edf","resolution":{"observed_at":"2026-08-16T00:09:04.080168Z","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":"2026-08-16T00:09:04.101121Z","title":"Confirming the Existence of Twin Stars in a","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.101121Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:3210cbaca887031ef0e99360555380645a51bee232a6897d7f2534fd144c543c","observation_id":"09b91625-20b5-450b-96be-ded217d4c8f6","resolution":{"observed_at":"2026-08-16T00:09:04.101121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.09798","last_updated":"2023-01-19T05:21:20Z","snapshot_observed_at":"2026-08-16T16:44:37.094996Z","submitted_at":"2022-07-20T10:28:48Z","title":"Ultracompact hybrid stars consistent with multimessenger astrophysics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.09798","snapshot_observed_at":"2026-08-16T00:09:04.106582Z","title":"Ultracompact hybrid stars consistent with multimessenger astrophysics","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.106582Z"},"links":{"cited_paper":"/paper/2207.09798","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:e2b03db25efb915590621b02f43fd8511321b4f6fb2f530391eda12aaeca4725","observation_id":"639399c0-d41a-4475-beaf-321d6e579349","resolution":{"observed_at":"2026-08-16T00:09:04.106582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.06453","last_updated":"2025-01-11T06:56:36Z","snapshot_observed_at":"2026-08-16T12:59:12.836793Z","submitted_at":"2025-01-11T06:56:36Z","title":"Comparison of Equations of State for Neutron Stars with First-Order Phase Transitions: A Qualitative Study","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.06453","snapshot_observed_at":"2026-08-16T00:09:04.112990Z","title":"Astrophysical Journal , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.112990Z"},"links":{"cited_paper":"/paper/2501.06453","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:8e579aa528f37fca797aa8552bc4305eaa7901209b371c6e5daa474c2e8e2c7d","observation_id":"03b46342-5e5d-49ef-adc0-84520560f1aa","resolution":{"observed_at":"2026-08-16T00:09:04.112990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.02945","last_updated":"2025-04-03T18:02:19Z","snapshot_observed_at":"2026-08-16T12:44:09.921032Z","submitted_at":"2025-04-03T18:02:19Z","title":"Is the central compact object in HESS J1731-347 a hybrid star with a quark core? An analysis with the constant speed of sound parametrization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.02945","snapshot_observed_at":"2026-08-16T00:09:04.118307Z","title":"Astrophysical Journal , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.118307Z"},"links":{"cited_paper":"/paper/2504.02945","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:8e4183110759b882d0582003febb41a64e64a4c264ffb70883d9d813f5352f7e","observation_id":"d5ad3998-6b16-411b-8cbc-560f5e6ceebb","resolution":{"observed_at":"2026-08-16T00:09:04.118307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.00240","last_updated":"2025-07-12T13:06:40Z","snapshot_observed_at":"2026-08-16T12:45:09.987132Z","submitted_at":"2025-03-31T21:21:29Z","title":"Properties of the Object HESS J1731-347 as a Twin Compact Star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.00240","snapshot_observed_at":"2026-08-16T00:09:04.122768Z","title":"Properties of the Object HESS J1731-347 as a Twin Compact Star","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.122768Z"},"links":{"cited_paper":"/paper/2504.00240","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:61aa08ef8131a974aced5a2e2ef09e4a70aededac73ec78d2e9dd3aad6c1a9d0","observation_id":"47681be3-e496-42e0-b8b0-0f46e79f7a04","resolution":{"observed_at":"2026-08-16T00:09:04.122768Z","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":"2026-08-16T00:09:04.191791Z","title":"Twin Stars and the Stiffness of the Nuclear Equation of State:","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.191791Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:6501c57492ceaa36e99db9d89bfee8d7248cd3e5286fc763f06cad132fcc31be","observation_id":"4c2057ea-d08f-4498-aeb7-be2f778a2623","resolution":{"observed_at":"2026-08-16T00:09:04.191791Z","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":"2026-08-16T00:09:04.257160Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.257160Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0bd619de824e21393d4af49930e7000050b6f4873cb0a6d128b5e43b8c64906c","observation_id":"9629bc02-eedc-4561-89a1-f3922c8cc48f","resolution":{"observed_at":"2026-08-16T00:09:04.257160Z","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":"2026-08-16T00:09:04.266677Z","title":"and Koliogiannis, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.266677Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:1d3f37cd3d5af5695986f0615ac466cbce09f94b9a392e376f5827cca239660e","observation_id":"58de4236-3b8c-4643-bb57-136108206aca","resolution":{"observed_at":"2026-08-16T00:09:04.266677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.10929","last_updated":"2019-06-11T13:00:11Z","snapshot_observed_at":"2026-08-16T08:19:04.918203Z","submitted_at":"2018-11-27T11:53:55Z","title":"Constraining twin stars with GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.10929","snapshot_observed_at":"2026-08-16T00:09:04.271486Z","title":"Constraining twin stars with GW170817","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.271486Z"},"links":{"cited_paper":"/paper/1811.10929","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:5d83e31d8f09b968548869bf8726ec40a9b7ca632514c26efab7b937c7689ffb","observation_id":"28f56b99-9eb3-4b27-a8f4-d1b86466d9bb","resolution":{"observed_at":"2026-08-16T00:09:04.271486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.10576","last_updated":"2023-08-08T15:37:35Z","snapshot_observed_at":"2026-08-16T16:07:11.196921Z","submitted_at":"2022-12-20T19:00:01Z","title":"Constraints on strong phase transitions in neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.10576","snapshot_observed_at":"2026-08-16T00:09:04.281990Z","title":"doi:10.3847/1538-4357/aceefb , archivePrefix =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.281990Z"},"links":{"cited_paper":"/paper/2212.10576","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:122db31882e04ca1bd6749ef6f9970fd7a6f1d0198e4345bbf29f8a23e3f9149","observation_id":"a4f80822-aca1-4cca-b891-df827f6a0165","resolution":{"observed_at":"2026-08-16T00:09:04.281990Z","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":"2026-08-16T00:09:04.364746Z","title":"Hybrid star properties with the NJL and mean field approximation of QCD models: A Bayesian approach","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.364746Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:a36eb98b45f507514841b28d0b0862cf43b5c9999e733b853509c71d0a96de6d","observation_id":"d4493e31-3c99-4f65-b3cd-5eeb907fde0b","resolution":{"observed_at":"2026-08-16T00:09:04.364746Z","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":"2026-08-16T00:09:04.403834Z","title":"Hybrid Star Models in the Light of New Multimessenger Data , volume=","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.403834Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:b018d9b1d94be256877738244ac5d328f4f152bada9ce43805e67427eb345fa3","observation_id":"4c0c721e-282d-41ec-8a0f-d1765248e01e","resolution":{"observed_at":"2026-08-16T00:09:04.403834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.03457","last_updated":"2016-03-10T21:43:40Z","snapshot_observed_at":"2026-08-16T08:19:01.221935Z","submitted_at":"2016-03-10T21:43:40Z","title":"New class of hybrid EoS and Bayesian M-R data analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.03457","snapshot_observed_at":"2026-08-16T00:09:04.409362Z","title":"and Ayriyan, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.409362Z"},"links":{"cited_paper":"/paper/1603.03457","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:f532a56625e747a65c8ee7f862ac3fd6c7a8474b08825f0c7f82f0990f9db7ae","observation_id":"5cde9147-5690-4d51-a012-385b0da45580","resolution":{"observed_at":"2026-08-16T00:09:04.409362Z","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":"2026-08-16T00:09:04.413987Z","title":null,"venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.413987Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:9acbc106f6705ea8ca2df0f6913d242644190bc763c69fe792c8401262ac6d82","observation_id":"7b153147-dac5-4b3f-bb81-3a3b1f0b1a31","resolution":{"observed_at":"2026-08-16T00:09:04.413987Z","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":"2026-08-16T00:09:04.419162Z","title":"On the Possibility of Stable Quark and Pion Condensed Stars","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.419162Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:b5fe995339f83dce82cb325aea29113edbff58dbbee3629d59cb1cec1a8ab349","observation_id":"db7c985c-6989-48b8-8ecb-64ad05a7190a","resolution":{"observed_at":"2026-08-16T00:09:04.419162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03252","last_updated":"2019-01-10T16:24:48Z","snapshot_observed_at":"2026-08-16T08:20:56.419908Z","submitted_at":"2019-01-10T16:24:48Z","title":"Phase Transitions in Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03252","snapshot_observed_at":"2026-08-16T00:09:04.423606Z","title":"and Soethe, L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.423606Z"},"links":{"cited_paper":"/paper/1901.03252","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:685653a6d5c9e273e62d459cda8be6fff2ec2d445d9ba634ab39f5b0132eaee0","observation_id":"a0f7b4f0-709b-4cac-ae48-26f27d1dde81","resolution":{"observed_at":"2026-08-16T00:09:04.423606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.4225","last_updated":"2008-09-24T16:25:08Z","snapshot_observed_at":"2026-08-15T10:06:09.401772Z","submitted_at":"2008-09-24T16:25:08Z","title":"Signals of the QCD phase transition in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.4225","snapshot_observed_at":"2026-08-16T00:09:04.587462Z","title":"and Fischer, T","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.587462Z"},"links":{"cited_paper":"/paper/0809.4225","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:64ff4f0bfe017303a1c63cf8f697b998c375525604f243812ebb8b0b12b36e15","observation_id":"d250f4d9-ebfd-4964-9eb9-d8c3bfe2f2dc","resolution":{"observed_at":"2026-08-16T00:09:04.587462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.4375","last_updated":"2010-04-25T19:53:48Z","snapshot_observed_at":"2026-08-15T05:20:41.613516Z","submitted_at":"2010-04-25T19:53:48Z","title":"Accessibility of color superconducting quark matter phases in heavy-ion collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.4375","snapshot_observed_at":"2026-08-16T00:09:04.591551Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.591551Z"},"links":{"cited_paper":"/paper/1004.4375","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0cf40e1dc459275508ce864e926d3ec5eec61ae37c0adb7f12d65264eb6fe0fe","observation_id":"72c0c5cd-94e3-4375-9b00-5254630b0c61","resolution":{"observed_at":"2026-08-16T00:09:04.591551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807155","last_updated":"1998-10-22T19:43:44Z","snapshot_observed_at":"2026-08-16T08:23:49.286306Z","submitted_at":"1998-07-15T16:14:13Z","title":"Non-Identical Neutron Star Twins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807155","snapshot_observed_at":"2026-08-16T00:09:04.595913Z","title":"and Kettner, Christiane","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.595913Z"},"links":{"cited_paper":"/paper/astro-ph/9807155","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:ee73b282c22e051084e1ec6e2ca2ead672f03d08e9b56a2522d5a5c90ab82883","observation_id":"0cd79d39-64e1-46ee-9808-b75eab8176ea","resolution":{"observed_at":"2026-08-16T00:09:04.595913Z","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":"2026-08-16T00:09:04.600723Z","title":"and Greiner, C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.600723Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:12a7c1b69174d74d3b3c325ca4c98f8d158a3ebbf3d6ec1eff4e171c395b414a","observation_id":"e4f92347-784c-4010-9696-308dbe058da4","resolution":{"observed_at":"2026-08-16T00:09:04.600723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06753","last_updated":"2022-11-16T23:01:14Z","snapshot_observed_at":"2026-08-16T16:46:03.414286Z","submitted_at":"2022-07-14T09:03:49Z","title":"Trace anomaly as signature of conformality in neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06753","snapshot_observed_at":"2026-08-16T00:09:04.606803Z","title":"and Praszalowicz, Michal","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.606803Z"},"links":{"cited_paper":"/paper/2207.06753","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:de96377f52c6b5c5adf60cb83ce2de8f02f18c92101a0c7837017b16c2196ddb","observation_id":"8694866b-2bda-4e71-b00b-62bd2b310ae8","resolution":{"observed_at":"2026-08-16T00:09:04.606803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04755","last_updated":"2025-02-10T17:46:22Z","snapshot_observed_at":"2026-08-16T13:20:34.183586Z","submitted_at":"2024-09-07T08:03:57Z","title":"Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.04755","snapshot_observed_at":"2026-08-16T00:09:04.612276Z","title":"and Ohse, D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.612276Z"},"links":{"cited_paper":"/paper/2409.04755","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:cbd0c439a364cea7e4e00eb3de06c225ae1dddcadae54f7cb79b57da1a00dc3e","observation_id":"9ad5139e-ca0d-4f70-8302-417d112e2d62","resolution":{"observed_at":"2026-08-16T00:09:04.612276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.00115","last_updated":"2025-04-12T11:42:07Z","snapshot_observed_at":"2026-08-13T20:29:26.332886Z","submitted_at":"2024-12-30T19:26:21Z","title":"Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.00115","snapshot_observed_at":"2026-08-16T00:09:04.661952Z","title":"and Grunfeld, Ana Gabriela","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.661952Z"},"links":{"cited_paper":"/paper/2501.00115","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:b3d6ad44726f1cdfecea686fef8130da3ceb2075bc3f3fa8b45f6a7582ccc343","observation_id":"ebce2899-1f00-46b0-b667-3ea36adc6072","resolution":{"observed_at":"2026-08-16T00:09:04.661952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.01426","last_updated":"2025-09-05T10:00:35Z","snapshot_observed_at":"2026-08-16T08:19:48.671194Z","submitted_at":"2024-12-02T12:08:02Z","title":"Simultaneous explanation of XTE J1814-338 and HESS J1731-347 objects using ${K^{-}}$ and ${\\bar{K}^{0}}$ condensates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.01426","snapshot_observed_at":"2026-08-16T00:09:04.732303Z","title":"and Petousis, V","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.732303Z"},"links":{"cited_paper":"/paper/2412.01426","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:cf8f6e4d5937064cb52016a4ce7ab6c93473aa76e3b4c9dfb01e851aa5a3a99c","observation_id":"00d9e6dd-8809-4bff-abb2-335eff3cba29","resolution":{"observed_at":"2026-08-16T00:09:04.732303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.15544","last_updated":"2024-08-19T23:42:15Z","snapshot_observed_at":"2026-08-16T13:40:39.000305Z","submitted_at":"2024-06-21T18:00:00Z","title":"Exploring pathways to forming twin stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.15544","snapshot_observed_at":"2026-08-16T00:09:04.737276Z","title":"Exploring pathways to forming twin stars","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.737276Z"},"links":{"cited_paper":"/paper/2406.15544","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:28efc18537ab95a3c1056df06c44fbb17a75bdc963714156f0edcc5cd6d6a09e","observation_id":"84bef75f-c496-48a6-86f3-f8c086dc9e81","resolution":{"observed_at":"2026-08-16T00:09:04.737276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.01975","last_updated":"2024-03-01T13:25:32Z","snapshot_observed_at":"2026-08-16T14:37:49.687624Z","submitted_at":"2023-12-04T15:43:43Z","title":"Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.01975","snapshot_observed_at":"2026-08-16T00:09:04.742312Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.742312Z"},"links":{"cited_paper":"/paper/2312.01975","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:c1d709a746fbf8861aafc99a8829983d647d5643ba52ada9381e1d864bacd6f2","observation_id":"29713cbd-097d-4e28-aea0-c5f1dda93f6f","resolution":{"observed_at":"2026-08-16T00:09:04.742312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11614","last_updated":"2024-12-17T15:59:00Z","snapshot_observed_at":"2026-08-16T13:24:53.960915Z","submitted_at":"2024-08-21T13:42:05Z","title":"How the QCD trace anomaly behaves at the core of twin stars?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11614","snapshot_observed_at":"2026-08-16T00:09:04.747230Z","title":"and Lazzari, Lucas and Gon c alves, Victor P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.747230Z"},"links":{"cited_paper":"/paper/2408.11614","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:54225f4300c56061741f0ff5a9c5a0e8b0b63d3ea3e16690fa13edde721a8d09","observation_id":"f685ee52-9032-44e9-a504-2f7edea15cba","resolution":{"observed_at":"2026-08-16T00:09:04.747230Z","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":"2026-08-16T00:09:04.751481Z","title":"2025 , version =","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.751481Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:d6cd693f62f18d9e17474d3c4147b908518ceb4f14b5d8f4b9e65d65ce547283","observation_id":"09d59a1e-c785-425c-8f6d-30d735467ec6","resolution":{"observed_at":"2026-08-16T00:09:04.751481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0004375","last_updated":"2000-04-27T09:59:18Z","snapshot_observed_at":"2026-08-15T16:54:57.324491Z","submitted_at":"2000-04-27T09:59:18Z","title":"Strange stars - linear approximation of the EOS and maximum QPO frequency","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0004375","snapshot_observed_at":"2026-08-16T00:09:04.758072Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.758072Z"},"links":{"cited_paper":"/paper/astro-ph/0004375","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:2f46a767a0bfd00dac1fa749c85086efa2a8820a2d0220dd619a03d6694b54a8","observation_id":"f63e1dd3-4bf5-46e1-b559-c4f0cfc48c70","resolution":{"observed_at":"2026-08-16T00:09:04.758072Z","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":"2026-08-16T00:09:04.800118Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.800118Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:5d0d5b2c7a5c6afd247b0bf146836437b318b0451fe0d2f42f805cfd85459873","observation_id":"179b007f-611f-4a02-b101-92f160e861b4","resolution":{"observed_at":"2026-08-16T00:09:04.800118Z","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":"2026-08-16T00:09:04.804502Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.804502Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:3d03a6c734d54824c2272a5253ce0bd0ebf40c4c908e7c220d1a51ebe5e762c3","observation_id":"d03e555d-d4ea-4537-8aba-c6a2b5a20eff","resolution":{"observed_at":"2026-08-16T00:09:04.804502Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6875","last_updated":"2013-04-25T11:01:50Z","snapshot_observed_at":"2026-08-15T02:01:27.880780Z","submitted_at":"2013-04-25T11:01:50Z","title":"A Massive Pulsar in a Compact Relativistic Binary","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.6875","snapshot_observed_at":"2026-08-16T00:09:04.808351Z","title":"A Massive Pulsar in a Compact Relativistic Binary","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.808351Z"},"links":{"cited_paper":"/paper/1304.6875","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:6d22dad8c834af6403b098a42cf5999962fe4802d7912e34c8e92ae8e5ed0bbc","observation_id":"3e56a3f9-976c-4f48-b7fd-2019467c8da6","resolution":{"observed_at":"2026-08-16T00:09:04.808351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.2856","last_updated":"2015-03-30T06:23:02Z","snapshot_observed_at":"2026-08-14T23:12:05.093912Z","submitted_at":"2014-11-11T15:41:18Z","title":"A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.2856","snapshot_observed_at":"2026-08-16T00:09:04.812525Z","title":"and Fischer, Tobias and Typel, Stefan","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.812525Z"},"links":{"cited_paper":"/paper/1411.2856","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:64b99e0e2e0ca8b7fe8bf5a0b8397d6a83e99d6b8dec9188e51277b5b8ec2f46","observation_id":"b72978b7-c438-4d55-8210-071dffb4f8bc","resolution":{"observed_at":"2026-08-16T00:09:04.812525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.04400","last_updated":"2017-06-19T17:19:47Z","snapshot_observed_at":"2026-08-14T21:20:58.020109Z","submitted_at":"2017-01-16T18:54:58Z","title":"Quark-Nuclear Hybrid EoS with Excluded Volume Effects","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.04400","snapshot_observed_at":"2026-08-16T00:09:04.816829Z","title":"Quark-nuclear hybrid star equation of state with excluded volume effects","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.816829Z"},"links":{"cited_paper":"/paper/1701.04400","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:6505a089d3edc6dfe7aa1d34f32de4b48412db709fd87b0b662e60bc08bd1921","observation_id":"1e333661-5fec-4524-ad8c-810e82481119","resolution":{"observed_at":"2026-08-16T00:09:04.816829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.04105","last_updated":"2019-01-17T18:24:23Z","snapshot_observed_at":"2026-08-14T19:16:41.066515Z","submitted_at":"2018-05-10T17:59:54Z","title":"Third family of compact stars within a nonlocal chiral quark model equation of state","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.04105","snapshot_observed_at":"2026-08-16T00:09:04.821324Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.821324Z"},"links":{"cited_paper":"/paper/1805.04105","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:c1fb1733c422e9cc95373b79abc0176c61ff04fef782e6debb1a2af8fd38d01a","observation_id":"01b1e81c-7ea8-40bf-b2d2-69343e69db1e","resolution":{"observed_at":"2026-08-16T00:09:04.821324Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.8463","last_updated":"2017-10-07T20:58:46Z","snapshot_observed_at":"2026-08-14T23:05:50.879719Z","submitted_at":"2014-12-29T20:55:59Z","title":"Mixed phase effects on high-mass twin stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.8463","snapshot_observed_at":"2026-08-16T00:09:04.826381Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.826381Z"},"links":{"cited_paper":"/paper/1412.8463","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:5fe69595c7831d269d08afb3a8fe5d561cbd073f05e38767c84b2e32a6340ce3","observation_id":"e15a447b-693a-454e-8914-d5b89c019e59","resolution":{"observed_at":"2026-08-16T00:09:04.826381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03926","last_updated":"2018-05-02T17:16:41Z","snapshot_observed_at":"2026-08-14T20:14:51.519880Z","submitted_at":"2017-11-10T17:23:54Z","title":"Robustness of third family solutions for hybrid stars against mixed phase effects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03926","snapshot_observed_at":"2026-08-16T00:09:04.857036Z","title":"and Bastian, N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.857036Z"},"links":{"cited_paper":"/paper/1711.03926","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:4ec4535005053540984ed2b49260f3e8989bb62084ecd80cacee9ad2b45afff3","observation_id":"1c629a14-3cab-4d25-b559-f67a06305daa","resolution":{"observed_at":"2026-08-16T00:09:04.857036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.07049","last_updated":"2017-01-08T15:57:49Z","snapshot_observed_at":"2026-08-16T08:20:01.625242Z","submitted_at":"2016-08-25T08:24:39Z","title":"Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.07049","snapshot_observed_at":"2026-08-16T00:09:04.862396Z","title":"and Blaschke, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.862396Z"},"links":{"cited_paper":"/paper/1608.07049","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:162f33ad7f562f8c216a5d9b0875760b3b645dc24073c60ef082278e95bcd8b2","observation_id":"2facf3cd-07df-4d79-9ca4-8e2bc1d05d6a","resolution":{"observed_at":"2026-08-16T00:09:04.862396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04971","last_updated":"2024-12-06T11:42:31Z","snapshot_observed_at":"2026-08-15T15:56:14.754222Z","submitted_at":"2024-12-06T11:42:31Z","title":"Tripling Fluctuations and Peaked Sound Speed in Fermionic Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.04971","snapshot_observed_at":"2026-08-16T00:09:04.867179Z","title":"Tripling Fluctuations and Peaked Sound Speed in Fermionic Matter","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.867179Z"},"links":{"cited_paper":"/paper/2412.04971","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:7c52fed60e755dbcf91085b3897a921c922081fa74447d103d67c865d1907ed9","observation_id":"bb20adc1-b4b4-426c-8f33-52433df62749","resolution":{"observed_at":"2026-08-16T00:09:04.867179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.02554","last_updated":"2025-09-02T17:50:38Z","snapshot_observed_at":"2026-08-16T13:05:49.605770Z","submitted_at":"2025-09-02T17:50:38Z","title":"Bayesian inference favors quark matter in neutron star interiors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.02554","snapshot_observed_at":"2026-08-16T00:09:04.872380Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.872380Z"},"links":{"cited_paper":"/paper/2509.02554","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:10e550f27ffb349b1e5a73f35c9ada4ab291f5996f1d9c14b0e2b7b0e2e743f9","observation_id":"9ec10476-ce20-40c1-82ae-df0c3e4e8b48","resolution":{"observed_at":"2026-08-16T00:09:04.872380Z","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":"2026-08-16T00:09:04.952945Z","title":"Gravitational waves from neutron star mergers and their relation to the nuclear equation of state","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.952945Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:46661f2108db273a2342a9e393b099ff674e9475ea8bb82133a2259a93853e66","observation_id":"d96e041f-d178-4d25-a7b7-17d2e00bd47c","resolution":{"observed_at":"2026-08-16T00:09:04.952945Z","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":"2026-08-16T00:09:04.996351Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:04.996351Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:e9c44795e59295158653fe186c8b257f0c4fd5433175575024bcf9b24e10904a","observation_id":"5012a1dc-a565-4070-a4de-32b1bae43a4a","resolution":{"observed_at":"2026-08-16T00:09:04.996351Z","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":"2026-08-16T00:09:05.000739Z","title":"Thankful and Gandolfi, Stefano and Tews, Ingo and Radice, David and Steiner, Andrew W","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.000739Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:559fdc799b304a07bfcea86ca8d89a9e759e02eb772435e945dc8fa3af0caf57","observation_id":"e4d1c11c-a705-4dbe-b2c3-9d0d5119a6ab","resolution":{"observed_at":"2026-08-16T00:09:05.000739Z","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":"2026-08-16T00:09:05.005933Z","title":"Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.005933Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0354392c1fba071810a5b6810917e754f29a7b54c874c1423c07f563572d1698","observation_id":"62b8226a-7378-4c5f-964f-b14301e17776","resolution":{"observed_at":"2026-08-16T00:09:05.005933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.03100","last_updated":"2025-01-06T15:58:36Z","snapshot_observed_at":"2026-08-15T12:11:00.835801Z","submitted_at":"2025-01-06T15:58:36Z","title":"The NewAthena mission concept in the context of the next decade of X-ray astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.03100","snapshot_observed_at":"2026-08-16T00:09:05.010672Z","title":"The NewAthena mission concept in the context of the next decade of X-ray astronomy","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.010672Z"},"links":{"cited_paper":"/paper/2501.03100","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:15ee2424480c77beac9f18c43c839d385b46d7aa53492a36a92f51a6685dafa0","observation_id":"74cf75ba-97d4-4690-ac59-b844bdf6bd2d","resolution":{"observed_at":"2026-08-16T00:09:05.010672Z","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":"2026-08-16T00:09:05.016251Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.016251Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:66662ddfb15741e4416f80271f2e4a28125e188bea3004b978f0ee6e3280005b","observation_id":"baf6876a-d6d4-48b9-af63-c4a48ef87822","resolution":{"observed_at":"2026-08-16T00:09:05.016251Z","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":"2026-08-16T00:09:05.022362Z","title":"Bernoulli","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.022362Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0b04657aebc448fe48a069baf2d6019d2b986efa2331ac5044ad7954a08155af","observation_id":"a71ef57f-3bfd-4490-aab0-06ef3a60ca3c","resolution":{"observed_at":"2026-08-16T00:09:05.022362Z","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":"2026-08-16T00:09:05.044993Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.044993Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:d8a4adec3331a2e2b84bfc3e33aac28590020aae4f392a6cbee978fd7a9a8ff6","observation_id":"47336996-7f26-4fe0-bbb4-44e03080ddda","resolution":{"observed_at":"2026-08-16T00:09:05.044993Z","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":"2026-08-16T00:09:05.126339Z","title":"https://global.oup.com/academic/product/microeconomic-theory-9780195073409","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.126339Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:bf525532c059596bdc9572235b40a737294877da74d624d4c7cabd39266ec1fa","observation_id":"fde0c831-19d0-4fdb-8799-725ee78fcdd9","resolution":{"observed_at":"2026-08-16T00:09:05.126339Z","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":"2026-08-16T00:09:05.187554Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.187554Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:6fe41044181b61dd758c3843de1bcd7bd528e2f8586e1043f748da4458c37305","observation_id":"1ff7c7dc-f3df-40a4-8e4a-972427ac466c","resolution":{"observed_at":"2026-08-16T00:09:05.187554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02935","last_updated":"2024-07-03T09:10:13Z","snapshot_observed_at":"2026-08-16T13:37:28.171136Z","submitted_at":"2024-07-03T09:10:13Z","title":"Properties of the QCD Matter -- An Experimental Review of Selected Results from RHIC BES Program","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.02935","snapshot_observed_at":"2026-08-16T00:09:05.191994Z","title":"Properties of the QCD matter: review of selected results from the relativistic heavy ion collider beam energy scan (RHIC BES) program","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.191994Z"},"links":{"cited_paper":"/paper/2407.02935","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:b2934b3b615f31ec4f25faf9078ae99e0f7b8dd693e148009c305791aee7afd8","observation_id":"cb7a5f54-0ba9-424f-83e1-f3a2ddff96e2","resolution":{"observed_at":"2026-08-16T00:09:05.191994Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2843","last_updated":"2014-07-10T16:06:47Z","snapshot_observed_at":"2026-08-14T23:27:11.547974Z","submitted_at":"2014-07-10T16:06:47Z","title":"Is there a \"$\\Delta$-isobar puzzle\" in the physics of neutron stars?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2843","snapshot_observed_at":"2026-08-16T00:09:05.196570Z","title":"Early appearance of isobars in neutron stars","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.196570Z"},"links":{"cited_paper":"/paper/1407.2843","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0107e7ce0f89f1cdffa5cf3d6a7423382e9baa078b6478010e9141020819f496","observation_id":"b809b2a4-53ac-4ecc-8a7c-fe7a2d07813c","resolution":{"observed_at":"2026-08-16T00:09:05.196570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01680","last_updated":"2015-06-22T23:27:41Z","snapshot_observed_at":"2026-08-14T23:04:52.700948Z","submitted_at":"2015-01-07T22:50:05Z","title":"Critical Density and Impact of $\\Delta (1232)$ Resonance Formation in Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01680","snapshot_observed_at":"2026-08-16T00:09:05.201560Z","title":"and Li, Bao-An and Newton, William G","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.201560Z"},"links":{"cited_paper":"/paper/1501.01680","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:66528ab5ec6c474cff779297473b5c3117d7666becda6538f69d35bc19dee457","observation_id":"4fb18a29-e02e-4f34-a246-5fc096dca850","resolution":{"observed_at":"2026-08-16T00:09:05.201560Z","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":"2026-08-16T00:09:05.206838Z","title":"Beyond ^ 2/3 Scaling: Microscopic Origins and Multimessengers of High-Density Nuclear Symmetry Energy","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.206838Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:817dac09ab3f0af2e86ec7808d4b25420ac9cb3084d3561fc4945273383313d3","observation_id":"e4bb7a35-55c7-4aef-8510-0db5a9772cd1","resolution":{"observed_at":"2026-08-16T00:09:05.206838Z","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":"2026-08-16T00:09:05.211921Z","title":"Coleman and Lamb, Frederick K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.211921Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:a64f09959cedf2492d410722c100f258eb5d8bcf7c33caf9ff82e1979cb4e9ac","observation_id":"2de6813a-08c3-4a24-8fd9-a7e5278d64fe","resolution":{"observed_at":"2026-08-16T00:09:05.211921Z","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":"2026-08-16T00:09:05.216974Z","title":"Dense matter in neutron stars with eXTP","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.216974Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:8dc4e7da1c09f36834f0d7e8b3a9627d970a383e7551ae4ecbd6bd7f3b9b7cc4","observation_id":"f941c840-16cb-40c4-b907-6b1133b3521e","resolution":{"observed_at":"2026-08-16T00:09:05.216974Z","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":"2026-08-16T00:09:05.222054Z","title":"2025 , note =","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.222054Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:e84da5208aad2becfca70ee4dc7c7d42621bfa868b4b46ef2a7af99fa5b4e5be","observation_id":"7c52b9f7-f095-4d19-b4e6-1230935bc78b","resolution":{"observed_at":"2026-08-16T00:09:05.222054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.14572","last_updated":"2025-01-09T19:39:33Z","snapshot_observed_at":"2026-08-16T13:07:58.869091Z","submitted_at":"2024-10-18T16:18:50Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements II: Hyperonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.14572","snapshot_observed_at":"2026-08-16T00:09:05.257404Z","title":"Constraining a relativistic mean field model using neutron star mass radius measurements II: hyperonic models","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.257404Z"},"links":{"cited_paper":"/paper/2410.14572","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:78465bc0522eea849b620fac6624ca94b18c2f96c64091aaa30dc12e7d1fb405","observation_id":"806db9f6-ee21-4260-a68e-13d850b4666f","resolution":{"observed_at":"2026-08-16T00:09:05.257404Z","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":"2026-08-16T00:09:05.380708Z","title":"2025 , note =","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.380708Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:430f64c2600142112e7dc3da1eabb340649b2fdb07354f0d91d7469fc1f905c2","observation_id":"f00138d9-db2d-4f8c-855a-c3546f020226","resolution":{"observed_at":"2026-08-16T00:09:05.380708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.4635","last_updated":"2008-01-21T08:57:17Z","snapshot_observed_at":"2026-08-15T10:31:18.786675Z","submitted_at":"2007-09-28T18:31:24Z","title":"Color superconductivity in dense quark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.4635","snapshot_observed_at":"2026-08-16T00:09:05.385067Z","title":"afer, Thomas , title =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.385067Z"},"links":{"cited_paper":"/paper/0709.4635","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:3848e734bfde1302b30c57a697841f9dad76f20bec8e989a057217fee68ae28f","observation_id":"dc13ee9e-4fe5-465b-b0c5-87664d4ba319","resolution":{"observed_at":"2026-08-16T00:09:05.385067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07823","last_updated":"2024-10-28T15:01:15Z","snapshot_observed_at":"2026-08-16T13:35:21.768400Z","submitted_at":"2024-07-10T16:48:22Z","title":"Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.07823","snapshot_observed_at":"2026-08-16T00:09:05.389639Z","title":"Bayesian inference of fine features of the nuclear equation of state from future neutron star radius measurements to 0.1 km accuracy","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.389639Z"},"links":{"cited_paper":"/paper/2407.07823","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0e685d4f4c80daf3bacddc49232ba7cf7c53e4426d154283cf63577cb1f81c2d","observation_id":"16206021-7350-4b7d-9b34-7a6d415f9cad","resolution":{"observed_at":"2026-08-16T00:09:05.389639Z","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":"10.48550/arxiv.2506.13677","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:09:08.665799Z","title":"Bayesian Quantification of Observability and Equation of State of Twin Stars","venue":null,"work_id":"22083efc-1fdf-4e33-b62a-d8d947b2b291","year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.394446Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:acdade9871906c074aee60128a0401c7306e4199c72b4cdb505eb765d103decc","observation_id":"521f5ff7-a167-464c-84bb-ca4e19b26d94","resolution":{"observed_at":"2026-08-16T00:09:08.671244Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T00:09:05.399524Z","title":"10.1051/0004-6361/201220697","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.399524Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:789b8c3d9513851f6c45a59d64f0895d4e767bfbbba4da970a44d79b98273232","observation_id":"100d29bb-a967-4d8b-bf42-1460857059f4","resolution":{"observed_at":"2026-08-16T00:09:05.399524Z","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":"2026-08-16T00:09:05.493016Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.493016Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:b9d9f1bad8e6de502efe4d641409d314acbc6d439f7182980e62d3c79b28edea","observation_id":"5b7a3fc6-fb79-4ffa-9f25-b9c6eec53e79","resolution":{"observed_at":"2026-08-16T00:09:05.493016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10766","last_updated":"2022-07-27T14:04:03Z","snapshot_observed_at":"2026-08-16T16:51:19.975859Z","submitted_at":"2022-06-21T23:05:12Z","title":"Probing high-density nuclear symmetry energy with $\\Xi^{-}/\\Xi^{0}$ ratio in heavy-ion collisions at $\\sqrt{s_{NN}} \\sim 3$ GeV","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.10766","snapshot_observed_at":"2026-08-16T00:09:05.496794Z","title":"Probing the high-density nuclear symmetry energy with the - / 0 ratio in heavy-ion collisions at s_ NN 3 GeV","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.496794Z"},"links":{"cited_paper":"/paper/2206.10766","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:cd6e08e5b526afc95cdb93e747e1fb8173dadfb91db60a2429b19611d3fba1b7","observation_id":"8bccd3d2-30cf-4ae3-9d55-d0f439bb9d41","resolution":{"observed_at":"2026-08-16T00:09:05.496794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/9505016","last_updated":"1995-05-12T02:49:05Z","snapshot_observed_at":"2026-08-04T05:20:01.687796Z","submitted_at":"1995-05-12T02:49:05Z","title":"Formation of superdense hadronic matter in high energy heavy-ion collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/9505016","snapshot_observed_at":"2026-08-16T00:09:05.503407Z","title":"Formation of superdense hadronic matter in high-energy heavy ion collisions","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.503407Z"},"links":{"cited_paper":"/paper/nucl-th/9505016","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:2672d419825feef2a38ae8b6da3442a07ecc42389175d834dc19b42db02f4f56","observation_id":"8b09ce22-fd43-43b3-a1f3-de2385bd74c4","resolution":{"observed_at":"2026-08-16T00:09:05.503407Z","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":"2026-08-16T00:09:05.508566Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.508566Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:eaaa3844662fe0ffbf31e0bb3651463002039f4dd3c3cd47635ec3b88ed57aba","observation_id":"79c0eb98-695e-4e66-a44b-9b2601227333","resolution":{"observed_at":"2026-08-16T00:09:05.508566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00321","last_updated":"2023-04-12T14:54:16Z","snapshot_observed_at":"2026-08-16T16:42:14.291218Z","submitted_at":"2022-07-30T22:56:43Z","title":"Impact of Symmetry Energy on Sound Speed and Spinodal Decomposition in Dense Neutron-Rich Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.00321","snapshot_observed_at":"2026-08-16T00:09:05.512885Z","title":"Impact of symmetry energy on sound speed and spinodal decomposition in dense neutron-rich matter","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.512885Z"},"links":{"cited_paper":"/paper/2208.00321","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:baed077cb1cc99779a3e73d68b00d4e06fa957d90b83c4ba657467c390420381","observation_id":"ebf24581-3d73-46bd-9731-a8e2fd2e7413","resolution":{"observed_at":"2026-08-16T00:09:05.512885Z","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":"2026-08-16T00:09:05.517007Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.517007Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:52f023f1b26c52bbb81d9b36832390ca6f75affa36f0ef02223d3341494f4a23","observation_id":"73f0825a-b962-4b3a-97d4-f0ec3be8ca0b","resolution":{"observed_at":"2026-08-16T00:09:05.517007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/0002065","last_updated":"2000-05-02T18:17:46Z","snapshot_observed_at":"2026-08-16T08:24:34.042906Z","submitted_at":"2000-02-29T19:39:44Z","title":"Effect of Cluster Formation on Isospin Asymmetry in the Liquid-Gas Phase Transition Region","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/0002065","snapshot_observed_at":"2026-08-16T00:09:05.522204Z","title":"and Danielewicz, P","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.522204Z"},"links":{"cited_paper":"/paper/nucl-th/0002065","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:1e73d3e11ccea1b14f0a225405fecde002158eb71495c5a691155ebbbdc8b082","observation_id":"f3afb230-7c28-452a-9834-6d332e72ed1a","resolution":{"observed_at":"2026-08-16T00:09:05.522204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.3580","last_updated":"2008-04-22T17:39:49Z","snapshot_observed_at":"2026-08-15T10:17:03.641521Z","submitted_at":"2008-04-22T17:39:49Z","title":"Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.3580","snapshot_observed_at":"2026-08-16T00:09:05.574005Z","title":"Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.574005Z"},"links":{"cited_paper":"/paper/0804.3580","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:30fbbca6093050c10c20963c1e308a930cc570f8fc4553ce2a14fba1f3a9d8e6","observation_id":"27c4a3d3-1009-4f3e-b82e-a729aff352af","resolution":{"observed_at":"2026-08-16T00:09:05.574005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.18349","last_updated":"2025-04-23T00:53:19Z","snapshot_observed_at":"2026-08-16T10:58:07.901658Z","submitted_at":"2024-11-27T13:52:59Z","title":"High density symmetry energy: A key to the solution of the hyperon puzzle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.18349","snapshot_observed_at":"2026-08-16T00:09:05.578548Z","title":"High-density Symmetry Energy: A Key to the Solution of the Hyperon Puzzle","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.578548Z"},"links":{"cited_paper":"/paper/2411.18349","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:c82c6e1ff21d49f335c898a57ea6a07946e234daae675c61ac56366a335b19f2","observation_id":"b7bf7b59-6a77-4f0f-94ed-4bc44b280bd4","resolution":{"observed_at":"2026-08-16T00:09:05.578548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.09875","last_updated":"2024-04-15T15:47:01Z","snapshot_observed_at":"2026-08-16T14:00:47.204623Z","submitted_at":"2024-04-15T15:47:01Z","title":"The NICER data and a $\\sigma$-field dependent stiffness of the hadronic equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.09875","snapshot_observed_at":"2026-08-16T00:09:05.583154Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.583154Z"},"links":{"cited_paper":"/paper/2404.09875","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:522e4c9eeb8f2937abcbe7198c41e22d722dd8c992b9348719d0ea87f7339f4f","observation_id":"d9061caf-19da-4814-a1a2-df4ce427f986","resolution":{"observed_at":"2026-08-16T00:09:05.583154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.01864","last_updated":"2023-12-19T02:42:03Z","snapshot_observed_at":"2026-08-16T15:03:21.989555Z","submitted_at":"2023-09-04T23:58:28Z","title":"Far-from-equilibrium bulk-viscous transport coefficients in neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.01864","snapshot_observed_at":"2026-08-16T00:09:05.588155Z","title":"Far-from-equilibrium bulk-viscous transport coefficients in neutron star mergers","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.588155Z"},"links":{"cited_paper":"/paper/2309.01864","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:e83cbda8ae8f66c2fb2c929eb05926b264cf103760d9bd2272ab31503fa3b55e","observation_id":"b21c21ce-8d84-4bd4-ab44-f5b8cdc8a300","resolution":{"observed_at":"2026-08-16T00:09:05.588155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06804","last_updated":"2021-07-14T16:04:29Z","snapshot_observed_at":"2026-08-13T07:54:48.786900Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06804","snapshot_observed_at":"2026-08-16T00:09:05.593487Z","title":"and Raithel, Carolyn A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.593487Z"},"links":{"cited_paper":"/paper/2107.06804","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:87f02b0d933573368f40a50d1d4ecef35285feca81cc082d67473ed20c9764f2","observation_id":"ccdc7ea5-b051-45fe-94bb-252cc786ac52","resolution":{"observed_at":"2026-08-16T00:09:05.593487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.18764","last_updated":"2026-04-20T20:15:29Z","snapshot_observed_at":"2026-08-13T11:07:21.903937Z","submitted_at":"2025-04-26T01:56:18Z","title":"Symmetry Energy Expansion with Strange Dense Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.18764","snapshot_observed_at":"2026-08-16T00:09:05.598085Z","title":"Symmetry Energy Expansion with Strange Dense Matter","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.598085Z"},"links":{"cited_paper":"/paper/2504.18764","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0d0af5f5aa6d83cca2927b55e58b6d8bf10e5b652eb37f85e14a5d05ea07d6ba","observation_id":"82381fd5-304e-4a41-948b-2aaf254a2fb8","resolution":{"observed_at":"2026-08-16T00:09:05.598085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.13175","last_updated":"2019-05-29T17:27:56Z","snapshot_observed_at":"2026-08-16T08:19:00.230699Z","submitted_at":"2019-05-29T17:27:56Z","title":"Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.13175","snapshot_observed_at":"2026-08-16T00:09:05.642373Z","title":"and Wen, De-Hua and Zhang, Nai-Bo","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.642373Z"},"links":{"cited_paper":"/paper/1905.13175","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:50977b70e5b0bfa07ee66efcc491fdd5406a3d7d68ae5fd3d1e794dd02acea2d","observation_id":"38f91359-ab3e-4203-96a4-0c9e7623894a","resolution":{"observed_at":"2026-08-16T00:09:05.642373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01213","last_updated":"2018-01-04T00:31:20Z","snapshot_observed_at":"2026-08-14T19:58:10.295344Z","submitted_at":"2018-01-04T00:31:20Z","title":"Nucleon Effective Masses in Neutron-Rich Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01213","snapshot_observed_at":"2026-08-16T00:09:05.747145Z","title":"Nucleon Effective Masses in Neutron-Rich Matter","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.747145Z"},"links":{"cited_paper":"/paper/1801.01213","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:c7a825ab598306c8a1fb2b43919204da43752b0f83fdb27358c107a63cdcb655","observation_id":"a4695099-c544-4fd5-ae51-cfc37c49463b","resolution":{"observed_at":"2026-08-16T00:09:05.747145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.09474","last_updated":"2021-07-19T17:44:10Z","snapshot_observed_at":"2026-08-16T08:20:08.478419Z","submitted_at":"2021-07-19T17:44:10Z","title":"PSR J2222--0137. I. Improved physical parameters for the system","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.09474","snapshot_observed_at":"2026-08-16T00:09:05.790208Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.790208Z"},"links":{"cited_paper":"/paper/2107.09474","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:0c72983ca0dc53539d6fc5be119ed6dd2771d5eef0293e42c7a1e3ae2f6f8349","observation_id":"e0156be1-12f0-4dba-b395-39493a2944b7","resolution":{"observed_at":"2026-08-16T00:09:05.790208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01837","last_updated":"2018-04-10T19:35:45Z","snapshot_observed_at":"2026-08-14T20:00:27.703188Z","submitted_at":"2017-12-24T01:44:26Z","title":"The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01837","snapshot_observed_at":"2026-08-16T00:09:05.795661Z","title":"The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.795661Z"},"links":{"cited_paper":"/paper/1801.01837","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:a0d423a71f970263f9adc308444a1c268949322bddc638d59faa6631da3ce431","observation_id":"93efa1a1-b9a8-4b42-9bd4-71b7c65e820c","resolution":{"observed_at":"2026-08-16T00:09:05.795661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.10438","last_updated":"2019-06-25T10:29:07Z","snapshot_observed_at":"2026-08-13T05:03:27.759835Z","submitted_at":"2019-06-25T10:29:07Z","title":"Thermal X-ray emission identified from the millisecond pulsar PSR J1909-3744","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.10438","snapshot_observed_at":"2026-08-16T00:09:05.799813Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.799813Z"},"links":{"cited_paper":"/paper/1906.10438","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:c45582661f68f0a53f20b742f4b7286fca84dfec3a6b6356cce7ca3d13650542","observation_id":"d79da17e-0176-42c3-9d1e-022bacff07d3","resolution":{"observed_at":"2026-08-16T00:09:05.799813Z","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":"2026-08-16T00:09:05.804983Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.804983Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:5e1a88cd9bb709af313212939310a3240e6904283a2a0c58ff6d7b126d5ae095","observation_id":"3e658cf8-7641-4f5f-850f-afaf2b50c5c0","resolution":{"observed_at":"2026-08-16T00:09:05.804983Z","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":"2026-08-16T00:09:05.809639Z","title":"and others","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.809639Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:786d3513d110c451b7e78607b80f7c2ffe859e00367a25926021e95ef8a2a3f1","observation_id":"d402db1b-0ce9-4e91-8417-4a9dd4c20e89","resolution":{"observed_at":"2026-08-16T00:09:05.809639Z","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":"2026-08-16T00:09:05.848712Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.848712Z"},"links":{"cited_paper":"/paper/1912.05705","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:d7bc456a211bb94af24be6e7f4916f2bb0282dbf8eb8b1857e3d4658675620e9","observation_id":"7aa4156a-6a0b-4d46-a7ca-085bf0690878","resolution":{"observed_at":"2026-08-16T00:09:05.848712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0612440","last_updated":"2006-12-15T17:22:23Z","snapshot_observed_at":"2026-08-15T10:53:27.537169Z","submitted_at":"2006-12-15T17:22:23Z","title":"Neutron Star Observations: Prognosis for Equation of State Constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0612440","snapshot_observed_at":"2026-08-16T00:09:05.868990Z","title":"and Prakash, Maddapa","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.868990Z"},"links":{"cited_paper":"/paper/astro-ph/0612440","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:400ae2a34ef02c0e8064addc936ad131677684a7a33e4b2b87533e856e14531b","observation_id":"a8270474-d351-4f75-97bb-ec551a2b55fa","resolution":{"observed_at":"2026-08-16T00:09:05.868990Z","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":"2026-08-16T00:09:05.874850Z","title":"Astrophys","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.874850Z"},"links":{"citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:bc849149b57473d6252ce0c5e07ec976454e46568fa73fe39ddf8477d7035086","observation_id":"36a0da4e-f716-4f94-b513-01bfe6b7b993","resolution":{"observed_at":"2026-08-16T00:09:05.874850Z","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":"2026-08-15T07:21:13.366969Z","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":"2026-08-16T00:09:05.880262Z","title":"and others","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.880262Z"},"links":{"cited_paper":"/paper/2105.06980","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:cc5a2796e5e048ce447df8c419f97e61d3c94ce1b188a5e970500924749490ec","observation_id":"fa34a150-3b77-465b-b1c4-9d1c4c68032f","resolution":{"observed_at":"2026-08-16T00:09:05.880262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.07155","last_updated":"2018-12-18T03:46:27Z","snapshot_observed_at":"2026-08-16T08:18:54.330573Z","submitted_at":"2018-12-18T03:46:27Z","title":"Influence of Nuclear Reaction Rate Uncertainties on Neutron Star Properties Extracted From X-ray Burst Model-Observation Comparisons","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.07155","snapshot_observed_at":"2026-08-16T00:09:05.885546Z","title":"Influence of Nuclear Reaction Rate Uncertainties on Neutron Star Properties Extracted from X-Ray Burst Model Observation Comparisons","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.885546Z"},"links":{"cited_paper":"/paper/1812.07155","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:2fcebe76a37c55b38531bf57da364e933716da9cd97c0faef51aacaa57acc943","observation_id":"171b7db1-e3f3-4ddd-8c99-3c6c1ef4e1e5","resolution":{"observed_at":"2026-08-16T00:09:05.885546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.0347","last_updated":"2012-02-07T21:00:49Z","snapshot_observed_at":"2026-08-16T08:19:05.888286Z","submitted_at":"2011-11-01T23:52:09Z","title":"Constraints on neutron star mass and radius in GS 1826-24 from sub-Eddington X-ray bursts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.0347","snapshot_observed_at":"2026-08-16T00:09:05.889695Z","title":"Constraints on neutron star mass and radius in GS 1826-24 from sub-Eddington X-ray bursts","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.889695Z"},"links":{"cited_paper":"/paper/1111.0347","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:99e66c577b38de429e13962bfc1dac3a6340911bd22c87d3f5a2987c1f3a11d0","observation_id":"ec49c10b-17d4-482e-9e11-1b7cc97112c0","resolution":{"observed_at":"2026-08-16T00:09:05.889695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0902.0328","last_updated":"2009-02-02T18:08:28Z","snapshot_observed_at":"2026-08-15T05:56:06.935846Z","submitted_at":"2009-02-02T18:08:28Z","title":"Long tails on thermonuclear X-ray bursts from neutron stars: a signature of inward heating?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0902.0328","snapshot_observed_at":"2026-08-16T00:09:05.894680Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.894680Z"},"links":{"cited_paper":"/paper/0902.0328","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:41756aa932b146762cbe532ba6d986bc07122d036190fd53fe1e29e1d0f52c24","observation_id":"932f0641-f5e1-4720-a555-1ab06ccbd069","resolution":{"observed_at":"2026-08-16T00:09:05.894680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.1195","last_updated":"2007-11-08T03:32:19Z","snapshot_observed_at":"2026-08-15T10:28:10.346874Z","submitted_at":"2007-11-08T03:32:19Z","title":"Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.1195","snapshot_observed_at":"2026-08-16T00:09:05.932349Z","title":"and Woosley, Stanford E","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:05.932349Z"},"links":{"cited_paper":"/paper/0711.1195","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:221eea381400ea43acaf3a206fa47e6fa0feef44f6c1c7b14aa0f5ed4c6f9f27","observation_id":"9416a6d8-f440-4095-a126-3d32a4fdf2c3","resolution":{"observed_at":"2026-08-16T00:09:05.932349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0308122","last_updated":"2003-10-02T20:03:11Z","snapshot_observed_at":"2026-08-16T08:23:46.715980Z","submitted_at":"2003-08-07T16:00:52Z","title":"Periodic Thermonuclear X-ray Bursts from GS 1826-24 and the Fuel Composition as a Function of Accretion Rate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0308122","snapshot_observed_at":"2026-08-16T00:09:06.040583Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:06.040583Z"},"links":{"cited_paper":"/paper/astro-ph/0308122","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:da5656d8d445484fbd11bf4f202bd171a34d2e876f788433bea35e5c2870b7b1","observation_id":"e793d47c-8b9a-462d-b700-c7c6138102c2","resolution":{"observed_at":"2026-08-16T00:09:06.040583Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T17:10:36.676883Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":2,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":96,"verified_exact":2,"verified_fuzzy":0},"total_outbound_references":296},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 296 outbound references and 0 inbound Pith citation observations for arXiv:2608.12632."}