{"as_of":"2026-08-19T18:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:187c16fbc35fb3586560f86a70ffa5506d6ec079b3adba2dd1a5063f5aae44e1","coverage":[{"denominator":74,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:25:24.527957Z","state":"measured"},{"denominator":86,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":86,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T20:33:14.976348Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-09T15:06:18.248247Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-08-11T13:29:11.516597Z","title":"NuSTAR bounds on radiatively decaying particles from M82,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13247","last_updated":"2024-12-17T19:00:00Z","snapshot_observed_at":"2026-08-17T01:20:54.479688Z","submitted_at":"2024-12-17T19:00:00Z","title":"Time-delayed gamma-ray signatures of heavy axions from core-collapse supernovae","version":1},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-08-11T13:29:11.516597Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2412.13247"},"observation_digest":"sha256:465ab228999dcc1569c2340098583c6284dc1ce85062b88be9f76b2c12907cd5","observation_id":"b633d48a-b58c-4c32-8f04-e883f9ad8c8c","resolution":{"observed_at":"2026-08-11T13:29:11.516597Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2503.15630","last_updated":"2026-04-13T00:19:50Z","snapshot_observed_at":"2026-08-17T16:22:08.217065Z","submitted_at":"2025-03-19T18:31:06Z","title":"Supernova production of axion-like particles coupling to electrons, reloaded","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-22T23:00:23.220844Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2503.15630"},"observation_digest":"sha256:28f28e59e8254e42a5d949a0f7047d6de8ce5ea9fb23f25ffc8bd546d81b8026","observation_id":"d8a23bb4-277a-49ed-9255-2370c3c24238","resolution":{"observed_at":"2026-05-22T23:02:13.417762Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-08-15T20:33:14.976348Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12905","last_updated":"2025-05-19T09:40:34Z","snapshot_observed_at":"2026-08-18T21:39:55.367625Z","submitted_at":"2025-05-19T09:40:34Z","title":"Lecture Notes: WISPs in gamma-ray astrophysics","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T20:33:14.976348Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2505.12905"},"observation_digest":"sha256:a70d4b816a8b759a1c81e3219afdc9dd7da50db2d6ba25cf67bfb1fc3b6caabf","observation_id":"8d63b168-959d-493c-83fb-29832443a62a","resolution":{"observed_at":"2026-08-15T20:33:14.976348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-08-06T20:14:37.541212Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.03535","last_updated":"2026-07-17T14:50:54Z","snapshot_observed_at":"2026-08-17T00:20:13.046174Z","submitted_at":"2025-07-04T12:39:23Z","title":"Constraining the axiverse with reionization","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T20:14:37.541212Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2507.03535"},"observation_digest":"sha256:c4005227f7ae8f2aa54181b29a8d3552ce6d2eba7c6241cfd52b4638c8358145","observation_id":"0f314ecd-3305-4ee7-923e-a2d2f3d7a77f","resolution":{"observed_at":"2026-08-06T20:14:37.541212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-08-05T10:57:49.433929Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03569","last_updated":"2025-09-03T18:00:00Z","snapshot_observed_at":"2026-08-12T19:04:12.708177Z","submitted_at":"2025-09-03T18:00:00Z","title":"Axion lines from nuclear de-excitations in galactic stellar populations","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-05T10:57:49.433929Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2509.03569"},"observation_digest":"sha256:92f9a6f10d42ca4d2b3c3bb31d88d04f13bfbb0f3e774417eb39e824cbff0352","observation_id":"4f0e1842-f8fa-4412-87ff-f260c9ecf287","resolution":{"observed_at":"2026-08-05T10:57:49.433929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2604.02413","last_updated":"2026-04-02T18:00:00Z","snapshot_observed_at":"2026-08-11T00:29:23.416387Z","submitted_at":"2026-04-02T18:00:00Z","title":"The Black Hole Mass Gap as a New Probe of Millicharged Particles","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-05-13T21:01:01.821843Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2604.02413"},"observation_digest":"sha256:b99f622dbc77f62acd49231160bf9f448b7d9d850ff845a106fc0c0a00a0570c","observation_id":"c901e54f-2695-4240-a8db-2018da90bff4","resolution":{"observed_at":"2026-05-13T21:03:19.761101Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2604.02419","last_updated":"2026-04-02T18:00:03Z","snapshot_observed_at":"2026-08-06T12:39:06.550051Z","submitted_at":"2026-04-02T18:00:03Z","title":"Millicharged Particle Production During Late-Stage Stellar Evolution","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-13T20:48:40.697992Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2604.02419"},"observation_digest":"sha256:93fa2f53d92251d0f9f1482b2f09a4bc38485fc61b802526009002ec995d0001","observation_id":"97803aa6-30d4-4529-9a2c-347f624fa946","resolution":{"observed_at":"2026-05-13T20:53:16.318947Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2604.18397","last_updated":"2026-04-20T15:20:22Z","snapshot_observed_at":"2026-08-03T00:06:52.301723Z","submitted_at":"2026-04-20T15:20:22Z","title":"Looking for Lights from the Darkness: Signals from MeV-scale Solar Axion-like Particles","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-10T04:20:23.219527Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2604.18397"},"observation_digest":"sha256:4714e148d6fae70478ad8ef6a4a7ce35ebd7eda46eb5e1bbe14b15ffee8c0048","observation_id":"b5f4f28f-958c-462f-a08e-d906997c58e3","resolution":{"observed_at":"2026-05-11T12:01:05.742796Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2604.20768","last_updated":"2026-04-22T16:57:22Z","snapshot_observed_at":"2026-08-16T10:16:57.402676Z","submitted_at":"2026-04-22T16:57:22Z","title":"Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition","version":1},"reference_index":191,"source":"pdf_text","source_observed_at":"2026-05-09T23:54:19.807809Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2604.20768"},"observation_digest":"sha256:67fdbfeeab5b3a73f5ee8e91477551f19443d06a2a8cb6c89955a95dbe5bb1fd","observation_id":"6b227b71-3e30-4ccf-bb8f-f3d13c8fc6d9","resolution":{"observed_at":"2026-05-11T13:56:03.720398Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2605.15261","last_updated":"2026-05-14T18:00:00Z","snapshot_observed_at":"2026-08-16T02:51:44.994897Z","submitted_at":"2026-05-14T18:00:00Z","title":"Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-19T16:10:46.102334Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2605.15261"},"observation_digest":"sha256:489a563d7973a63ac26e11318be9423461b8142a17272151500d7fa3e3764e15","observation_id":"ef00d028-1284-41c6-a9e5-0e8d7e6aae99","resolution":{"observed_at":"2026-05-19T16:12:38.972790Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2605.21092","last_updated":"2026-05-20T12:24:00Z","snapshot_observed_at":"2026-08-03T10:38:16.949612Z","submitted_at":"2026-05-20T12:24:00Z","title":"Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves","version":1},"reference_index":125,"source":"pdf_text","source_observed_at":"2026-05-21T04:24:21.715932Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2605.21092"},"observation_digest":"sha256:dde51abab7ff20c2df17954d97b14cf03a16ca808542d855f812faf886bbc933","observation_id":"7bed0046-5d63-4609-94f1-d92cbc57aaf4","resolution":{"observed_at":"2026-05-21T04:24:33.421850Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"cited_work":{"arxiv_id":"2412.03660","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.03660","snapshot_observed_at":"2026-07-09T15:06:18.248247Z","title":"Cand´ on, D.F.G","venue":"hep-ph","work_id":"6eb2a07c-da9b-407f-bd1c-02c4aa2e2315","year":2024},"citing_paper":{"arxiv_id":"2607.07297","last_updated":"2026-07-08T11:40:05Z","snapshot_observed_at":"2026-08-07T04:07:28.927106Z","submitted_at":"2026-07-08T11:40:05Z","title":"Reappraisal of the Constraints on Heavy Axion-like Particles from Gamma-Ray Bursts","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-09T14:56:45.760028Z"},"links":{"cited_paper":"/paper/2412.03660","citing_paper":"/paper/2607.07297"},"observation_digest":"sha256:249e613aa4bcfeaed7d257e4e7659eda740a59e718cc11962d6c78565637b71f","observation_id":"c5035644-69e2-4cf3-93b1-44eb88bf08ba","resolution":{"observed_at":"2026-07-09T15:06:18.249547Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2412.03660/citation-record","integrity":"/paper/2412.03660/integrity","json":"/paper/2412.03660/citation-record.json","paper":"/paper/2412.03660"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1611.03864","last_updated":"2019-05-31T21:23:15Z","snapshot_observed_at":"2026-08-14T21:30:48.726079Z","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":"2026-08-11T22:25:24.255734Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.255734Z"},"links":{"cited_paper":"/paper/1611.03864","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:eaa0dd240a58177498141ddee551e4536544e8719ad2535990fd53e138e099a1","observation_id":"d56128a5-dc13-4b56-a5be-7486263894a5","resolution":{"observed_at":"2026-08-11T22:25:24.255734Z","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":"2026-08-14T21:29:52.715965Z","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":"2026-08-11T22:25:24.261808Z","title":"Hardy and R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.261808Z"},"links":{"cited_paper":"/paper/1611.05852","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:c417b0671eb518aca76f4a020232a0a758e55af512335dc9aee2ec97035f5203","observation_id":"bbd99521-a296-4973-8393-7ab27a2a5e43","resolution":{"observed_at":"2026-08-11T22:25:24.261808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02964","last_updated":"2018-09-29T08:28:43Z","snapshot_observed_at":"2026-08-14T21:17:09.636207Z","submitted_at":"2017-02-09T19:47:09Z","title":"Decay photons from the ALP burst of type-II supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02964","snapshot_observed_at":"2026-08-11T22:25:24.266544Z","title":"Jaeckel, P","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.266544Z"},"links":{"cited_paper":"/paper/1702.02964","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:a9f0eabd92f62d43ddda9eb01fba182d2e707e0b5bb8f20243958940b577372e","observation_id":"fe314ecf-8a95-4061-9c06-973d7dcf01d9","resolution":{"observed_at":"2026-08-11T22:25:24.266544Z","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":"2026-08-14T19:40:10.034578Z","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":"2026-08-11T22:25:24.270786Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.270786Z"},"links":{"cited_paper":"/paper/1803.00993","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:e2e82b75bedfe7b7a0ebab2812c04e23e56905bd8d382e1922734d440931adee","observation_id":"685f714b-e2e3-42f4-bc98-f3a3a5cdb43f","resolution":{"observed_at":"2026-08-11T22:25:24.270786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.08596","last_updated":"2020-07-03T02:08:16Z","snapshot_observed_at":"2026-08-14T17:26:17.311917Z","submitted_at":"2019-01-24T19:00:00Z","title":"Observable signatures of dark photons from supernovae","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.08596","snapshot_observed_at":"2026-08-11T22:25:24.275132Z","title":"DeRocco, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.275132Z"},"links":{"cited_paper":"/paper/1901.08596","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:832aa074bf49de94352c1738cafe9ade0c281554208f9e35a63e82b658769f20","observation_id":"fec8d3f0-1a6f-48d2-8253-e9d228e6e759","resolution":{"observed_at":"2026-08-11T22:25:24.275132Z","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":"2026-08-11T22:25:24.279340Z","title":"Croon, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.279340Z"},"links":{"cited_paper":"/paper/2006.13942","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:e71cba83b79b5e2f19a07d84527293e8fff7d85c241ebfeb991c602bef496a1d","observation_id":"4535d08b-12cf-493a-8580-763830362061","resolution":{"observed_at":"2026-08-11T22:25:24.279340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.09764","last_updated":"2023-03-28T17:47:09Z","snapshot_observed_at":"2026-08-16T16:07:33.854247Z","submitted_at":"2022-12-19T19:00:01Z","title":"Updated constraints on axion-like particles from temporal information in supernova SN1987A gamma-ray data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.09764","snapshot_observed_at":"2026-08-11T22:25:24.283965Z","title":"Hoof and L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.283965Z"},"links":{"cited_paper":"/paper/2212.09764","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:c71e7e25a47994410b38f79b9c9460da5bf2c57b4a98ee11616eac08479c9cfa","observation_id":"25ebfe63-552a-4238-aeda-d5f9e6241131","resolution":{"observed_at":"2026-08-11T22:25:24.283965Z","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":"2026-08-16T18:56:53.496565Z","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":"2026-08-11T22:25:24.287529Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.287529Z"},"links":{"cited_paper":"/paper/2012.11632","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:0ad8cbb373856a8b4dc80bb55e5b2c5148ce3e82b5353afd25b463ba40c42755","observation_id":"f6f143e2-34d2-4b2a-9403-3d1e24bedb46","resolution":{"observed_at":"2026-08-11T22:25:24.287529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.05727","last_updated":"2021-04-12T18:00:02Z","snapshot_observed_at":"2026-08-16T18:32:09.040928Z","submitted_at":"2021-04-12T18:00:02Z","title":"Axion-like Particles from Hypernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.05727","snapshot_observed_at":"2026-08-11T22:25:24.291133Z","title":"Caputo, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.291133Z"},"links":{"cited_paper":"/paper/2104.05727","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:af691c17f202d116c931570de60c902524f70d2a6128af066b9e70ae35e9cdf3","observation_id":"3e77a710-1663-4d3e-8b11-1b094251fa08","resolution":{"observed_at":"2026-08-11T22:25:24.291133Z","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":"2026-08-15T01:25:39.071158Z","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":"2026-08-11T22:25:24.294799Z","title":"Caputo, G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.294799Z"},"links":{"cited_paper":"/paper/2109.03244","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:30654b76fe2179707cd6b2a520863b0dcf55ba007228c44e1e5f324e0c4f057b","observation_id":"a9df9960-2a8c-4472-a58d-9b4ea19685b5","resolution":{"observed_at":"2026-08-11T22:25:24.294799Z","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":"2026-08-16T17:26:18.809199Z","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":"2026-08-11T22:25:24.298268Z","title":"Caputo, H.-T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.298268Z"},"links":{"cited_paper":"/paper/2201.09890","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:da2a73482bc3a29b77744383c2fb565a320db7b336266234e5451447aeff89b5","observation_id":"6f519364-441f-4c6d-b607-2150c90b34af","resolution":{"observed_at":"2026-08-11T22:25:24.298268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.07896","last_updated":"2022-11-25T09:52:18Z","snapshot_observed_at":"2026-08-16T16:59:56.553108Z","submitted_at":"2022-05-16T18:00:01Z","title":"Strong supernovae bounds on ALPs from quantum loops","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.07896","snapshot_observed_at":"2026-08-11T22:25:24.301777Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.301777Z"},"links":{"cited_paper":"/paper/2205.07896","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:50a61041eaa8494494271b127fb43007a72be497ca2f0b080a1373fdd4dae43a","observation_id":"656e15a3-1e59-4870-9cee-5aa22668c2f7","resolution":{"observed_at":"2026-08-11T22:25:24.301777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11862","last_updated":"2022-09-17T12:21:08Z","snapshot_observed_at":"2026-08-19T13:37:19.103890Z","submitted_at":"2022-04-25T18:00:00Z","title":"Radiative transfer in stars by feebly interacting bosons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11862","snapshot_observed_at":"2026-08-11T22:25:24.305219Z","title":"Caputo, G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.305219Z"},"links":{"cited_paper":"/paper/2204.11862","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:93f028f6bb0daca118f77281f217ef78068d9b38d3e81f7aabc1fe8db3ad11ec","observation_id":"2c804d1b-cd5e-4c8a-bf23-79f97c0140e1","resolution":{"observed_at":"2026-08-11T22:25:24.305219Z","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":"2026-08-17T22:21:24.965278Z","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":"2026-08-11T22:25:24.308716Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.308716Z"},"links":{"cited_paper":"/paper/2209.11773","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:4bb4714a3663fc20f0926218fa19f72953aec3dac7964c00bf4f23c78c5182d9","observation_id":"3e0a9ddf-a5e6-4f6b-af18-1514dbfc33a9","resolution":{"observed_at":"2026-08-11T22:25:24.308716Z","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":"2026-08-18T21:25:20.514680Z","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":"2026-08-11T22:25:24.312542Z","title":"Carenza, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.312542Z"},"links":{"cited_paper":"/paper/2311.00033","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:7a0c19644824414ba3a108ea954a96995a000951cc7dd721de4017b868b8d939","observation_id":"085952da-49d4-4cad-8c56-97891ae62ddc","resolution":{"observed_at":"2026-08-11T22:25:24.312542Z","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":"2026-08-19T15:55:13.714983Z","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":"2026-08-11T22:25:24.316515Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.316515Z"},"links":{"cited_paper":"/paper/2307.03143","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:12053c385ada95b5e24857a91eea7a7eafb2f7bbadac7aa38a2a700b3d5f84df","observation_id":"6727efc2-52ec-47ae-b4ed-aae43e6b8298","resolution":{"observed_at":"2026-08-11T22:25:24.316515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01048","last_updated":"2024-01-03T09:54:10Z","snapshot_observed_at":"2026-08-16T15:27:21.804168Z","submitted_at":"2023-06-01T18:00:05Z","title":"Getting the most on supernova axions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01048","snapshot_observed_at":"2026-08-11T22:25:24.320465Z","title":"Lella, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.320465Z"},"links":{"cited_paper":"/paper/2306.01048","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:a972e1bb6fbd180291df212ae4a9209b2b357c4e1b528f8e62fc626c87e9f3a3","observation_id":"98b1683d-ab8a-42b2-8c40-526a017d8284","resolution":{"observed_at":"2026-08-11T22:25:24.320465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.11395","last_updated":"2023-07-14T15:55:40Z","snapshot_observed_at":"2026-08-16T15:46:45.404918Z","submitted_at":"2023-03-20T19:00:02Z","title":"Axion-sourced fireballs from supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.11395","snapshot_observed_at":"2026-08-11T22:25:24.324362Z","title":"Diamond, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.324362Z"},"links":{"cited_paper":"/paper/2303.11395","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:20ea01dd21ab4429c10a2f7d53620e203b91f0f6dbaca2c72ff1fa53534eeb74","observation_id":"b3e2fe11-c702-418f-9ff5-57aa4a84ded4","resolution":{"observed_at":"2026-08-11T22:25:24.324362Z","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":"2026-08-16T14:32:43.170709Z","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":"2026-08-11T22:25:24.328130Z","title":"Akita, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.328130Z"},"links":{"cited_paper":"/paper/2312.13627","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:2a59dc802cef3805ea2d0fcb81edc5ff0bf66e622e34dcdf3ae546ab0886c864","observation_id":"422a599c-dfb3-44a5-b9a9-06854ba78c99","resolution":{"observed_at":"2026-08-11T22:25:24.328130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16397","last_updated":"2024-01-17T09:44:16Z","snapshot_observed_at":"2026-08-16T15:20:18.733319Z","submitted_at":"2023-06-28T17:43:57Z","title":"Constraining MeV-scale axion-like particles with Fermi-LAT observations of SN 2023ixf","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16397","snapshot_observed_at":"2026-08-11T22:25:24.331933Z","title":"M¨ uller, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.331933Z"},"links":{"cited_paper":"/paper/2306.16397","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:37bd3753f0b06295b40079b99e03a2a62431879d9f6a67c6af2c332b5f11af28","observation_id":"ed9b43b7-ecbf-4781-81f2-aaee6c694e46","resolution":{"observed_at":"2026-08-11T22:25:24.331933Z","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":"2026-08-16T15:12:43.423713Z","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":"2026-08-11T22:25:24.335741Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.335741Z"},"links":{"cited_paper":"/paper/2307.15122","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:eef8a70e37a446bff78923f2a2dab56f1730bac940f25df19ed99bae725b249a","observation_id":"41359748-c3d9-46a8-b8ba-b919992de430","resolution":{"observed_at":"2026-08-11T22:25:24.335741Z","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":"2026-08-17T17:40:51.773546Z","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":"2026-08-11T22:25:24.339737Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.339737Z"},"links":{"cited_paper":"/paper/2307.15115","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:b9fdd64caab3a62e7852b5f1ed14bbe213c43b3c96760e8a048c89697be7747b","observation_id":"7ae3af88-e4f2-4d9e-a518-d27f1972e9b5","resolution":{"observed_at":"2026-08-11T22:25:24.339737Z","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":"2026-08-16T14:01:46.008228Z","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":"2026-08-11T22:25:24.344376Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.344376Z"},"links":{"cited_paper":"/paper/2404.07714","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:e7b9d3439795bceaa9324a431879dd0fae2f933b1b9edcda02daff62da4e4dea","observation_id":"78da165d-5983-49b7-8e98-f2bb7b9152ee","resolution":{"observed_at":"2026-08-11T22:25:24.344376Z","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":"2026-08-19T10:41:47.015542Z","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":"2026-08-11T22:25:24.348251Z","title":"Telalovic, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.348251Z"},"links":{"cited_paper":"/paper/2406.15506","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:6deedf7ec2eab88ef636b8333327c17da75c082ffdb99dd58f40230bb3ad8a77","observation_id":"1db28f17-abdf-4dda-a41c-40af4bbf6c74","resolution":{"observed_at":"2026-08-11T22:25:24.348251Z","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":"2026-08-11T22:25:24.352185Z","title":"Hardy, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.352185Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:cba0a39b08bf283c2226502b4fe5a53f34ee5a6e91037b171122ab55de8e1628","observation_id":"72541e6d-6ec3-4c79-b6a1-6d6e9ff640f5","resolution":{"observed_at":"2026-08-11T22:25:24.352185Z","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":"2026-08-11T22:25:24.355602Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.355602Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:794f21d8c93ae344866a32324312e8ab1a169a01e89812db847140728251d494","observation_id":"8eea8269-4909-4c72-a195-824609b68169","resolution":{"observed_at":"2026-08-11T22:25:24.355602Z","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":"2026-08-16T23:22:59.822526Z","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":"2026-08-11T22:25:24.358661Z","title":"Caputo and G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.358661Z"},"links":{"cited_paper":"/paper/2401.13728","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:9b103e1bf1f7c5bacfe61763024b1b73a26bec01211109bd75f50486a8dea255","observation_id":"226d5548-122f-4643-8565-cc05ea704898","resolution":{"observed_at":"2026-08-11T22:25:24.358661Z","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":"2026-08-16T13:03:02.405457Z","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":"2026-08-11T22:25:24.361847Z","title":"Carenza, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.361847Z"},"links":{"cited_paper":"/paper/2411.02492","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:4d1ce4faf97f49c0ff353bcf9a20ba541ea7c12bbcca78fd7a85031a54f0de36","observation_id":"199cd88c-06e8-4ca0-afdf-88c81672b18b","resolution":{"observed_at":"2026-08-11T22:25:24.361847Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.06519","last_updated":"2021-05-18T13:20:08Z","snapshot_observed_at":"2026-08-16T19:06:15.663594Z","submitted_at":"2020-11-12T17:32:14Z","title":"Updated BBN constraints on electromagnetic decays of MeV-scale particles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.06519","snapshot_observed_at":"2026-08-11T22:25:24.365600Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.365600Z"},"links":{"cited_paper":"/paper/2011.06519","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:e62cd3d2fdd2e733ce2c126962bb3af9dfa47d2abb5fda04b1f238263df2fa8c","observation_id":"d06df139-603c-4b6b-aa95-6daa421b88fc","resolution":{"observed_at":"2026-08-11T22:25:24.365600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.13549","last_updated":"2022-12-19T15:12:51Z","snapshot_observed_at":"2026-08-17T14:12:20.867574Z","submitted_at":"2022-05-26T18:00:00Z","title":"Cosmological constraints on decaying axion-like particles: a global analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.13549","snapshot_observed_at":"2026-08-11T22:25:24.369270Z","title":"Bal´ azs et al.,Cosmological constraints on decaying axion-like particles: a global analysis , JCAP 12 (2022) 027 [2205.13549]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.369270Z"},"links":{"cited_paper":"/paper/2205.13549","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:3bc3a3dafdd11ef99957e681f01ee6399807a41ab81050f176c226cdad944983","observation_id":"ba557340-8042-4437-b50d-0e4057df3063","resolution":{"observed_at":"2026-08-11T22:25:24.369270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.06216","last_updated":"2022-09-20T14:28:29Z","snapshot_observed_at":"2026-08-16T16:32:46.889341Z","submitted_at":"2022-09-13T18:00:00Z","title":"The Irreducible Axion Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.06216","snapshot_observed_at":"2026-08-11T22:25:24.373153Z","title":"Langhoff, N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.373153Z"},"links":{"cited_paper":"/paper/2209.06216","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:26c240351f735791d8294b69b75ab0ec694a6049513c31c9a612e5a6b6fd05f6","observation_id":"be78a44e-dd55-41b2-aea3-029531f80348","resolution":{"observed_at":"2026-08-11T22:25:24.373153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.6053","last_updated":"2014-10-14T10:33:11Z","snapshot_observed_at":"2026-08-14T23:29:20.903221Z","submitted_at":"2014-06-23T20:00:07Z","title":"Revisiting the bound on axion-photon coupling from Globular Clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.6053","snapshot_observed_at":"2026-08-11T22:25:24.376704Z","title":"Ayala, I","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.376704Z"},"links":{"cited_paper":"/paper/1406.6053","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:f36bfe3ea1e247a6cdf47b74eb33b7892e796e3b4287aa34a9a40ad65d8862fe","observation_id":"ca39a731-ed69-47fb-b308-99e63a776056","resolution":{"observed_at":"2026-08-11T22:25:24.376704Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03102","last_updated":"2022-11-25T05:49:07Z","snapshot_observed_at":"2026-08-16T16:47:45.153421Z","submitted_at":"2022-07-07T05:50:49Z","title":"Advancing Globular Cluster Constraints on the Axion-Photon Coupling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03102","snapshot_observed_at":"2026-08-11T22:25:24.380249Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.380249Z"},"links":{"cited_paper":"/paper/2207.03102","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:7f59dfd050530a5c9476c3571179ce73e3765b443b3261e3691ba6b8b07c57f6","observation_id":"2836a523-ea01-41ab-95c2-ea391b5454fe","resolution":{"observed_at":"2026-08-11T22:25:24.380249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.11216","last_updated":"2023-10-19T23:22:49Z","snapshot_observed_at":"2026-08-16T15:14:31.379245Z","submitted_at":"2023-07-20T20:03:46Z","title":"Spectra of axions emitted from main sequence stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.11216","snapshot_observed_at":"2026-08-11T22:25:24.384019Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.384019Z"},"links":{"cited_paper":"/paper/2307.11216","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:5805de7504b14885727cfbd04f7ed4fde1761e16da34890b4f2f6fde7cbb46a1","observation_id":"c425825e-bf54-4b3b-a190-27202783b1d2","resolution":{"observed_at":"2026-08-11T22:25:24.384019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.12431","last_updated":"2020-06-22T16:57:39Z","snapshot_observed_at":"2026-08-12T20:32:40.137338Z","submitted_at":"2020-06-22T16:57:39Z","title":"Stellar Basins of Gravitationally Bound Particles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.12431","snapshot_observed_at":"2026-08-11T22:25:24.387985Z","title":"Van Tilburg, Stellar basins of gravitationally bound particles, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.387985Z"},"links":{"cited_paper":"/paper/2006.12431","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:dc9512e1a3be4a33767b4fb55ad75b2f1169653f102d87e0b81fe7232b7af840","observation_id":"276b30c9-a596-4aad-8828-686c8d0b5ffb","resolution":{"observed_at":"2026-08-11T22:25:24.387985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.06968","last_updated":"2023-06-19T09:22:37Z","snapshot_observed_at":"2026-08-16T15:48:45.451173Z","submitted_at":"2023-03-13T10:09:46Z","title":"New solar X-ray constraints on keV Axion-Like Particles","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.06968","snapshot_observed_at":"2026-08-11T22:25:24.391726Z","title":"Beaufort, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.391726Z"},"links":{"cited_paper":"/paper/2303.06968","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:70518b04a382314e8c8fd142ce64d9737756db14d61b9ab3b0d845b5d0bb6f94","observation_id":"f3ae9d81-53a8-49b6-8792-1f461c5dc2bc","resolution":{"observed_at":"2026-08-11T22:25:24.391726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.10327","last_updated":"2024-03-08T17:02:34Z","snapshot_observed_at":"2026-08-16T15:32:17.677819Z","submitted_at":"2023-05-17T16:07:40Z","title":"Multimessenger Constraints on Radiatively Decaying Axions from GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.10327","snapshot_observed_at":"2026-08-11T22:25:24.395616Z","title":"Diamond, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.395616Z"},"links":{"cited_paper":"/paper/2305.10327","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:64e50e829d3ad20a15200c0ad844b966ccad8a6efdf827ed159da7805e226f48","observation_id":"22e157e1-2705-40e4-8900-31f7db6d9267","resolution":{"observed_at":"2026-08-11T22:25:24.395616Z","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":"2026-08-11T22:25:24.399449Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.399449Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:193e0b3e337ea5abf34d1815823f9469f222869a0a04a9b1aa497b9ab2b893fd","observation_id":"8980f690-da27-404c-ab16-df1f68d11ec2","resolution":{"observed_at":"2026-08-11T22:25:24.399449Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.526429Z","title":"O’Hare, cajohare/axionlimits: Axionlimits , https://cajohare.github.io/AxionLimits/, July,","venue":null,"work_id":"c4518498-ebee-4583-9d6c-6903dcddcc77","year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.403412Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:30d09c05193eb41357869b9755e107ac4b3539797ce44e01cd3df8d4f87b2e2c","observation_id":"8ea4f959-7c9a-445a-82a0-7a54389807f9","resolution":{"observed_at":"2026-08-11T22:25:25.530879Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1301.7307","last_updated":"2013-01-30T17:48:36Z","snapshot_observed_at":"2026-08-18T01:26:06.579259Z","submitted_at":"2013-01-30T17:48:36Z","title":"The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.7307","snapshot_observed_at":"2026-08-11T22:25:24.411701Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.411701Z"},"links":{"cited_paper":"/paper/1301.7307","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:b251d4b8217ea4572dc931a8c3c84904c510b3e02db8c9dd5783f0c1225e8a5b","observation_id":"c2fb5609-3416-40f2-b5dd-16140b286951","resolution":{"observed_at":"2026-08-11T22:25:24.411701Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.514844Z","title":null,"venue":null,"work_id":"1846b5ae-6040-47ea-8a00-f597f28fa6a5","year":1980},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.415624Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:78ec97c4ae3cfdb817a37c23cd43d1ed765826d870cd35e5138b97c9db786344","observation_id":"cfd84e58-0cc5-491e-a6ef-4df11222abea","resolution":{"observed_at":"2026-08-11T22:25:25.518703Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.502533Z","title":null,"venue":null,"work_id":"c1c5616d-8f5b-41f0-b59b-90ca2228557b","year":1986},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.419228Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:d40f61889edf23551f0d592062b463ffc89c38c6b77aaa7d25967a7df15294f5","observation_id":"2e980461-10e5-46d4-a181-ac24567fe0ef","resolution":{"observed_at":"2026-08-11T22:25:25.506792Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0006327","last_updated":"2000-10-09T16:40:32Z","snapshot_observed_at":"2026-07-07T03:48:58.012801Z","submitted_at":"2000-06-28T20:03:47Z","title":"Search for solar Kaluza-Klein axions in theories of low-scale quantum gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0006327","snapshot_observed_at":"2026-08-11T22:25:24.422798Z","title":"Di Lella, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.422798Z"},"links":{"cited_paper":"/paper/hep-ph/0006327","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:b726bcf32422718b504fb24f0f3e2c95b40f2be6a8ee1bec2e7d83c7c9d90521","observation_id":"ef78e18e-2520-4141-8293-f262e6ff2dc4","resolution":{"observed_at":"2026-08-11T22:25:24.422798Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.08399","last_updated":"2020-09-03T06:13:12Z","snapshot_observed_at":"2026-08-12T15:48:39.215843Z","submitted_at":"2020-04-17T18:00:06Z","title":"Constraints on the coupling with photons of heavy axion-like-particles from Globular Clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.08399","snapshot_observed_at":"2026-08-11T22:25:24.426387Z","title":"Carenza, O","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.426387Z"},"links":{"cited_paper":"/paper/2004.08399","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:135b3a3b4ffc95c12fc6f5a9caeb1a4098fd9e8b984075834c51bc72b61ffb7f","observation_id":"ed627f23-5a28-4b0d-91cf-7f202c906d96","resolution":{"observed_at":"2026-08-11T22:25:24.426387Z","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":"2026-08-11T22:25:24.429611Z","title":"Lucente, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.429611Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:a26c143566a64d31647518a32ed974f082ab4526a6ed5e81d19616404166ec43","observation_id":"7c4a9b11-4973-4833-acf0-e1e2e5fb932e","resolution":{"observed_at":"2026-08-11T22:25:24.429611Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.490868Z","title":null,"venue":null,"work_id":"4d86df2f-fc8d-4eeb-83bc-b35b7b84d0bb","year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.432644Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:afdbe222613dae239bfab0217aa1aba99f28801f16c37223ac3712bdd8211c77","observation_id":"e9eabd00-8e54-4756-831b-eb29c00bfa6c","resolution":{"observed_at":"2026-08-11T22:25:25.494691Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1009.1622","last_updated":"2010-09-08T20:00:05Z","snapshot_observed_at":"2026-08-15T05:09:18.642020Z","submitted_at":"2010-09-08T20:00:05Z","title":"Modules for Experiments in Stellar Astrophysics (MESA)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.1622","snapshot_observed_at":"2026-08-11T22:25:24.435915Z","title":"Paxton, L","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.435915Z"},"links":{"cited_paper":"/paper/1009.1622","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:6c1adaf24372df2a7f642f1cf6248c748277ccead4ae93632eb29fc84231990d","observation_id":"743a6f56-516c-4aef-ac22-3487d9deed11","resolution":{"observed_at":"2026-08-11T22:25:24.435915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0319","last_updated":"2013-06-12T19:42:55Z","snapshot_observed_at":"2026-08-12T19:03:26.795307Z","submitted_at":"2013-01-02T21:00:00Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.0319","snapshot_observed_at":"2026-08-11T22:25:24.439667Z","title":"Paxton et al., Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, 7 and Massive Stars , Astrophys","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.439667Z"},"links":{"cited_paper":"/paper/1301.0319","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:fee0fe6473e2a093dee6f1615b2f56ce2c4d60d2fcf1be16319dd85d439f4844","observation_id":"fbba4c94-54d0-48d3-afff-d7b853176797","resolution":{"observed_at":"2026-08-11T22:25:24.439667Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14476","last_updated":"2024-04-22T18:00:00Z","snapshot_observed_at":"2026-08-17T19:45:07.213157Z","submitted_at":"2024-04-22T18:00:00Z","title":"Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.14476","snapshot_observed_at":"2026-08-11T22:25:24.443285Z","title":"Ning and B","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.443285Z"},"links":{"cited_paper":"/paper/2404.14476","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:b2d0378cb455c7d2cec74d1afa9afec74f1369e71a85e2e6257d982b12b2ce9d","observation_id":"6c842823-59a3-4f4f-9a5d-dd79dca565f2","resolution":{"observed_at":"2026-08-11T22:25:24.443285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0309357","last_updated":"2003-09-12T14:41:18Z","snapshot_observed_at":"2026-08-19T11:23:33.359324Z","submitted_at":"2003-09-12T14:41:18Z","title":"The Nature of Starburst Activity in M82","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0309357","snapshot_observed_at":"2026-08-11T22:25:24.446620Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.446620Z"},"links":{"cited_paper":"/paper/astro-ph/0309357","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:2f53ce17f901e146dfcf980c11c7c4ba8e173bd724d6495b5f36ba369aa0e1b9","observation_id":"cd9cb7c9-f936-48ee-af11-e259ba453d46","resolution":{"observed_at":"2026-08-11T22:25:24.446620Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.479611Z","title":null,"venue":null,"work_id":"04226572-fd71-4797-98ab-5344a2766278","year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.449893Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:86c9d7daaccbf4ea24f33f1560893e65280ccaa6ee600c80aea5716db865f2a6","observation_id":"2f5db33b-8ccd-4cb0-90a5-38bec42ee310","resolution":{"observed_at":"2026-08-11T22:25:25.483544Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.467412Z","title":null,"venue":null,"work_id":"5e34a2aa-099e-4f9f-baca-d7d91b993e38","year":2014},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.453075Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:e0decef34650bd8de686a9b7a9c44897db8bd8b2f9f8e0dbaa4d3c571e1e3208","observation_id":"05e6c55d-9776-46b7-9dd0-ffe77b67a883","resolution":{"observed_at":"2026-08-11T22:25:25.471763Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.456208Z","title":"Astrophysics Source Code Library, record ascl:1408.004","venue":null,"work_id":"28e09c9b-3fcc-4bb0-94bb-8a31dd05fe59","year":2014},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.456274Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:4fff7bc2d783f78d7f482b8ec3bd5336b98678818db9e68aff93e696a2941c39","observation_id":"0e8a30ab-6ac3-480e-bdb7-8ad0f5229bb7","resolution":{"observed_at":"2026-08-11T22:25:25.459725Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1007.1727","last_updated":"2013-06-24T14:20:41Z","snapshot_observed_at":"2026-08-13T20:03:05.337756Z","submitted_at":"2010-07-10T15:48:35Z","title":"Asymptotic formulae for likelihood-based tests of new physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.1727","snapshot_observed_at":"2026-08-11T22:25:24.459358Z","title":"Cowan, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.459358Z"},"links":{"cited_paper":"/paper/1007.1727","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:b48c98ed5cbbea11d335b3df1d00193f3c72f7d9b50f53de0d81edbe0c02df2a","observation_id":"e99b104e-7762-498b-bd45-3c1a0a495a37","resolution":{"observed_at":"2026-08-11T22:25:24.459358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.16065","last_updated":"2025-06-12T06:21:45Z","snapshot_observed_at":"2026-08-16T13:07:22.658157Z","submitted_at":"2024-10-21T14:45:25Z","title":"Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri","version":2},"cited_work":{"arxiv_id":"2410.16065","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.16065","snapshot_observed_at":"2026-08-11T22:25:24.642495Z","title":"Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri","venue":"astro-ph.HE","work_id":"f9226b64-2fbd-41c0-a1d6-f6919caa30f2","year":2024},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.462799Z"},"links":{"cited_paper":"/paper/2410.16065","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:ecdaeebaf1ba22a5ea23c6fde1868d33b39bb3f128f9eb6a576305d700753aba","observation_id":"59a4d1aa-3ae6-4868-a620-ef42e7a100a5","resolution":{"observed_at":"2026-08-11T22:25:24.648632Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401361","last_updated":"2004-01-19T11:25:57Z","snapshot_observed_at":"2026-07-07T00:39:50.327348Z","submitted_at":"2004-01-19T11:25:57Z","title":"Stellar and gaseous abundances in M82","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401361","snapshot_observed_at":"2026-08-11T22:25:24.467037Z","title":"Origlia, P","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.467037Z"},"links":{"cited_paper":"/paper/astro-ph/0401361","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:7beb3f05646e31af3cdab542991f45953ebb35b071e82d3db6888ad9848eca4e","observation_id":"7485c9bf-27e7-4e37-a4b2-14e1822eb291","resolution":{"observed_at":"2026-08-11T22:25:24.467037Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.444484Z","title":null,"venue":null,"work_id":"f5bdb4a3-b71e-4c1a-a60f-c7bb33dd4b0b","year":1996},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.470843Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:514c338c7f7e29b5a4bb8dba41eea560b36951e36977e3deec9119113ab0fac3","observation_id":"2ccd9cc4-348e-4315-b9c1-3b51a4570f66","resolution":{"observed_at":"2026-08-11T22:25:25.448370Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:24.474693Z","title":"Oberauer, C","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.474693Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:60ac35b2421fe2d2cd4b52041591e12b3b3d16487c30fee89aa8bc6979ea139e","observation_id":"d03d3d38-8705-4989-822f-284ab673592c","resolution":{"observed_at":"2026-08-11T22:25:24.474693Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.423707Z","title":"Blackburn, Ftools: A fits data processing and analysis software package, in Astronomical Data Analysis Software and Systems IV , vol","venue":null,"work_id":"158df36e-dd8a-44ca-84d5-6c23dd21b073","year":1995},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.478553Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:1ca0d9541594b2f640238d1c88ae75df2b417136bacea194179b4bdab8d59790","observation_id":"3a398b67-915b-4ff7-a5e5-4c124d808c44","resolution":{"observed_at":"2026-08-11T22:25:25.427461Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.411963Z","title":"Arnaud and et al., Xspec: An x-ray spectral fitting package, Astrophysics Source Code Library (1999) ascl","venue":null,"work_id":"bc44392f-f754-4b04-aa38-371d14d227de","year":1999},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.482260Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:ea1d85ebe9b237425ac1afb493045f8b34259971be9aa28f98fb38e776de6432","observation_id":"0c0594b0-3869-4145-b001-e9809b6fdd9e","resolution":{"observed_at":"2026-08-11T22:25:25.416142Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.400851Z","title":null,"venue":null,"work_id":"3fca5d17-7a63-44bd-aca8-21a4117dcfdc","year":2014},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.485969Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:740afeeb99559168079ab234e31ba7251bdcca3b8c9ffeb7ef27a8f7b2c9cf40","observation_id":"a1dff78b-2202-4c8c-89f9-36297e38d0d4","resolution":{"observed_at":"2026-08-11T22:25:25.404516Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.389533Z","title":"Krivonos, D","venue":null,"work_id":"26f7ec48-bf1b-4a46-9ca4-aefa92b7e38c","year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.490205Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:e22629bc2ec35a222cf9a8cd88c0567f46b3e17c2e37363fa3926539f53c930d","observation_id":"151e620d-30e6-4ea8-8928-ebd066394ec2","resolution":{"observed_at":"2026-08-11T22:25:25.393378Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.377288Z","title":"Bergsma et al., Search for Axion Like Particle Production in 400-GeV Proton - Copper Interactions, Phys","venue":null,"work_id":"85836499-8b9d-4ad0-8308-d3f155b3c2b3","year":1985},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.493906Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:da0d7b740f3756d38e03377bb5bc995019a8f2718404aae9ccb0783c3a546837","observation_id":"10f01643-ec11-4c5e-9f58-ddf12a10e8b2","resolution":{"observed_at":"2026-08-11T22:25:25.381183Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:24.497694Z","title":null,"venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.497694Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:bfe248d47f231c5df295af2357e4bcf5cc978dc688bef6199c1e3847fd0a9c64","observation_id":"e7b71047-ee63-4b32-b074-0c998dd4e987","resolution":{"observed_at":"2026-08-11T22:25:24.497694Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.358211Z","title":"Blumlein et al., Limits on neutral light scalar and pseudoscalar particles in a proton beam dump experiment, Z","venue":null,"work_id":"1d11c508-6e71-4967-8ea6-1f6aac878071","year":1991},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.501217Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:34121c3401e29373a93ed9b070c21bd8df0d881790d6d16e0cae2ea37ad60cb9","observation_id":"17c7fa37-fe06-4f4c-b389-18431ceb37b8","resolution":{"observed_at":"2026-08-11T22:25:25.362164Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.02710","last_updated":"2020-08-02T16:53:08Z","snapshot_observed_at":"2026-08-09T06:21:12.814595Z","submitted_at":"2020-05-06T10:33:32Z","title":"Search for Axionlike and Scalar Particles with the NA64 Experiment","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.02710","snapshot_observed_at":"2026-08-11T22:25:24.504826Z","title":"Banerjee et al., Search for Axionlike and Scalar Particles with the NA64 Experiment, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.504826Z"},"links":{"cited_paper":"/paper/2005.02710","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:b99485c3b04ea918f7506836f300fdba746c166b07c9a93a9fbb3595e6003300","observation_id":"14501862-d955-4413-bd8b-7a467ea4034a","resolution":{"observed_at":"2026-08-11T22:25:24.504826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.00009","last_updated":"2018-01-04T11:05:13Z","snapshot_observed_at":"2026-08-19T12:56:58.129941Z","submitted_at":"2017-08-31T18:00:02Z","title":"Revised constraints and Belle II sensitivity for visible and invisible axion-like particles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.00009","snapshot_observed_at":"2026-08-11T22:25:24.508114Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.508114Z"},"links":{"cited_paper":"/paper/1709.00009","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:71b9a4580a14da4373cc9541fc193b0437e1d27625ad40d9c850d87601358e0b","observation_id":"99830adf-9005-46bd-b434-96f0df0f0a43","resolution":{"observed_at":"2026-08-11T22:25:24.508114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03878","last_updated":"2023-07-11T17:04:44Z","snapshot_observed_at":"2026-08-16T15:17:49.371449Z","submitted_at":"2023-07-08T01:48:03Z","title":"New Constraints on ALP Electron and Photon Couplings from ArgoNeuT and the MiniBooNE Beam Dump","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03878","snapshot_observed_at":"2026-08-11T22:25:24.511660Z","title":"Capozzi, B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.511660Z"},"links":{"cited_paper":"/paper/2307.03878","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:55ae1419057d2c0d7a2836b1aae526fe1f87ac7ad3060cb6edebb97c8a5b62e7","observation_id":"0d28d741-58aa-44cb-9025-ee3fcaeff19c","resolution":{"observed_at":"2026-08-11T22:25:24.511660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01639","last_updated":"2015-07-29T20:12:48Z","snapshot_observed_at":"2026-08-14T23:04:53.814323Z","submitted_at":"2015-01-07T21:00:12Z","title":"New axion and hidden photon constraints from a solar data global fit","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01639","snapshot_observed_at":"2026-08-11T22:25:24.514875Z","title":"Vinyoles, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.514875Z"},"links":{"cited_paper":"/paper/1501.01639","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:a66f5b2a4a1b5dd415129bf77b639ad360a40585763674146fc5e461c7f9b831","observation_id":"e18895f9-2dda-49f8-bd1a-1e7f963b665b","resolution":{"observed_at":"2026-08-11T22:25:24.514875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.00379","last_updated":"2021-09-15T10:42:09Z","snapshot_observed_at":"2026-08-16T18:48:48.081863Z","submitted_at":"2021-01-31T05:05:19Z","title":"Constraining axion-like particles using the white dwarf initial-final mass relation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.00379","snapshot_observed_at":"2026-08-11T22:25:24.518242Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.518242Z"},"links":{"cited_paper":"/paper/2102.00379","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:c3f3be6c30eb28a95cc87494370f20a462e06d0a71298851efae745736ad0f33","observation_id":"dfa471cd-e751-4dd9-8b90-45dcd07f5118","resolution":{"observed_at":"2026-08-11T22:25:24.518242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.01403","last_updated":"2023-10-03T09:36:44Z","snapshot_observed_at":"2026-08-16T15:11:13.928870Z","submitted_at":"2023-08-02T19:53:40Z","title":"Supernova Simulations Confront SN 1987A Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.01403","snapshot_observed_at":"2026-08-11T22:25:24.521490Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.521490Z"},"links":{"cited_paper":"/paper/2308.01403","citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:11765c949941e215904b110a38348af5ef010dd523f3217e66a7b6c6a5e45d73","observation_id":"5dbd75f5-00e5-4ed0-8b7e-3b57d697b00e","resolution":{"observed_at":"2026-08-11T22:25:24.521490Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.344920Z","title":"S5, where β is the polar angle at the detection point, while θ is the polar angle at the decay point","venue":null,"work_id":"f9c857fc-cddc-4172-a5ed-bdc6523d0c28","year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.524940Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:5b85bafcfc61fe857f67c5f82032929a44e227551085ca99362ec460a538f808","observation_id":"73de68bc-163e-4974-9bc7-ec55e6e677a6","resolution":{"observed_at":"2026-08-11T22:25:25.349204Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:25.332735Z","title":"two-burst","venue":null,"work_id":"cf4cbec1-3f3b-4f41-886f-04f3b02b3a7d","year":2012},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.527957Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:2a9395eaed53c1c98807b04067fc89df27f1d81b4c4d21e2d5668a09284a0dcd","observation_id":"0feddd35-22c5-4822-947e-072d8ef6ea9f","resolution":{"observed_at":"2026-08-11T22:25:25.336803Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:25:24.407635Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82","version":2},"reference_index":2020,"source":"pdf_text","source_observed_at":"2026-08-11T22:25:24.407635Z"},"links":{"citing_paper":"/paper/2412.03660"},"observation_digest":"sha256:55d60990ed53e3ec9c580dad8a90f0f29e0e3f98845210936d98d80f2668d8f2","observation_id":"d16efc79-945e-41d3-be4a-56c711ac6ad6","resolution":{"observed_at":"2026-08-11T22:25:24.407635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.03660","last_updated":"2025-05-04T12:22:49Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-17T05:14:47.314624Z","submitted_at":"2024-12-04T19:00:05Z","title":"NuSTAR bounds on radiatively decaying particles from M82"},"reference_resolution":{"displayed":74,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":64,"verified_exact":1,"verified_fuzzy":9},"total_outbound_references":74},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 12 inbound Pith citation observations for arXiv:2412.03660."}