{"as_of":"2026-08-13T01:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ac90f49242d28f5fcae0e9bc6a8be5b484659d52529553c559879e9c9da5882f","coverage":[{"denominator":97,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":97,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T11:39:46.791237Z","state":"measured"},{"denominator":98,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":98,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-25T20:27:04.894292Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T20:20:06.716801Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"cited_work":{"arxiv_id":"2411.18052","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.18052","snapshot_observed_at":"2026-07-04T20:20:06.716801Z","title":"Heating the dark matter halo with dark radiation from supernovae,","venue":null,"work_id":"4937b5a5-44a2-4f63-b298-9a23e282b915","year":2025},"citing_paper":{"arxiv_id":"2606.25779","last_updated":"2026-06-24T12:56:46Z","snapshot_observed_at":"2026-07-07T00:00:12.737052Z","submitted_at":"2026-06-24T12:56:46Z","title":"Dark Photons from Red Dwarfs","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-25T20:27:04.894292Z"},"links":{"cited_paper":"/paper/2411.18052","citing_paper":"/paper/2606.25779"},"observation_digest":"sha256:163353435d7c3b977cc5115ce34c6c09da746c24991ede88924d3d4faebc1af6","observation_id":"ea7aa4a5-3a58-4de8-98fd-a2268f285619","resolution":{"observed_at":"2026-07-04T20:20:06.718675Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2411.18052/citation-record","integrity":"/paper/2411.18052/integrity","json":"/paper/2411.18052/citation-record.json","paper":"/paper/2411.18052"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T11:39:46.355719Z","title":"Astrophysical methods to constrain axions and other novel particle phenomena,","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.355719Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:257c954c2c7fc77fddbe648b501ffcc46e28449c827c775ce7213fbcd8708bb8","observation_id":"bd8b6b80-086c-454f-b130-2614417b10ba","resolution":{"observed_at":"2026-08-12T11:39:46.355719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.13728","last_updated":"2024-03-12T17:38:28Z","snapshot_observed_at":"2026-08-03T18:36:38.003151Z","submitted_at":"2024-01-24T19:00:00Z","title":"Astrophysical Axion Bounds: The 2024 Edition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.13728","snapshot_observed_at":"2026-08-12T11:39:46.361730Z","title":"Astrophysical Axion Bounds: The 2024 Edition,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.361730Z"},"links":{"cited_paper":"/paper/2401.13728","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:95d4b893a3cf0641c00d8eb90a254f13a8781919894f74aeb13c14a8d9488b9e","observation_id":"1de72a07-48b3-4e51-bbab-e70838a1dbad","resolution":{"observed_at":"2026-08-12T11:39:46.361730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0612072","last_updated":"2006-12-04T19:06:43Z","snapshot_observed_at":"2026-07-07T01:05:07.664736Z","submitted_at":"2006-12-04T19:06:43Z","title":"Theory of Core-Collapse Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0612072","snapshot_observed_at":"2026-08-12T11:39:46.366171Z","title":"Theory of core-collapse supernovae,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.366171Z"},"links":{"cited_paper":"/paper/astro-ph/0612072","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:6865a8f4bf7e845121147a0747b7ec622b6d0639cb0bbd66e8a7c7a9423de3d1","observation_id":"123573fb-ab11-48c3-9cd7-655659cb59c5","resolution":{"observed_at":"2026-08-12T11:39:46.366171Z","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":"2026-08-12T11:39:46.371059Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.371059Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:bfac218f0f9773c506429dda0df253a5895818fb6882abea2497d3a00705824d","observation_id":"f06212e9-e266-44f9-afc5-e751421b9f63","resolution":{"observed_at":"2026-08-12T11:39:46.371059Z","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":"2026-08-12T11:39:46.376159Z","title":"Bounds on Exotic Particle Interactions from SN 1987a,","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.376159Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:afe58e5937ad86c79bf1c1ec098284db72819afca2102e18a73ac76855f40dfa","observation_id":"d14ccab6-1ffd-4cb0-897c-18beb1ef70d0","resolution":{"observed_at":"2026-08-12T11:39:46.376159Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9702372","last_updated":"1997-03-11T14:08:45Z","snapshot_observed_at":"2026-07-07T04:25:04.682130Z","submitted_at":"1997-02-19T21:34:13Z","title":"Supernova Bounds on Resonant Active-Sterile Neutrino Conversions","version":2},"cited_work":{"arxiv_id":"hep-ph/9702372","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9702372","snapshot_observed_at":"2026-08-12T11:39:48.105508Z","title":"Supernova Bounds on Resonant Active-Sterile Neutrino Conversions","venue":"hep-ph","work_id":"d6beeb6e-f153-4d85-b062-394963298599","year":1997},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.381215Z"},"links":{"cited_paper":"/paper/hep-ph/9702372","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:a792f4d0dece8546220e23a04673cd472674615667c40d51803bd94d49412931","observation_id":"69fb157e-f0ef-4aed-a320-6ba67c735fbd","resolution":{"observed_at":"2026-08-12T11:39:48.110387Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1102.5124","last_updated":"2011-05-26T15:43:46Z","snapshot_observed_at":"2026-07-06T02:24:02.340187Z","submitted_at":"2011-02-24T22:54:29Z","title":"Supernova bound on keV-mass sterile neutrinos reexamined","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.5124","snapshot_observed_at":"2026-08-12T11:39:46.386837Z","title":"Supernova bound on keV-mass sterile neutrinos reexamined,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.386837Z"},"links":{"cited_paper":"/paper/1102.5124","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:da884ade8fd83f6cdd583fe1250791287d0c2ea434a1b4c603d3544ffc045ea5","observation_id":"522e42f8-dabf-4adc-a0e2-00a7240e87f3","resolution":{"observed_at":"2026-08-12T11:39:46.386837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.00654","last_updated":"2019-03-03T19:27:50Z","snapshot_observed_at":"2026-08-08T23:10:13.152945Z","submitted_at":"2016-05-02T20:00:04Z","title":"Production of keV Sterile Neutrinos in Supernovae: New Constraints and Gamma Ray Observables","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.00654","snapshot_observed_at":"2026-08-12T11:39:46.392196Z","title":"Production of keV Sterile Neutrinos in Supernovae: New Constraints and Gamma Ray Observables,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.392196Z"},"links":{"cited_paper":"/paper/1605.00654","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:1f4297e93225eb197f351004dbffb460b131703b48df96ff915b1c85f7313b7d","observation_id":"c6af5a4b-a43e-445f-b1e5-4ccb1bef9978","resolution":{"observed_at":"2026-08-12T11:39:46.392196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10965","last_updated":"2023-04-21T15:09:38Z","snapshot_observed_at":"2026-08-11T00:02:53.354210Z","submitted_at":"2023-02-21T19:49:43Z","title":"The Neutrino Magnetic Moment Portal and Supernovae: New Constraints and Multimessenger Opportunities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10965","snapshot_observed_at":"2026-08-12T11:39:46.396916Z","title":"Neutrino magnetic moment portal and supernovae: New constraints and multimessenger opportunities,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.396916Z"},"links":{"cited_paper":"/paper/2302.10965","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5fcbd7704485d3124b7c345d94de15ded9719d0ecb6952168207b26659ea9133","observation_id":"3974e5f8-7548-4712-afde-51f62808fcb3","resolution":{"observed_at":"2026-08-12T11:39:46.396916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00033","last_updated":"2024-03-10T10:21:32Z","snapshot_observed_at":"2026-07-06T16:41:19.189036Z","submitted_at":"2023-10-31T18:00:02Z","title":"Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00033","snapshot_observed_at":"2026-08-12T11:39:46.401379Z","title":"Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.401379Z"},"links":{"cited_paper":"/paper/2311.00033","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:998ec1bbe7e68855dcbb76505c56ee35a95488f154c74021136a1fb1f1d56764","observation_id":"fe2bde31-7a35-470e-9a38-eae3aea24742","resolution":{"observed_at":"2026-08-12T11:39:46.401379Z","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":"2026-08-12T11:39:46.405807Z","title":"Axions from SN 1987a,","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.405807Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:c2f2b515fe6da3031fee509d1225a3975e1b063aeb267f279d117f14a98d01a0","observation_id":"b8abc380-c0c3-4fb2-b34d-2eb0b3989a08","resolution":{"observed_at":"2026-08-12T11:39:46.405807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00993","last_updated":"2018-09-17T04:50:13Z","snapshot_observed_at":"2026-07-06T06:26:20.207918Z","submitted_at":"2018-03-02T18:46:17Z","title":"Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00993","snapshot_observed_at":"2026-08-12T11:39:46.410254Z","title":"Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.410254Z"},"links":{"cited_paper":"/paper/1803.00993","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:d5856b34b4b3e3b8b158c61b20d9ca000da4fe75269530f45d49ae19f377e591","observation_id":"be01bb22-0d39-4771-85c7-fdbcf6be0b67","resolution":{"observed_at":"2026-08-12T11:39:46.410254Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11844","last_updated":"2020-05-28T08:44:29Z","snapshot_observed_at":"2026-08-09T16:31:24.809097Z","submitted_at":"2019-06-27T18:00:03Z","title":"Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11844","snapshot_observed_at":"2026-08-12T11:39:46.414578Z","title":"Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.414578Z"},"links":{"cited_paper":"/paper/1906.11844","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:cfbdffae1c6486c49d10ed48961f923168be40edca945979379e2ca267b022f5","observation_id":"dcfc45b2-9144-4cc9-9ceb-b4176e7de29e","resolution":{"observed_at":"2026-08-12T11:39:46.414578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-08-12T11:39:46.418714Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.418714Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:7d9ead7e507b3b93b8e877c0975c34f745b3faf464b5778e30c12288bd6197be","observation_id":"300f1ffe-2951-4f3f-a457-9ee18e75f5f3","resolution":{"observed_at":"2026-08-12T11:39:46.418714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.19902","last_updated":"2025-09-11T22:25:55Z","snapshot_observed_at":"2026-08-12T22:14:56.464848Z","submitted_at":"2024-10-25T18:00:00Z","title":"A Universal Bound on QCD Axions from Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.19902","snapshot_observed_at":"2026-08-12T11:39:46.423874Z","title":"A Universal Bound on QCD Axions from Supernovae,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.423874Z"},"links":{"cited_paper":"/paper/2410.19902","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:91298f7852e4575dd9c30be2c60eb7781bbe455bd8e226d067961e5ec7288e7e","observation_id":"3ee3ea88-6c9f-425a-b54f-f221b343fed3","resolution":{"observed_at":"2026-08-12T11:39:46.423874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.02492","last_updated":"2025-02-26T20:20:46Z","snapshot_observed_at":"2026-08-12T22:07:57.398481Z","submitted_at":"2024-11-04T19:00:01Z","title":"Axion Astrophysics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.02492","snapshot_observed_at":"2026-08-12T11:39:46.428685Z","title":"Axion Astrophysics,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.428685Z"},"links":{"cited_paper":"/paper/2411.02492","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:3ceb38f20d0f88710ef6079a91dd9c798ba2d2f94ef6f3eeb4800d5636ad19f0","observation_id":"3ff8b903-f0fc-42e8-b01e-a3395b030195","resolution":{"observed_at":"2026-08-12T11:39:46.428685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2683","last_updated":"2012-01-12T21:01:29Z","snapshot_observed_at":"2026-08-10T08:24:57.390468Z","submitted_at":"2012-01-12T21:01:29Z","title":"Constraints on Light Hidden Sector Gauge Bosons from Supernova Cooling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2683","snapshot_observed_at":"2026-08-12T11:39:46.432683Z","title":"Constraints on Light Hidden Sector Gauge Bosons from Supernova Cooling,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.432683Z"},"links":{"cited_paper":"/paper/1201.2683","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:6ed19a0ce56a544ff3101c62f7b6010659b10ebbac87e1837da85ab9aa8e9447","observation_id":"05739ef3-f8a5-4aba-9308-70b007c98c5c","resolution":{"observed_at":"2026-08-12T11:39:46.432683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.0221","last_updated":"2014-11-07T18:44:19Z","snapshot_observed_at":"2026-08-10T02:48:33.115682Z","submitted_at":"2014-10-01T13:45:46Z","title":"Supernova Bounds on the Dark Photon Using its Electromagnetic Decay","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.0221","snapshot_observed_at":"2026-08-12T11:39:46.436797Z","title":"Supernova Bounds on the Dark Photon Using its Electromagnetic Decay,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.436797Z"},"links":{"cited_paper":"/paper/1410.0221","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:846b13c9bb9a0d9bbbe0400db4b035f7524a16ef90e8e65437ec17e35bdb1e81","observation_id":"58545d4c-a35e-473e-80a1-8b49344f865d","resolution":{"observed_at":"2026-08-12T11:39:46.436797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.03864","last_updated":"2019-05-31T21:23:15Z","snapshot_observed_at":"2026-08-10T11:53:56.212491Z","submitted_at":"2016-11-11T21:00:00Z","title":"Revisiting Supernova 1987A Constraints on Dark Photons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.03864","snapshot_observed_at":"2026-08-12T11:39:46.440614Z","title":"Revisiting Supernova 1987A Constraints on Dark Photons,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.440614Z"},"links":{"cited_paper":"/paper/1611.03864","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:a77c6cb4ac44e12fbce9bfd27584eaa3e579ca52b509ce45d2e4bb6b8e5a68e8","observation_id":"ad12b05d-dbcb-4bf1-89d8-d88f706a6480","resolution":{"observed_at":"2026-08-12T11:39:46.440614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07923","last_updated":"2019-09-02T09:31:16Z","snapshot_observed_at":"2026-08-11T18:11:19.350169Z","submitted_at":"2019-03-19T10:32:23Z","title":"New constraint from supernova explosions on light particles beyond the Standard Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07923","snapshot_observed_at":"2026-08-12T11:39:46.444818Z","title":"New constraint from supernova explosions on light particles beyond the Standard Model,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.444818Z"},"links":{"cited_paper":"/paper/1903.07923","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:2bd6da6c55e48e497af5816471a2ceb44aa06398a17be1f649558ec0144973db","observation_id":"d612e2c2-9ffa-4f95-91e0-9f39870245f5","resolution":{"observed_at":"2026-08-12T11:39:46.444818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13942","last_updated":"2020-06-30T12:55:46Z","snapshot_observed_at":"2026-08-08T16:44:16.293476Z","submitted_at":"2020-06-24T18:00:01Z","title":"Supernova Muons: New Constraints on Z' Bosons, Axions, and ALPs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13942","snapshot_observed_at":"2026-08-12T11:39:46.449197Z","title":"Supernova Muons: New Constraints on Z’ Bosons, Axions and ALPs,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.449197Z"},"links":{"cited_paper":"/paper/2006.13942","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:cfe994249acc7bb8731b23398071f6a34c7e27dcd931994c725cc914a4630a23","observation_id":"df531e32-a600-486a-b89d-bf7a65d94d18","resolution":{"observed_at":"2026-08-12T11:39:46.449197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.05427","last_updated":"2021-04-29T09:03:31Z","snapshot_observed_at":"2026-08-08T04:14:14.729955Z","submitted_at":"2020-12-10T02:55:11Z","title":"Cooling of young neutron stars and dark gauge bosons","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.05427","snapshot_observed_at":"2026-08-12T11:39:46.453485Z","title":"Cooling of young neutron stars and dark gauge bosons,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.453485Z"},"links":{"cited_paper":"/paper/2012.05427","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:808e9807df144141a68a55835acf9847c17920d1e76c7a425e532ede7ea7c76c","observation_id":"2a500099-17b8-418f-ac7b-5353c2731515","resolution":{"observed_at":"2026-08-12T11:39:46.453485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.03362","last_updated":"2022-02-16T14:39:20Z","snapshot_observed_at":"2026-08-10T14:06:13.273513Z","submitted_at":"2021-10-07T12:00:15Z","title":"Dark gauge boson production from neutron stars via nucleon-nucleon bremsstrahlung","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.03362","snapshot_observed_at":"2026-08-12T11:39:46.457728Z","title":"Dark gauge boson production from neutron stars via nucleon-nucleon bremsstrahlung,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.457728Z"},"links":{"cited_paper":"/paper/2110.03362","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:199d528eb77d488f7d8af8cbebafd34c46d2a8e7a3330cba43a5e9e6e52b0ff6","observation_id":"cde6760c-5f1b-43ec-a6a3-3326306a27f6","resolution":{"observed_at":"2026-08-12T11:39:46.457728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.15677","last_updated":"2023-09-07T14:45:50Z","snapshot_observed_at":"2026-08-02T18:00:42.203501Z","submitted_at":"2022-11-28T19:00:00Z","title":"Dark gauge boson emission from supernova pions","version":2},"cited_work":{"arxiv_id":"2211.15677","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.15677","snapshot_observed_at":"2026-08-12T11:39:47.873774Z","title":"Dark gauge boson emission from supernova pions","venue":"hep-ph","work_id":"9102de7a-3d79-40d4-9011-cc68186b2107","year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.462173Z"},"links":{"cited_paper":"/paper/2211.15677","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:23c6e349ecb4865dad30599f0c8ba77f11c9e292196f436a927628b2fe880078","observation_id":"f98b0fd7-2485-49e5-891b-79f228251ccf","resolution":{"observed_at":"2026-08-12T11:39:47.878104Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1511.09136","last_updated":"2016-02-03T17:50:18Z","snapshot_observed_at":"2026-08-07T08:19:52.166501Z","submitted_at":"2015-11-30T02:25:57Z","title":"Nucleon-nucleon bremsstrahlung of dark gauge bosons and revised supernova constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.09136","snapshot_observed_at":"2026-08-12T11:39:46.466033Z","title":"Nucleon-nucleon bremsstrahlung of dark gauge bosons and revised supernova constraints,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.466033Z"},"links":{"cited_paper":"/paper/1511.09136","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:9a7355dd00087fc61146c63214ea0a975bbc5508cca6d1d6e229d0c64e3241f4","observation_id":"e1201966-5a76-4e9d-9606-ab220dcebc9e","resolution":{"observed_at":"2026-08-12T11:39:46.466033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.04119","last_updated":"2016-11-01T19:47:53Z","snapshot_observed_at":"2026-08-12T14:50:07.179624Z","submitted_at":"2015-12-13T21:00:21Z","title":"Probing Light Thermal Dark-Matter With a Higgs Portal Mediator","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.04119","snapshot_observed_at":"2026-08-12T11:39:46.470122Z","title":"Probing Light Thermal Dark-Matter With a Higgs Portal Mediator,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.470122Z"},"links":{"cited_paper":"/paper/1512.04119","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5a8f5ae5d0ce764dd848ab0969906abc5009ebc675183106c3f1acd80410ce91","observation_id":"af3cc787-c426-4ab8-9d45-e6a53b8f9032","resolution":{"observed_at":"2026-08-12T11:39:46.470122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.05852","last_updated":"2017-02-08T05:49:09Z","snapshot_observed_at":"2026-08-06T11:34:08.724405Z","submitted_at":"2016-11-17T20:47:41Z","title":"Stellar cooling bounds on new light particles: plasma mixing effects","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.05852","snapshot_observed_at":"2026-08-12T11:39:46.474411Z","title":"Stellar cooling bounds on new light particles: plasma mixing effects,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.474411Z"},"links":{"cited_paper":"/paper/1611.05852","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:1ffaa29cc3052f6ba785e5b4e5ca37e05cdc91f052f298676fbd386520fc21eb","observation_id":"8db7bd04-3dce-4430-83d7-ef5995bb6c44","resolution":{"observed_at":"2026-08-12T11:39:46.474411Z","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":"2026-08-12T11:39:46.478853Z","title":"Supernova bounds on new scalars from resonant and soft emission,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.478853Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:8cdc12cf29c888fa036b6adba96d9706ed7f0fb83ba7d224d30bf7b8d0774bd9","observation_id":"3e31fb95-8a8d-4767-a6e6-e1c4f1f5d29c","resolution":{"observed_at":"2026-08-12T11:39:46.478853Z","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":"2026-08-12T11:39:46.482844Z","title":"Majorons and Supernova Cooling,","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.482844Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5e25061aa1bda7f1b582cc1ac9d67be572249fe1e2de9998ca02dc86523e2ed0","observation_id":"13bff160-68c0-4280-aebb-ffa0bbce1d3e","resolution":{"observed_at":"2026-08-12T11:39:46.482844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05882","last_updated":"2017-02-22T13:13:42Z","snapshot_observed_at":"2026-08-06T19:35:23.750334Z","submitted_at":"2016-09-19T19:45:45Z","title":"Supernova Constraints on Massive (Pseudo)Scalar Coupling to Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.05882","snapshot_observed_at":"2026-08-12T11:39:46.486543Z","title":"Supernova Constraints on Massive (Pseudo)Scalar Coupling to Neutrinos,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.486543Z"},"links":{"cited_paper":"/paper/1609.05882","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:f0adb6d20f297f587c572ea5cf29c21fd7b2e285661d98af4d4c3a1412b6e085","observation_id":"4e64c078-e366-43f8-92b2-898df073f827","resolution":{"observed_at":"2026-08-12T11:39:46.486543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00553","last_updated":"2019-10-07T09:34:20Z","snapshot_observed_at":"2026-07-06T08:11:51.384595Z","submitted_at":"2019-08-01T18:00:15Z","title":"Stellar probes of dark sector-photon interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00553","snapshot_observed_at":"2026-08-12T11:39:46.491379Z","title":"Stellar probes of dark sector-photon interactions,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.491379Z"},"links":{"cited_paper":"/paper/1908.00553","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:10bb23e581f79bcfa79078e0d348e748e4833c836a7039fc2faa144d47220e4d","observation_id":"2cc104ee-eac9-4bd9-a0b3-3e36bfc13c6f","resolution":{"observed_at":"2026-08-12T11:39:46.491379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.07141","last_updated":"2024-05-31T21:48:35Z","snapshot_observed_at":"2026-08-08T10:39:28.689464Z","submitted_at":"2020-05-14T17:00:30Z","title":"Muons in supernovae: implications for the axion-muon coupling","version":7},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.07141","snapshot_observed_at":"2026-08-12T11:39:46.496751Z","title":"Muons in Supernovae: Implications for the Axion-Muon Coupling,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.496751Z"},"links":{"cited_paper":"/paper/2005.07141","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:1bffbd09bc3b66587b769ade6da3b2b8023e5e21bc5a54e50d4fdbce263e90e7","observation_id":"ca7eb1dd-d659-431e-b024-18072ed25872","resolution":{"observed_at":"2026-08-12T11:39:46.496751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.00490","last_updated":"2020-09-23T03:58:54Z","snapshot_observed_at":"2026-08-10T14:03:57.913608Z","submitted_at":"2020-05-01T17:05:27Z","title":"Revisiting supernova constraints on a light CP-even scalar","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.00490","snapshot_observed_at":"2026-08-12T11:39:46.501614Z","title":"Revisiting supernova constraints on a light CP-even scalar,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.501614Z"},"links":{"cited_paper":"/paper/2005.00490","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:0517634d4dbcedf489035d131b605b11352c14d956e03a026073921c09ab702c","observation_id":"f7ff77ed-fa90-4b1d-b13f-5cc2d8d755aa","resolution":{"observed_at":"2026-08-12T11:39:46.501614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.11632","last_updated":"2022-03-07T11:00:09Z","snapshot_observed_at":"2026-08-08T03:43:42.365655Z","submitted_at":"2020-12-21T19:00:52Z","title":"Supernova Constraints on Dark Flavored Sectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.11632","snapshot_observed_at":"2026-08-12T11:39:46.506461Z","title":"Supernova Constraints on Dark Flavored Sectors,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.506461Z"},"links":{"cited_paper":"/paper/2012.11632","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:c777a4aa59dd52a10ef29f7ea0b9b6fa4e4b24809c1e6edede52752bf6e13408","observation_id":"6abf988e-687a-416c-ad61-07933ef48605","resolution":{"observed_at":"2026-08-12T11:39:46.506461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.03244","last_updated":"2026-04-03T12:28:24Z","snapshot_observed_at":"2026-08-08T14:23:34.396873Z","submitted_at":"2021-09-07T18:00:00Z","title":"Muonic Boson Limits: Supernova Redux","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.03244","snapshot_observed_at":"2026-08-12T11:39:46.510433Z","title":"Muonic boson limits: Supernova redux,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.510433Z"},"links":{"cited_paper":"/paper/2109.03244","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:b202cf896ab59d50535aeb65d9d1f65722646cd9fd6031be0ef07321be532636","observation_id":"2711ee9b-7988-4d3e-8670-38275325178f","resolution":{"observed_at":"2026-08-12T11:39:46.510433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.11773","last_updated":"2023-07-15T14:48:22Z","snapshot_observed_at":"2026-08-11T13:07:02.812132Z","submitted_at":"2022-09-23T18:00:00Z","title":"Strong Supernova 1987A Constraints on Bosons Decaying to Neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.11773","snapshot_observed_at":"2026-08-12T11:39:46.514333Z","title":"Strong Supernova 1987A Constraints on Bosons Decaying to Neutrinos,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.514333Z"},"links":{"cited_paper":"/paper/2209.11773","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:1d180b22586ada83ccf37e784067a5e43b821fdf83be7978cb67b6cc47d51157","observation_id":"f2c2817e-213e-4953-800a-1d60fc3f3e55","resolution":{"observed_at":"2026-08-12T11:39:46.514333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.06852","last_updated":"2022-12-12T09:06:52Z","snapshot_observed_at":"2026-07-06T13:20:40.919352Z","submitted_at":"2022-06-14T13:45:27Z","title":"Probing non-standard neutrino interactions with a light boson from next galactic and diffuse supernova neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.06852","snapshot_observed_at":"2026-08-12T11:39:46.518866Z","title":"Probing non-standard neutrino interactions with a light boson from next galactic and diffuse supernova neutrinos,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.518866Z"},"links":{"cited_paper":"/paper/2206.06852","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:88352bedf6e0aa3be2dabe17cdbac360ff20995ce75afa987c68d60ca754b9e6","observation_id":"5ddb7eec-102e-4a5d-b368-1f72a7b41d3f","resolution":{"observed_at":"2026-08-12T11:39:46.518866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.13627","last_updated":"2024-07-10T18:47:38Z","snapshot_observed_at":"2026-08-11T07:10:03.224813Z","submitted_at":"2023-12-21T07:38:24Z","title":"Limits on heavy neutral leptons, $Z'$ bosons and majorons from high-energy supernova neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.13627","snapshot_observed_at":"2026-08-12T11:39:46.523840Z","title":"Limits on heavy neutral leptons, Z ′ bosons and majorons from high-energy supernova neutrinos,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.523840Z"},"links":{"cited_paper":"/paper/2312.13627","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:ccde834843f75efe457651b21c46ce40f87d190c03ecd93e1ca8a805307b80fe","observation_id":"f208a8b3-0d56-42f2-ab02-1579d4ccf12f","resolution":{"observed_at":"2026-08-12T11:39:46.523840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.12676","last_updated":"2022-11-29T15:14:51Z","snapshot_observed_at":"2026-07-06T13:24:34.692661Z","submitted_at":"2022-06-25T15:55:01Z","title":"Chiral $Z^\\prime$ in FASER, FASER2, DUNE, and ILC beam dump experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.12676","snapshot_observed_at":"2026-08-12T11:39:46.528440Z","title":"Chiral Z’ in F ASER, F ASER2, DUNE, and ILC beam dump experiments,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.528440Z"},"links":{"cited_paper":"/paper/2206.12676","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:cb09efceec1e8e7eae372736c063608c8000b665697f1208a0d83642d3afc91b","observation_id":"fc12f02a-7573-40ec-84e4-f6637bede6da","resolution":{"observed_at":"2026-08-12T11:39:46.528440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15122","last_updated":"2024-01-11T16:14:26Z","snapshot_observed_at":"2026-08-10T02:10:18.091486Z","submitted_at":"2023-07-27T18:00:06Z","title":"Supernova Emission of Secretly Interacting Neutrino Fluid: Theoretical Foundations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15122","snapshot_observed_at":"2026-08-12T11:39:46.533154Z","title":"Supernova emission of secretly interacting neutrino fluid: Theoretical foundations,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.533154Z"},"links":{"cited_paper":"/paper/2307.15122","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:fbc006c99b1d91c5e8dbfd41ea249e94ef51a89fe55842f169a4f4f33221fdd8","observation_id":"4e7a5e2a-6db0-4151-b0ec-de42c5f0e494","resolution":{"observed_at":"2026-08-12T11:39:46.533154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03143","last_updated":"2023-10-12T20:16:51Z","snapshot_observed_at":"2026-08-10T14:23:08.192545Z","submitted_at":"2023-07-06T17:11:28Z","title":"Supernova Limits on Muonic Dark Forces","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03143","snapshot_observed_at":"2026-08-12T11:39:46.538179Z","title":"Supernova limits on muonic dark forces,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.538179Z"},"links":{"cited_paper":"/paper/2307.03143","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:227a7a4754a439e6339b77dffedd64c74a832259ca2a4fca22320e8855aec741","observation_id":"108b5b31-0eb2-4b5e-817c-c62738e4b40d","resolution":{"observed_at":"2026-08-12T11:39:46.538179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15115","last_updated":"2024-01-11T16:22:02Z","snapshot_observed_at":"2026-08-09T19:32:12.828417Z","submitted_at":"2023-07-27T18:00:02Z","title":"Large Neutrino Secret Interactions, Small Impact on Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15115","snapshot_observed_at":"2026-08-12T11:39:46.542863Z","title":"Large Neutrino Secret Interactions Have a Small Impact on Supernovae,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.542863Z"},"links":{"cited_paper":"/paper/2307.15115","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:50d38674fc5e0f28b6fef6d000a8789915353b59f8959cabe7a23d08177035aa","observation_id":"4e56788b-ad60-4094-8cb8-7675f7da4c5a","resolution":{"observed_at":"2026-08-12T11:39:46.542863Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.09781","last_updated":"2025-06-12T16:37:25Z","snapshot_observed_at":"2026-08-13T00:54:01.064765Z","submitted_at":"2024-03-14T18:02:44Z","title":"Supernovae Time Profiles as a Probe of New Physics at Neutrino Telescopes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.09781","snapshot_observed_at":"2026-08-12T11:39:46.547834Z","title":"Supernovae Time Profiles as a Probe of New Physics at Neutrino Telescopes,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.547834Z"},"links":{"cited_paper":"/paper/2403.09781","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:9c3319b54e09be8278fa5b9c0839daf84b931877bf884f4785af3d929b5a88c7","observation_id":"f0019047-294a-43ec-9860-549ec0a0c837","resolution":{"observed_at":"2026-08-12T11:39:46.547834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.15506","last_updated":"2024-06-19T18:00:15Z","snapshot_observed_at":"2026-08-12T23:38:59.125881Z","submitted_at":"2024-06-19T18:00:15Z","title":"The next galactic supernova can uncover mass and couplings of particles decaying to neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.15506","snapshot_observed_at":"2026-08-12T11:39:46.553754Z","title":"The next galactic supernova can uncover mass and couplings of particles decaying to neutrinos,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.553754Z"},"links":{"cited_paper":"/paper/2406.15506","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5eebebf4fb9d93f97a39d11d31de9793b2538a5a10addc717a73c02948591246","observation_id":"403810d8-bafa-4f6e-ba54-9895ec4b545a","resolution":{"observed_at":"2026-08-12T11:39:46.553754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07714","last_updated":"2025-01-07T05:05:12Z","snapshot_observed_at":"2026-08-13T00:32:42.876774Z","submitted_at":"2024-04-11T13:04:14Z","title":"Self-Interacting Dark Sectors in Supernovae Can Behave as a Relativistic Fluid","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07714","snapshot_observed_at":"2026-08-12T11:39:46.558566Z","title":"Self-interacting dark sectors in supernovae are fluid,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.558566Z"},"links":{"cited_paper":"/paper/2404.07714","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:54d2f1d8a06394459fabf6ceb84ecd33d136ad1f9b2b3268cdc665c851f74f00","observation_id":"0534d37f-7534-4496-bee3-e3dca4870d10","resolution":{"observed_at":"2026-08-12T11:39:46.558566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611107","last_updated":"1997-10-21T23:14:37Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-13T22:59:55Z","title":"A Universal Density Profile from Hierarchical Clustering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611107","snapshot_observed_at":"2026-08-12T11:39:46.562567Z","title":"A Universal density profile from hierarchical clustering,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.562567Z"},"links":{"cited_paper":"/paper/astro-ph/9611107","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:8a02166c85194221962c719884d251929c70a30e9d348e2a3c423c96a9a28b84","observation_id":"73c7365c-936a-49c4-8534-d6b53071d1df","resolution":{"observed_at":"2026-08-12T11:39:46.562567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.04256","last_updated":"2019-09-02T22:12:33Z","snapshot_observed_at":"2026-08-12T15:52:42.048317Z","submitted_at":"2017-07-13T18:00:00Z","title":"Small-Scale Challenges to the $\\Lambda$CDM Paradigm","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.04256","snapshot_observed_at":"2026-08-12T11:39:46.566576Z","title":"Small-Scale Challenges to the ΛCDM Paradigm,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.566576Z"},"links":{"cited_paper":"/paper/1707.04256","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:177c31bacb3452234fee4b1721bd4629cfae9686541a0bc64927e8b40103368a","observation_id":"ed01a36a-c265-44af-8a43-6ae019fbfc60","resolution":{"observed_at":"2026-08-12T11:39:46.566576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.2772","last_updated":"2012-09-19T17:08:09Z","snapshot_observed_at":"2026-07-06T02:51:41.118939Z","submitted_at":"2012-07-11T20:01:52Z","title":"The coupling between the core/cusp and missing satellite problems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.2772","snapshot_observed_at":"2026-08-12T11:39:46.570627Z","title":"The coupling between the core/cusp and missing satellite problems,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.570627Z"},"links":{"cited_paper":"/paper/1207.2772","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:57a94c1726b6cecd4d6bf86a537eceaf42d4f59eb4dad30b5637268ce372cfca","observation_id":"8e9a5b67-c0d2-491d-9fd5-068e344d8f70","resolution":{"observed_at":"2026-08-12T11:39:46.570627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.08718","last_updated":"2024-07-08T14:52:21Z","snapshot_observed_at":"2026-08-09T03:02:36.655282Z","submitted_at":"2024-02-13T19:00:01Z","title":"Constraining neutrino-DM interactions with Milky Way dwarf spheroidals and supernova neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.08718","snapshot_observed_at":"2026-08-12T11:39:46.575124Z","title":"Constraining neutrino-DM interactions with Milky Way dwarf spheroidals and supernova neutrinos,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.575124Z"},"links":{"cited_paper":"/paper/2402.08718","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:a6c9c984009006bc4b3f2a81e5569b62a366ffe4d8b35db9abcd6dab541732df","observation_id":"c0663388-7c3c-46c7-a199-64d4a1cd91dc","resolution":{"observed_at":"2026-08-12T11:39:46.575124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.06634","last_updated":"2019-04-11T19:33:13Z","snapshot_observed_at":"2026-08-10T08:49:13.729482Z","submitted_at":"2018-08-20T18:09:34Z","title":"Dark matter heats up in dwarf galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.06634","snapshot_observed_at":"2026-08-12T11:39:46.579905Z","title":"Dark matter heats up in dwarf galaxies,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.579905Z"},"links":{"cited_paper":"/paper/1808.06634","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5e9bf48855640cb1dbef3bb188af33156c21ee1ec85697efd85138c6588a18b6","observation_id":"17c1c91b-74d7-4866-b610-e33c4b5c3d79","resolution":{"observed_at":"2026-08-12T11:39:46.579905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.7073","last_updated":"2014-04-29T14:14:50Z","snapshot_observed_at":"2026-08-04T03:39:32.769738Z","submitted_at":"2014-02-27T21:00:01Z","title":"Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.7073","snapshot_observed_at":"2026-08-12T11:39:46.584582Z","title":"Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.584582Z"},"links":{"cited_paper":"/paper/1402.7073","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:2eebe1ddd7d09fdf87bc2f79752c84a15a67eecd8265638e035a14a7a30c30a2","observation_id":"de4cd6d8-7625-42eb-b16b-9dd27749fef3","resolution":{"observed_at":"2026-08-12T11:39:46.584582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.04143","last_updated":"2016-05-05T08:25:22Z","snapshot_observed_at":"2026-07-06T04:26:57.065710Z","submitted_at":"2015-08-17T20:07:34Z","title":"Dark matter cores all the way down","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.04143","snapshot_observed_at":"2026-08-12T11:39:46.588999Z","title":"Dark matter cores all the way down,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.588999Z"},"links":{"cited_paper":"/paper/1508.04143","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:62a9f5fb57008ca7bed957e5762fa446b7cec572d57683d445b690726d6427fb","observation_id":"38c14037-6def-42df-8759-bcd45495281f","resolution":{"observed_at":"2026-08-12T11:39:46.588999Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.04833","last_updated":"2017-08-09T09:53:14Z","snapshot_observed_at":"2026-07-06T05:26:33.371610Z","submitted_at":"2017-01-17T19:01:03Z","title":"How to break the density-anisotropy degeneracy in spherical stellar systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.04833","snapshot_observed_at":"2026-08-12T11:39:46.594044Z","title":"How to break the density-anisotropy degeneracy in spherical stellar systems,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.594044Z"},"links":{"cited_paper":"/paper/1701.04833","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:4baec620482796fcc61707aff96836f6656d2ff09438721aae683e1e5cbf2c66","observation_id":"667ed4c1-4b5b-4887-a335-ce61370b161c","resolution":{"observed_at":"2026-08-12T11:39:46.594044Z","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":"2026-08-12T11:39:46.598485Z","title":"Binney and S","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.598485Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:96d665dce9b769b3b4068428aab5c8e4714f5a6eea9ad485cf3fefd88e00f3f3","observation_id":"57139fba-5913-457b-a2ad-a2150011a475","resolution":{"observed_at":"2026-08-12T11:39:46.598485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201098","last_updated":"2002-01-07T21:09:22Z","snapshot_observed_at":"2026-07-07T00:24:25.145904Z","submitted_at":"2002-01-07T21:09:22Z","title":"The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201098","snapshot_observed_at":"2026-08-12T11:39:46.602830Z","title":"The Initial mass function of stars: Evidence for uniformity in variable systems,","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.602830Z"},"links":{"cited_paper":"/paper/astro-ph/0201098","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5b7ba4abcd7218e702c3b534f57920b22af4ac0a4ce4c9a6d009645dd1486c4b","observation_id":"bbf1f52a-39b7-4d42-a6a4-918f4f70ac70","resolution":{"observed_at":"2026-08-12T11:39:46.602830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0304382","last_updated":"2003-07-09T01:38:17Z","snapshot_observed_at":"2026-08-01T01:55:23.925855Z","submitted_at":"2003-04-22T15:16:01Z","title":"Galactic Stellar and Substellar Initial Mass Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0304382","snapshot_observed_at":"2026-08-12T11:39:46.607886Z","title":"Galactic stellar and substellar initial mass function,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.607886Z"},"links":{"cited_paper":"/paper/astro-ph/0304382","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:e06a2947d5b3b27eb91cf8661708bdbd5d5291b1af5cdb883f0b607c3d7c40da","observation_id":"739092bb-9e06-41b1-b314-1cbc4dcb39b7","resolution":{"observed_at":"2026-08-12T11:39:46.607886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.00778","last_updated":"2023-08-17T09:43:41Z","snapshot_observed_at":"2026-08-11T03:43:00.588042Z","submitted_at":"2023-03-01T19:05:41Z","title":"Stellar limits on scalars from electron-nucleus bremsstrahlung","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.00778","snapshot_observed_at":"2026-08-12T11:39:46.612267Z","title":"Stellar limits on scalars from electron-nucleus bremsstrahlung,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.612267Z"},"links":{"cited_paper":"/paper/2303.00778","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:029e5effd50484d80c5f50612bff01b1ff7f3d9306156cbdfae8b7aa5a2899e1","observation_id":"b58e1d2e-4fbf-488c-881e-b62f786e674c","resolution":{"observed_at":"2026-08-12T11:39:46.612267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12907","last_updated":"2023-08-30T08:27:18Z","snapshot_observed_at":"2026-07-06T15:19:50.076606Z","submitted_at":"2023-04-25T15:21:17Z","title":"Production rates of dark photons and $Z'$ in the Sun and stellar cooling bounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.12907","snapshot_observed_at":"2026-08-12T11:39:46.616276Z","title":"Production rates of dark photons and Z ′ in the Sun and stellar cooling bounds,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.616276Z"},"links":{"cited_paper":"/paper/2304.12907","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:05c2b251aa30fc1e24b5ab38da8e08768444bde6e85cd2aec79655c117e69225","observation_id":"8b57f32b-0a4b-49ce-bcc5-1cdce9658039","resolution":{"observed_at":"2026-08-12T11:39:46.616276Z","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":"2026-08-12T11:39:46.621636Z","title":"Are There Real Goldstone Bosons Associated with Broken Lepton Number?,","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.621636Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:95caaec8aadfa4fe6b1d8ceb389b3a25c526c595f0201331f6126f995ee0f0df","observation_id":"b546995d-f66a-4cca-9aed-650125833e2c","resolution":{"observed_at":"2026-08-12T11:39:46.621636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09980","last_updated":"2021-03-03T18:56:00Z","snapshot_observed_at":"2026-08-09T21:07:03.808501Z","submitted_at":"2020-12-17T23:47:04Z","title":"How dark is the $\\nu_R$-philic dark photon?","version":2},"cited_work":{"arxiv_id":"2012.09980","doi":null,"metadata_source":"pith","pith_arxiv_id":"2012.09980","snapshot_observed_at":"2026-08-12T11:39:47.381564Z","title":"How dark is the $\\nu_R$-philic dark photon?","venue":"hep-ph","work_id":"72929e58-2a67-4d39-9498-948e3fee2868","year":2020},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.625578Z"},"links":{"cited_paper":"/paper/2012.09980","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5b8132b429416ad7b00b991c59f68e2e44a649a85477f3391d1796ae2587119f","observation_id":"ae5814dd-f75e-4fe5-9168-39f3f1180b07","resolution":{"observed_at":"2026-08-12T11:39:47.385998Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11876","last_updated":"2023-05-01T00:54:59Z","snapshot_observed_at":"2026-07-06T13:03:36.428167Z","submitted_at":"2022-04-25T18:00:03Z","title":"Probing the $\\nu_{R}$-philic $Z'$ at DUNE near detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11876","snapshot_observed_at":"2026-08-12T11:39:46.630175Z","title":"Probing the νR-philic Z’ at DUNE near detectors,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.630175Z"},"links":{"cited_paper":"/paper/2204.11876","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:87d75cdec4a82b5d5d391f4b81d5225d3c62c084befe0928abb6668056e8639c","observation_id":"efe89a76-4359-4654-bf1a-bf5778983ad5","resolution":{"observed_at":"2026-08-12T11:39:46.630175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.0823","last_updated":"2013-10-02T20:00:04Z","snapshot_observed_at":"2026-07-06T03:24:38.637019Z","submitted_at":"2013-10-02T20:00:04Z","title":"Solar axion flux from the axion-electron coupling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.0823","snapshot_observed_at":"2026-08-12T11:39:46.634587Z","title":"Solar axion flux from the axion-electron coupling,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.634587Z"},"links":{"cited_paper":"/paper/1310.0823","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:8725e43e71cdfd7ead7dd2be3535995096d082e4189b3b040926258489417f53","observation_id":"bbc5c1c9-f135-4c8e-a06d-237d8c4e7168","resolution":{"observed_at":"2026-08-12T11:39:46.634587Z","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":"2026-08-12T11:39:46.638979Z","title":"Itzykson and J","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.638979Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:439874df6acfdcac7e532fb1a71b985f6135304689ae8702d0570cbd018cc6aa","observation_id":"0fb713cf-185c-4285-87a7-cfc8f167eff2","resolution":{"observed_at":"2026-08-12T11:39:46.638979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.09109","last_updated":"2023-06-09T08:51:33Z","snapshot_observed_at":"2026-08-10T22:08:06.815313Z","submitted_at":"2022-12-18T15:29:58Z","title":"Dark matter produced from right-handed neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.09109","snapshot_observed_at":"2026-08-12T11:39:46.643959Z","title":"Dark matter produced from right-handed neutrinos,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.643959Z"},"links":{"cited_paper":"/paper/2212.09109","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:1950a9db60bc561c73fd6921b85a5e66e60a55df18a375ac3737bfe517b54dcc","observation_id":"d6e41dbf-ecbd-4664-8031-acc85843ba1b","resolution":{"observed_at":"2026-08-12T11:39:46.643959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.09890","last_updated":"2022-06-04T12:58:49Z","snapshot_observed_at":"2026-08-07T23:28:45.964691Z","submitted_at":"2022-01-24T19:00:00Z","title":"Low-Energy Supernovae Severely Constrain Radiative Particle Decays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.09890","snapshot_observed_at":"2026-08-12T11:39:46.648620Z","title":"Low-Energy Supernovae Severely Constrain Radiative Particle Decays,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.648620Z"},"links":{"cited_paper":"/paper/2201.09890","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:bddc485fd4e9209abb9c2778bcb63ab4f67d242563da157841cc2ebab13b1111","observation_id":"5f9465c4-6683-4c8f-b411-3f729bd835ba","resolution":{"observed_at":"2026-08-12T11:39:46.648620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.08623","last_updated":"2019-02-22T19:00:00Z","snapshot_observed_at":"2026-08-08T17:38:12.049751Z","submitted_at":"2019-02-22T19:00:00Z","title":"Making dark matter out of light: freeze-in from plasma effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.08623","snapshot_observed_at":"2026-08-12T11:39:46.654014Z","title":"Making dark matter out of light: freeze-in from plasma effects,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.654014Z"},"links":{"cited_paper":"/paper/1902.08623","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:378a1455a64de05f0035f799c83e60ac620c9b2efc348ef3efc6ebda8cd2c870","observation_id":"9b1e98bc-4df1-4d16-a907-1e40881f24af","resolution":{"observed_at":"2026-08-12T11:39:46.654014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.05913","last_updated":"2021-06-10T16:59:03Z","snapshot_observed_at":"2026-08-10T14:22:55.980091Z","submitted_at":"2021-06-10T16:59:03Z","title":"Sterile Neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.05913","snapshot_observed_at":"2026-08-12T11:39:46.659064Z","title":"Sterile Neutrinos,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.659064Z"},"links":{"cited_paper":"/paper/2106.05913","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:9c3c0fa2a17a87dc9135e3d00973f80fd92f2f4e87f5748ea9bf6c472e81c54d","observation_id":"3a58e65b-5f31-44f7-aa28-cdb749745992","resolution":{"observed_at":"2026-08-12T11:39:46.659064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.01837","last_updated":"2017-10-25T17:38:59Z","snapshot_observed_at":"2026-08-05T01:51:45.857393Z","submitted_at":"2017-05-04T13:48:23Z","title":"Sterile neutrinos in cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.01837","snapshot_observed_at":"2026-08-12T11:39:46.663438Z","title":"Sterile neutrinos in cosmology,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.663438Z"},"links":{"cited_paper":"/paper/1705.01837","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:5b29aed70c5cb0d7378be25ec4f9965038463d79448382ca4c480d2affbfb77c","observation_id":"ab6738cb-ffd7-428a-9468-6b08ca972f3e","resolution":{"observed_at":"2026-08-12T11:39:46.663438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.04816","last_updated":"2017-02-09T14:07:58Z","snapshot_observed_at":"2026-08-02T08:15:54.788931Z","submitted_at":"2016-02-15T21:00:03Z","title":"A White Paper on keV Sterile Neutrino Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.04816","snapshot_observed_at":"2026-08-12T11:39:46.668323Z","title":"A White Paper on keV Sterile Neutrino Dark Matter,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.668323Z"},"links":{"cited_paper":"/paper/1602.04816","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:6b16e03cb9f2f34a5bc458bcf0719580e93496855a3f9e0a2e9c9e656c067839","observation_id":"8342bef5-3e62-44a2-8162-1cf46af5f826","resolution":{"observed_at":"2026-08-12T11:39:46.668323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15565","last_updated":"2024-02-15T10:25:13Z","snapshot_observed_at":"2026-08-10T14:22:55.208957Z","submitted_at":"2023-07-28T14:02:39Z","title":"Boosting the production of sterile neutrino dark matter with self-interactions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15565","snapshot_observed_at":"2026-08-12T11:39:46.673243Z","title":"Boosting the production of sterile neutrino dark matter with self-interactions,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.673243Z"},"links":{"cited_paper":"/paper/2307.15565","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:a316900803e612c37985236e767844434e7528a207e6cfc47154c32a35b6210e","observation_id":"b32a751a-28f5-4160-9719-06349193de21","resolution":{"observed_at":"2026-08-12T11:39:46.673243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.02707","last_updated":"2018-01-10T17:46:58Z","snapshot_observed_at":"2026-08-03T09:02:37.525190Z","submitted_at":"2017-06-08T18:00:03Z","title":"Thermalizing sterile neutrino dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.02707","snapshot_observed_at":"2026-08-12T11:39:46.678181Z","title":"Thermalizing sterile neutrino dark matter,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.678181Z"},"links":{"cited_paper":"/paper/1706.02707","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:01bfe289e30130e5b342d182d1340fa976c2e6e7bee9de1101713c79023956d3","observation_id":"baa2c707-2ea6-4b9f-9f92-932880bfee34","resolution":{"observed_at":"2026-08-12T11:39:46.678181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.09883","last_updated":"2021-10-19T11:56:52Z","snapshot_observed_at":"2026-08-09T15:28:05.336284Z","submitted_at":"2021-10-19T11:56:52Z","title":"Dark matter produced from neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.09883","snapshot_observed_at":"2026-08-12T11:39:46.682617Z","title":"Dark matter produced from neutrinos,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.682617Z"},"links":{"cited_paper":"/paper/2110.09883","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:4668da1369f4bf32e70f55f83599c8f03f1c18b38a4189c3d858b073fc7d5201","observation_id":"1e68e966-e722-41c2-8942-3d6a6656a9d1","resolution":{"observed_at":"2026-08-12T11:39:46.682617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.17151","last_updated":"2024-03-18T00:31:39Z","snapshot_observed_at":"2026-08-12T11:41:20.887963Z","submitted_at":"2023-12-28T17:32:17Z","title":"Imprints of light dark matter on the evolution of cosmic neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.17151","snapshot_observed_at":"2026-08-12T11:39:46.686893Z","title":"Imprints of light dark matter on the evolution of cosmic neutrinos,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.686893Z"},"links":{"cited_paper":"/paper/2312.17151","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:904cc7eeb2c598d1e9481137e6f5eadc7d526ea8fa78b0e6227251a31b262eb5","observation_id":"debcc458-d7d3-46c5-952f-70e48e128aec","resolution":{"observed_at":"2026-08-12T11:39:46.686893Z","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":"2026-08-12T11:39:46.691787Z","title":"Two U(1)’s and Epsilon Charge Shifts,","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.691787Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:7686bf8ff727a40aad45c38a38a76c85fd5d9a204fb1e95b8f15039180979289","observation_id":"758b510e-0949-4a1a-84ac-86fc6a6602c3","resolution":{"observed_at":"2026-08-12T11:39:46.691787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.3884","last_updated":"2013-08-20T15:56:09Z","snapshot_observed_at":"2026-07-06T03:06:32.268635Z","submitted_at":"2013-02-15T21:00:01Z","title":"New stellar constraints on dark photons","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.3884","snapshot_observed_at":"2026-08-12T11:39:46.696522Z","title":"New stellar constraints on dark photons,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.696522Z"},"links":{"cited_paper":"/paper/1302.3884","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:560603ea2b66a43de4079002e6f125b3b78531ac8ef4114ae2b2c5c4eee6b180","observation_id":"72b5e3f2-536d-4ffd-89a9-b07ffc924558","resolution":{"observed_at":"2026-08-12T11:39:46.696522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04847","last_updated":"2018-07-09T13:36:00Z","snapshot_observed_at":"2026-08-12T15:04:06.584907Z","submitted_at":"2018-01-15T15:25:50Z","title":"Serendipity in dark photon searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04847","snapshot_observed_at":"2026-08-12T11:39:46.701132Z","title":"Serendipity in dark photon searches,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.701132Z"},"links":{"cited_paper":"/paper/1801.04847","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:9b2495576eefbef02a84cebb09e0a21aef0d14f3171e80295f2803141ed1e638","observation_id":"b6eaa460-cf1a-44a0-bd7e-7c26de107b81","resolution":{"observed_at":"2026-08-12T11:39:46.701132Z","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":"2026-08-12T11:39:46.705809Z","title":"Search for Neutral Metastable Penetrating Particles Produced in the SLAC Beam Dump,","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.705809Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:2e2bd5ea54e766d4445cb68be83fdc0222aae63b71e3973fcb3c389794020613","observation_id":"84581c4a-b173-4e8b-adc9-12841eba56dc","resolution":{"observed_at":"2026-08-12T11:39:46.705809Z","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":"2026-08-12T11:39:46.709822Z","title":"A Search for Short Lived Axions in an Electron Beam Dump Experiment,","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.709822Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:d4cf3ee9874c18af7e30ead7aa73b519d61f455347ed61a1eb7a53488df6db44","observation_id":"6a5abf60-9b9c-4548-b39e-c8b5ee050ddb","resolution":{"observed_at":"2026-08-12T11:39:46.709822Z","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":"2026-08-12T11:39:46.714430Z","title":"An Unambiguous Search for a Light Higgs Boson,","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.714430Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:fad45d9ef0e49ad428fce754e0c72d3923d6508ce8c2d2f59937a0522e2629d6","observation_id":"02b5de63-0256-4716-ba02-d3154b9f4ba3","resolution":{"observed_at":"2026-08-12T11:39:46.714430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.2980","last_updated":"2014-09-18T22:17:20Z","snapshot_observed_at":"2026-07-06T03:46:05.904156Z","submitted_at":"2014-06-11T17:54:39Z","title":"Search for a dark photon in e+e- collisions at BABAR","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.2980","snapshot_observed_at":"2026-08-12T11:39:46.718161Z","title":"Search for a Dark Photon in e+e− Collisions at BaBar,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.718161Z"},"links":{"cited_paper":"/paper/1406.2980","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:65f41ff45c8a66cbe01b2bb895c870d9b095611b324cffd265720a1f6064979b","observation_id":"4bd481dc-b0e5-4ee2-948d-c6d1b0a014fa","resolution":{"observed_at":"2026-08-12T11:39:46.718161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.00607","last_updated":"2015-04-30T16:19:56Z","snapshot_observed_at":"2026-07-06T04:13:55.589663Z","submitted_at":"2015-04-02T16:21:03Z","title":"Search for the dark photon in $\\pi^0$ decays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.00607","snapshot_observed_at":"2026-08-12T11:39:46.722154Z","title":"Search for the dark photon in π0 decays,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.722154Z"},"links":{"cited_paper":"/paper/1504.00607","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:914fcda5a66c91b350a50f8de93e8f788dc17056c516ef536db79743db88fdea","observation_id":"906701f3-eee8-4ddb-9f71-b96d2be47513","resolution":{"observed_at":"2026-08-12T11:39:46.722154Z","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":"2026-08-12T11:39:46.726717Z","title":"Search for A′ → µ+µ− decays,","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.726717Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:d8d7aaae8c53a35069e7d6883e2a368c1a445d2bf115e7d44f78aac136856a10","observation_id":"9592f672-db33-4f16-b865-37a0e1e2da5a","resolution":{"observed_at":"2026-08-12T11:39:46.726717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.13967","last_updated":"2023-10-03T07:26:47Z","snapshot_observed_at":"2026-08-08T12:43:37.011870Z","submitted_at":"2023-07-26T05:58:10Z","title":"$N_{{\\rm eff}}$ constraints on light mediators coupled to neutrinos: the dilution-resistant effect","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.13967","snapshot_observed_at":"2026-08-12T11:39:46.731025Z","title":"Neff constraints on light mediators coupled to neutrinos: the dilution-resistant effect,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.731025Z"},"links":{"cited_paper":"/paper/2307.13967","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:2f3491096a41017c48e7841dd892e96167cd8bf5fa9129bc62eb716ec25dbc79","observation_id":"e1ea6bba-102d-4617-961f-d0fd3ac2fbb6","resolution":{"observed_at":"2026-08-12T11:39:46.731025Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0326","last_updated":"2008-11-03T16:14:44Z","snapshot_observed_at":"2026-07-06T01:45:42.903745Z","submitted_at":"2008-11-03T16:14:44Z","title":"Massive hidden photons as lukewarm dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.0326","snapshot_observed_at":"2026-08-12T11:39:46.735256Z","title":"Massive hidden photons as lukewarm dark matter,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.735256Z"},"links":{"cited_paper":"/paper/0811.0326","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:15cfff36eb4d082908b68125888617774181f42bba98b72953cb60ae1221cfca","observation_id":"22b9f84d-c103-4cf8-a8b4-057661ebcf16","resolution":{"observed_at":"2026-08-12T11:39:46.735256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.00619","last_updated":"2017-05-01T18:00:01Z","snapshot_observed_at":"2026-07-06T05:40:07.126075Z","submitted_at":"2017-05-01T18:00:01Z","title":"Dark Photon Decay Beyond The Euler-Heisenberg Limit","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.00619","snapshot_observed_at":"2026-08-12T11:39:46.740142Z","title":"Dark Photon Decay Beyond The Euler-Heisenberg Limit,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.740142Z"},"links":{"cited_paper":"/paper/1705.00619","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:88bd3abbf9ceb8405a8842bbe5e4cf79a71010463a85ff4b78b3a87659d38f15","observation_id":"9591f2dd-14b2-4d4a-b73e-4ce90f704e06","resolution":{"observed_at":"2026-08-12T11:39:46.740142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.01839","last_updated":"2024-02-02T19:00:11Z","snapshot_observed_at":"2026-08-11T04:06:17.486053Z","submitted_at":"2024-02-02T19:00:11Z","title":"Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.01839","snapshot_observed_at":"2026-08-12T11:39:46.744648Z","title":"Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.744648Z"},"links":{"cited_paper":"/paper/2402.01839","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:6959967f4a092def113ba1e464e7dc5838a462d83ca5b41d2025af84a2c9277b","observation_id":"346e23fd-60eb-4ccd-92b4-034dc25ce8d1","resolution":{"observed_at":"2026-08-12T11:39:46.744648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.19445","last_updated":"2025-07-21T16:45:13Z","snapshot_observed_at":"2026-08-12T23:33:22.816208Z","submitted_at":"2024-06-27T18:00:01Z","title":"X-Ray Constraints on Dark Photon Tridents","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.19445","snapshot_observed_at":"2026-08-12T11:39:46.750152Z","title":"X-Ray Constraints on Dark Photon Tridents,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.750152Z"},"links":{"cited_paper":"/paper/2406.19445","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:a617276ebb346d5cb2cb0c851d5fd8c32da70c7f5ee09c5ac6d54fbf74d1655a","observation_id":"951aedbf-2e9c-4258-b76e-3270394351a3","resolution":{"observed_at":"2026-08-12T11:39:46.750152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.05147","last_updated":"2021-08-11T10:48:31Z","snapshot_observed_at":"2026-07-06T11:37:25.989607Z","submitted_at":"2021-08-11T10:48:31Z","title":"Probing the muon $g-2$ with future beam dump experiments","version":1},"cited_work":{"arxiv_id":"2108.05147","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.05147","snapshot_observed_at":"2026-08-12T11:39:46.910280Z","title":"Probing the muon $g-2$ with future beam dump experiments","venue":"hep-ph","work_id":"b8000b1e-deff-4ca1-bd7e-307fc4d43055","year":2021},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.754423Z"},"links":{"cited_paper":"/paper/2108.05147","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:e7c9eae5918eaa672b74dbbbf9693856088a0d6172199d85d7dd625927dd965f","observation_id":"45d863db-310f-4822-8057-32fe86c2ebe8","resolution":{"observed_at":"2026-08-12T11:39:46.914639Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1606.03501","last_updated":"2016-06-10T23:43:18Z","snapshot_observed_at":"2026-08-09T23:14:40.687632Z","submitted_at":"2016-06-10T23:43:18Z","title":"Search for a muonic dark force at BABAR","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.03501","snapshot_observed_at":"2026-08-12T11:39:46.758833Z","title":"Search for a muonic dark force at BABAR,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.758833Z"},"links":{"cited_paper":"/paper/1606.03501","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:c88628eeb99249b743f62a89c7d7a0ce3b02839334e2f885e67d9789185b87e8","observation_id":"b1713de0-771d-4342-998b-ec233a36a99b","resolution":{"observed_at":"2026-08-12T11:39:46.758833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.03684","last_updated":"2019-04-11T12:54:19Z","snapshot_observed_at":"2026-07-06T06:55:08.241651Z","submitted_at":"2018-08-10T19:26:16Z","title":"Search for an $L_{\\mu}$ $-$ $L_{\\tau}$ gauge boson using Z $\\to$ 4$\\mu$ events in proton-proton collisions at $\\sqrt{s} =$ 13 TeV","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.03684","snapshot_observed_at":"2026-08-12T11:39:46.762553Z","title":"Search for an Lµ − Lτ gauge boson using Z → 4µ events in proton-proton collisions at √s = 13 TeV,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.762553Z"},"links":{"cited_paper":"/paper/1808.03684","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:469cb4260314096deb1cf06ec46b7febe45303ae9c5fc44c015f143f87894cdb","observation_id":"8f53524c-d88f-436d-834a-d909eb76c75b","resolution":{"observed_at":"2026-08-12T11:39:46.762553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.07955","last_updated":"2024-04-29T17:20:33Z","snapshot_observed_at":"2026-08-02T00:39:07.759922Z","submitted_at":"2023-08-15T18:00:02Z","title":"Cosmological Implications of Gauged $U(1)_{B-L}$ on $\\Delta N_{\\rm eff}$ in the CMB and BBN","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.07955","snapshot_observed_at":"2026-08-12T11:39:46.765903Z","title":"Cosmological implications of gauged U(1) B−L on ∆N ef fin the CMB and BBN,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.765903Z"},"links":{"cited_paper":"/paper/2308.07955","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:f1ae73fd73a42eaa81ab3099b695483f32bdddc24e63fbcf474a004b91393074","observation_id":"bccedd48-41c7-419b-8eda-4733d574c2e8","resolution":{"observed_at":"2026-08-12T11:39:46.765903Z","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":"2026-08-12T11:39:46.770684Z","title":"Low-energy interactions of scalar and pseudoscalar Higgs bosons with baryons,","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.770684Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:bef723640c277599a4ecc0e2628e20ebf9f4d9f6856ab94b8457708a04e8c0d6","observation_id":"32ab0aaa-8623-4006-a6a8-9da209d7ac0b","resolution":{"observed_at":"2026-08-12T11:39:46.770684Z","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":"2026-08-12T11:39:46.775219Z","title":"Remarks on Higgs Boson Interactions with Nucleons,","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.775219Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:8eb232ea73d6f0105b18810d629c22ed3c6884a093ac6190f1023537a6f985ca","observation_id":"3741ba89-05bf-4ac2-b40b-06b1f150ee09","resolution":{"observed_at":"2026-08-12T11:39:46.775219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.03123","last_updated":"2023-04-30T06:40:27Z","snapshot_observed_at":"2026-07-06T14:59:10.875394Z","submitted_at":"2023-03-06T13:37:14Z","title":"Stellar cooling limits on light scalar boson revisited","version":2},"cited_work":{"arxiv_id":"2303.03123","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.03123","snapshot_observed_at":"2026-08-12T11:39:46.847201Z","title":"Stellar cooling limits on light scalar boson revisited","venue":"hep-ph","work_id":"99c9591e-4315-4406-9e53-01211ba1c4c9","year":2023},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.778928Z"},"links":{"cited_paper":"/paper/2303.03123","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:da8de25e088a9f1c70e738ebc48dced6151f894351901c83555d3ca398462a42","observation_id":"7ec5dcb9-4925-4a39-b217-c7995d480abd","resolution":{"observed_at":"2026-08-12T11:39:46.853955Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02471","last_updated":"2017-08-08T18:50:39Z","snapshot_observed_at":"2026-08-10T17:43:06.520104Z","submitted_at":"2017-03-07T17:02:24Z","title":"Long Lived Light Scalars as Probe of Low Scale Seesaw Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02471","snapshot_observed_at":"2026-08-12T11:39:46.783310Z","title":"Long Lived Light Scalars as Probe of Low Scale Seesaw Models,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.783310Z"},"links":{"cited_paper":"/paper/1703.02471","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:c7a1f99896a42b511164ea81ec1ef4f8a8f2c9cc4201a0585edff43738a9bbf6","observation_id":"df5a54f0-2748-49a6-9da9-53769a97dbc1","resolution":{"observed_at":"2026-08-12T11:39:46.783310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0503172","last_updated":"2005-05-03T15:16:20Z","snapshot_observed_at":"2026-08-06T06:42:39.028076Z","submitted_at":"2005-03-17T16:46:33Z","title":"The Anatomy of Electro-Weak Symmetry Breaking. I: The Higgs boson in the Standard Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0503172","snapshot_observed_at":"2026-08-12T11:39:46.787082Z","title":"The Anatomy of electro-weak symmetry breaking. I: The Higgs boson in the standard model,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.787082Z"},"links":{"cited_paper":"/paper/hep-ph/0503172","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:31fa1a98f11a748437c948490d7502d303f5d4902059552e5fa19ea35ac35213","observation_id":"68893ecf-1acd-4e4a-987d-f26086ee3329","resolution":{"observed_at":"2026-08-12T11:39:46.787082Z","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":"2026-08-12T11:39:46.791237Z","title":"Simple Rules for Discontinuities in Finite Temperature Field Theory,","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.791237Z"},"links":{"citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:1772458ee2b17029b8367898a24787742dbcf95e07e2804aa0189e6720e43e4e","observation_id":"842f6751-8fcc-4e7c-9bce-5cc863d39764","resolution":{"observed_at":"2026-08-12T11:39:46.791237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-13T01:27:39.373957Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae"},"reference_resolution":{"displayed":97,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":92,"verified_exact":5,"verified_fuzzy":0},"total_outbound_references":97},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 97 of 97 outbound references and 1 inbound Pith citation observation for arXiv:2411.18052."}