{"as_of":"2026-08-17T16:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9ecdb9c1875c6b396d23136ec0cfae34ca4b7a7b7433dcfbf8edd09383015273","coverage":[{"denominator":81,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":81,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:03:06.856926Z","state":"measured"},{"denominator":82,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":82,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T13:07:51.676302Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.12636","snapshot_observed_at":"2026-08-01T13:07:51.676302Z","title":"and Benson, Andrew J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19244","last_updated":"2026-07-21T16:15:17Z","snapshot_observed_at":"2026-08-15T15:18:50.209233Z","submitted_at":"2026-07-21T16:15:17Z","title":"Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.676302Z"},"links":{"cited_paper":"/paper/2501.12636","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:c6a507933fa3c11db3f30f0338e34099817afd3c79882c2c1efa905ed4f16835","observation_id":"93aa061e-57a2-4f4b-beae-a0862c8d5707","resolution":{"observed_at":"2026-08-01T13:07:51.676302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2501.12636/citation-record","integrity":"/paper/2501.12636/integrity","json":"/paper/2501.12636/citation-record.json","paper":"/paper/2501.12636"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:03:06.424041Z","title":"Hambye, PoS IDM2010, 098 (2011)","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.424041Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:9c6e8521e9b97b924379e9202d6927dd0f1ae2b51c9e8a5fac4d557cfdec85ce","observation_id":"ed95510e-f1ae-4343-ad86-95dcb9a237c6","resolution":{"observed_at":"2026-08-10T17:03:06.424041Z","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":"2026-08-10T17:03:08.538856Z","title":null,"venue":null,"work_id":"8ec3e0e2-3f70-4526-9f8e-21dfcdf33325","year":2003},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.431520Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:9dac0a95a4f1213d13f2979b02e5a72cd4bca2250c32b9c81a289028491b3bde","observation_id":"3a872150-fd2d-481b-9414-53e2146beeb5","resolution":{"observed_at":"2026-08-10T17:03:08.543709Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.524578Z","title":null,"venue":null,"work_id":"63ce510d-6ac4-42ed-9735-78cb19a6aa51","year":2007},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.437156Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:59dce8830821140f339a2fc4421c9bb4679f52136d375645f120a214f24b3279","observation_id":"f29fd6ff-7900-47c0-a4eb-1e39db615ddc","resolution":{"observed_at":"2026-08-10T17:03:08.529355Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.509826Z","title":null,"venue":null,"work_id":"ee754892-ed37-405d-a5f3-7f059e30d3c7","year":2010},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.444118Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:1ff455447a20afd1f32436328fbbc885d452ec8d55f37bad7a77afc58219fc19","observation_id":"35c1f402-09a2-478b-b5d2-c03ab1183280","resolution":{"observed_at":"2026-08-10T17:03:08.514283Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.494307Z","title":"Pagels and J","venue":null,"work_id":"c8ac7a6b-a27a-48cb-afef-cee676aed0fb","year":1982},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.449665Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:38ed46fe6c71001636781b786719e592bc067a663ea1a1eb906738007b801f99","observation_id":"13a7aa68-a8bf-42ad-a84d-c0f07331aabf","resolution":{"observed_at":"2026-08-10T17:03:08.498967Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.479034Z","title":"Weinberg, Phys","venue":null,"work_id":"c09aba3e-a1b1-43f9-8156-7d34fe6aa4f4","year":1982},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.455704Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:3fe15c08df313f51c94c419f6011aa51b6c95edcfcb79be13e58447306711d11","observation_id":"ed0e802f-7b53-4492-9bb4-46f8a5f40482","resolution":{"observed_at":"2026-08-10T17:03:08.483891Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.463108Z","title":"Berezinsky, A","venue":null,"work_id":"cad931b2-9c04-44de-9e8f-a50182d42b4b","year":1991},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.460849Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:29bb7faeaf611e6b820a592710df82a8883a5c684b482ae2675f5f8348e522ab","observation_id":"3ea1208c-e079-4d0b-8fbf-8fac6f25681a","resolution":{"observed_at":"2026-08-10T17:03:08.467935Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.446513Z","title":null,"venue":null,"work_id":"f923532d-4486-4384-8c3c-cfef654a6106","year":1999},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.465284Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:041e5fbbdf603e055743d0081cdcc4623067af2122eec74a2202f604645e9e70","observation_id":"bbc970f6-2df8-469e-8276-e842474e18c1","resolution":{"observed_at":"2026-08-10T17:03:08.452101Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.429444Z","title":null,"venue":null,"work_id":"977c1e03-b96b-465f-a44f-1d99c3a9e68c","year":2003},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.469867Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:7d731d06a513a554eb595bedc10aa9682108161d4c57939918920a853c0f8941","observation_id":"681ac4c6-18c1-4004-ba55-667129f44b3d","resolution":{"observed_at":"2026-08-10T17:03:08.434463Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.413304Z","title":"Kaplinghat, Phys","venue":null,"work_id":"8e108133-b48c-44fb-8147-dc5ca394f058","year":2005},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.474333Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:9f028dd433a8cc3b10ae826f7c7a4ec502bab42855510a8efde6aaf330cf3cb5","observation_id":"353ecfdf-671d-4949-a2ec-f42dc7de6df4","resolution":{"observed_at":"2026-08-10T17:03:08.418532Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.396973Z","title":"Allahverdi, B","venue":null,"work_id":"90def61e-7fa7-4c9e-8d5a-da11754c43bb","year":2015},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.479638Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:a22060a57876af06f926eb456548f038081bb3412da4ec5cc1b2d14f6d820f80","observation_id":"cfdb8094-97f3-4b1f-bd0f-7db3c3132293","resolution":{"observed_at":"2026-08-10T17:03:08.402458Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.381386Z","title":"Abazajian, G","venue":null,"work_id":"750cb6e7-8d1d-455f-96fa-b249d8e630df","year":2003},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.484617Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:ed0df7ec29f1787dafd497e714ba3c18d2afcdc94d70b844adeb4b97e9b96c85","observation_id":"6db9e327-5fa8-44fe-9c78-ab7f877168e5","resolution":{"observed_at":"2026-08-10T17:03:08.386347Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.364790Z","title":"Gonzalo, M","venue":null,"work_id":"d2101a47-54c7-4a1f-b487-5dd7bdde4e96","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.490082Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:e41457eb9b325e727eeb978808d0db288c3f34272c62d4f1d2f722e5de4b8735","observation_id":"890120da-5b8d-4c54-b7d0-9b291efbdb29","resolution":{"observed_at":"2026-08-10T17:03:08.370235Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.346498Z","title":null,"venue":null,"work_id":"502873d7-66d0-4c02-bf40-3a935fd48e6a","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.494820Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:fdd9d1ab80be424527af53c2e2bd00b84720b4fc0bc45592d56218d452c9d792","observation_id":"bb012e47-ec51-4c6b-b9e5-f23ff5c5562a","resolution":{"observed_at":"2026-08-10T17:03:08.352622Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.329732Z","title":"Obied, C","venue":null,"work_id":"15f52c16-a241-43fd-9e9e-45670406c434","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.499868Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:1747b32c6a87adae805aa8a29814f59aae8dbe22a3563bfd4dc9a160a9c13fd1","observation_id":"115efc8a-8d75-4dcd-bbe7-ff167799ce28","resolution":{"observed_at":"2026-08-10T17:03:08.334844Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.312339Z","title":"McKeen, J","venue":null,"work_id":"10393012-0a39-46e9-b158-2ed507f5983c","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.504653Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:92ed67c90e5e68164a2c5f5f2c68559fe8cebbc1b9c97fcce3b5447a7ba708bf","observation_id":"57b00203-1c38-41a7-9cde-c64f3f119f9e","resolution":{"observed_at":"2026-08-10T17:03:08.317579Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.292661Z","title":"Chen and M","venue":null,"work_id":"21759af2-a7ab-492a-8870-24f9f344e6c0","year":2004},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.509536Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2acace489f616d7d477a5605c586fcd092bfa58b5b0eac9eb0a4184fd5226dfd","observation_id":"d6d2a28f-af2f-453c-bc68-79295973f0e2","resolution":{"observed_at":"2026-08-10T17:03:08.298323Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.277377Z","title":null,"venue":null,"work_id":"c1f97d88-4c49-4122-9557-532cd75df921","year":2016},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.514472Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:32a128c0d047f18dd966f20f069beb057bf50e8aeb5602413dfa0961c631dec6","observation_id":"f41a2710-9520-46c9-89a2-858c186bfa09","resolution":{"observed_at":"2026-08-10T17:03:08.281930Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.261188Z","title":"Poulin, P","venue":null,"work_id":"2b8116ff-d2ab-4133-9970-da08233beb4d","year":2016},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.519421Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:01cc77c97589c014d2a59587a2b56149120db8d543bde8523fe2585d269246f0","observation_id":"8030498e-e3bf-4bbd-9567-4fb887deff9b","resolution":{"observed_at":"2026-08-10T17:03:08.266426Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.244551Z","title":null,"venue":null,"work_id":"b8102a56-7067-431e-8ddd-065c744ad79c","year":2017},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.524229Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:ba66fd932ffb12cdf6ad46ad3b4ec93ce50116abf301e50a0af89de3d1efb4d2","observation_id":"46bd1110-b308-4043-885b-b19d55e261a2","resolution":{"observed_at":"2026-08-10T17:03:08.249062Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.225929Z","title":"Chen et al","venue":null,"work_id":"e1ea5625-82e1-418a-8765-3a23039e582e","year":2021},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.529433Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2decb9376a99978d1fc079d973285ca516a935618c8d587ecfbac157184028ae","observation_id":"13d45de6-abc7-4426-bed6-91a40cf09d9d","resolution":{"observed_at":"2026-08-10T17:03:08.232174Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.206226Z","title":"Nygaard, T","venue":null,"work_id":"731added-69dc-440c-b7a8-6fe62858437d","year":2021},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.536513Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:22b70bccffdf78715e1608153179d010da3f31ea1b5a4f10c0b2db793b2d3944","observation_id":"003de571-4061-415f-be6a-3186e0499091","resolution":{"observed_at":"2026-08-10T17:03:08.211897Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:06.542980Z","title":"Nygaard, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.542980Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:c09ba729bc6f1c18cff4d11e46880fb900bcc0b0550d48071e5a24177a6ff867","observation_id":"259e33e1-1cda-4dbb-ba1f-afcb6295fe50","resolution":{"observed_at":"2026-08-10T17:03:06.542980Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:03:08.184096Z","title":"Bucko, S","venue":null,"work_id":"495d1bc1-085d-4986-8f35-1cd4f4f8c56e","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.549095Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:d556261f2694b3fdd7a758db306c2334d6762c76b2da000dda0edfb7187fc8fa","observation_id":"39226e1a-ee5c-4fe6-b58e-0f615ea748bd","resolution":{"observed_at":"2026-08-10T17:03:08.189489Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.167437Z","title":"Simon, G","venue":null,"work_id":"ee2bcac0-bd5a-4a90-9842-8302906da8be","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.554936Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:3875b7066b73c728f45283eba582aa6ac4abae49640d6963b7164b80d6335ee8","observation_id":"97e77eb2-9009-4648-ab5b-b24004f4fcdb","resolution":{"observed_at":"2026-08-10T17:03:08.172844Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.147485Z","title":null,"venue":null,"work_id":"dbbb9c45-078e-4f03-913e-06cface6b335","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.560755Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2ad155a7389d7f9a3d49266740f050c32dd19ba6dd81615c8647d55f31d9876b","observation_id":"6d7aec9d-1302-4fd6-958d-085fdd3907a6","resolution":{"observed_at":"2026-08-10T17:03:08.153884Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.126847Z","title":null,"venue":null,"work_id":"ff7975c9-46a5-4dd1-89bd-6143b7d23ddc","year":2021},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.568022Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2da7e4836a5805c28e4829f9b55f80774d585571d732b9297aba985d9665e34a","observation_id":"f48b41dc-0470-4f28-815d-ec02451f45b3","resolution":{"observed_at":"2026-08-10T17:03:08.132104Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.110453Z","title":"Franco Abell´ an, R","venue":null,"work_id":"db55f439-8d9f-423e-a58f-de192c428d7e","year":2021},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.573418Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:aeab0d197d797d6179b9f19eb4193f745f8ee5e44c42c70a97e6193799e47949","observation_id":"65d3b2c8-af0b-479c-a928-6ddbe256348c","resolution":{"observed_at":"2026-08-10T17:03:08.115763Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.093030Z","title":"Bucko, S","venue":null,"work_id":"fd05d9ca-75b8-426e-8b94-259e80403d48","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.578810Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:5e209b4ccf33d939d6f6fd70dece64e2e6b42f2560c12f8e9e27385f197fb8a7","observation_id":"b78aeaf4-61f5-4442-b3da-95a5f30ce5d4","resolution":{"observed_at":"2026-08-10T17:03:08.098537Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.076664Z","title":"Vattis, S","venue":null,"work_id":"efc65255-bc56-4d95-ae4b-39b043c7bcef","year":2019},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.584184Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:65b7d0b70cbf997d1d0e1524fa6c3b9f85fbfb2770566830cb5b586f936b9cb8","observation_id":"57b9ad20-f69e-4980-b013-dbcd7471513e","resolution":{"observed_at":"2026-08-10T17:03:08.081779Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.060507Z","title":"Abdalla et al., JHEAp 34, 49 (2022)","venue":null,"work_id":"9801c379-853b-49ea-87a2-9200d757c9c8","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.589917Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2fd86ab8061d3658a394d64dbaf70e7feb982691123dafdf401b961c5b6a476a","observation_id":"2e4f1ebb-3485-438e-b204-487d42183300","resolution":{"observed_at":"2026-08-10T17:03:08.065065Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.043377Z","title":"Tanimura, M","venue":null,"work_id":"8fbafc0f-e425-4759-a9b4-94005a54a497","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.594968Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:579cda317796af07443d77fbc3b4f6ef7b8c0d48b81b343b7f19488b767eb48e","observation_id":"7a221a37-3393-429f-9bf9-c2f8b52d6c3e","resolution":{"observed_at":"2026-08-10T17:03:08.049207Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.027568Z","title":null,"venue":null,"work_id":"1b3920f1-7f30-4b7f-a3d0-5dc44b6906f4","year":2025},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.600704Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:4d91588141ffb9dee25d018df8d69d98480bdc0bb95ed10915ea0cbfdf9d0228","observation_id":"b3e6e475-435b-445c-b5cb-a90209a1b19c","resolution":{"observed_at":"2026-08-10T17:03:08.032159Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:08.009857Z","title":null,"venue":null,"work_id":"c1a60ae3-08d1-4796-aa3c-4e13f3cc469b","year":2010},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.608004Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:55a00b754eb339f3b9e1fc0a2da2af62d8cc638f62c15ce4e8f605b8d8aa9dec","observation_id":"3d5f44aa-5334-4266-87fa-995b44fef619","resolution":{"observed_at":"2026-08-10T17:03:08.015444Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.989027Z","title":null,"venue":null,"work_id":"fe66cde3-d48c-4539-aa06-33bb7454e33c","year":2014},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.614491Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:ca950ea43dda9fe6283b700ce8712f0c61a05717d222eda77886fb8bfb8a8bda","observation_id":"04347045-6d12-4c81-bd42-bc1db293dd7c","resolution":{"observed_at":"2026-08-10T17:03:07.995712Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.972451Z","title":null,"venue":null,"work_id":"a97c6f55-9efa-4cb4-ac10-6a197a774a73","year":2013},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.621468Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:54bbcc188ffcec43eb57e7af5061f985189cc7b4546f633bfdb37cf2de7f6b88","observation_id":"3fb3aec8-0d98-4ff2-aa82-f77a7f78152d","resolution":{"observed_at":"2026-08-10T17:03:07.978021Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.955921Z","title":"Fuß and M","venue":null,"work_id":"bf0741e9-3911-4c3d-b33a-58a2b9a7142b","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.626565Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:6411ff3245b91f450cf2b8da93dc05d08582433bbb7387c890fab520da292d9f","observation_id":"05ea606d-50b2-4b16-8ec6-d0a854d7f5f0","resolution":{"observed_at":"2026-08-10T17:03:07.961177Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.939808Z","title":"Wang and A","venue":null,"work_id":"fee437ee-ca7d-466c-b079-4648a65ca849","year":2010},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.631708Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:c3d646d911c5925335a05bec4e71d94ef695916dd59ac0ff1858b2a12d29254c","observation_id":"2afcabc1-84f0-4155-bb8c-6f435c98ba08","resolution":{"observed_at":"2026-08-10T17:03:07.944653Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.923794Z","title":"Wang and A","venue":null,"work_id":"e2ac64c6-75c9-4ae6-8ceb-b225c0cecdde","year":2012},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.637649Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:6fbde414342b87c1176bcf615f238c6b4df79f17470138165ff9d2aa0947767c","observation_id":"1915b3c6-066d-419a-83bc-86d6581a9b18","resolution":{"observed_at":"2026-08-10T17:03:07.928835Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.908473Z","title":null,"venue":null,"work_id":"b2ee6e59-3cf9-41b5-92e0-d344b43c58c4","year":2011},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.643270Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:eb9e0dc2c22dcb0d2ee71908d2e5d4d28d8943c37c3731bd08e747b85b17874b","observation_id":"89c26702-d717-4e8b-a077-31c4d767e2b5","resolution":{"observed_at":"2026-08-10T17:03:07.913345Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.892074Z","title":null,"venue":null,"work_id":"427e056f-b8cd-4edc-9896-e5e4f4ce6b85","year":2010},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.649009Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:996f86a75b4df126cdc6b0892fef0a94bd2f5eb7dbd6734c55af834dc9d91295","observation_id":"82d28492-b87a-47eb-a320-ea6362cdb0b3","resolution":{"observed_at":"2026-08-10T17:03:07.897274Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.875897Z","title":"Mau et al","venue":null,"work_id":"f1cfeb22-eced-4e54-a915-b55bdb9c613e","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.654054Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:cdf98b768aece72a3847e868f1b03f9bcd333dda5c27df0965193f9e723be570","observation_id":"736d26c2-9f63-42f7-923c-a6f76e738db8","resolution":{"observed_at":"2026-08-10T17:03:07.880884Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.769012Z","title":"Drlica-Wagner et al","venue":null,"work_id":"5d6936ca-41a1-4c8a-9559-9b848700ee2c","year":2020},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.659652Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:abdabb61026b1697112386477f5e3b9ad91e88f2294b15161aa2ad0902630448","observation_id":"cb5b3d92-154a-458e-9b16-2d359f854da7","resolution":{"observed_at":"2026-08-10T17:03:07.819867Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.716298Z","title":"Bechtol et al., in Snowmass 2021 (2022)","venue":null,"work_id":"17155226-766b-4603-a1c0-fd21fe484e83","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.665372Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:037df371d9e46543a4876815eb12e8f73ad9fc98f74e7e5b0bebb6577bef17ed","observation_id":"b694a342-027b-42ca-aa69-f160fe50bb64","resolution":{"observed_at":"2026-08-10T17:03:07.729477Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.700366Z","title":null,"venue":null,"work_id":"6eb5477f-0988-41b5-8b05-cef4ef31e0c3","year":2012},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.670428Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:39f7925dafcaa908986116b343a6d20693359bc41b8bfb222036e6b80dcca8d7","observation_id":"3ee14d38-5bcb-4a5d-8944-98adb4b3122b","resolution":{"observed_at":"2026-08-10T17:03:07.705292Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.683680Z","title":null,"venue":null,"work_id":"f1156413-9acd-488c-a9d3-71e432e4a8c3","year":2014},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.675240Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:fc2eb59d272157584363db310e4f6965b7c57f6e56b8cf453da9bc6c07896a50","observation_id":"e327dd92-2b1b-4e2a-9a42-fb4c25faaafa","resolution":{"observed_at":"2026-08-10T17:03:07.689957Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.666484Z","title":null,"venue":null,"work_id":"6419043b-9ba4-40ea-b4fc-5e3d5b60e911","year":2020},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.679645Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:04db0928e9ce84f699e2d47fd41cae2f21da026a24a8eb48238bfb6c79d5f542","observation_id":"f32866be-40ae-4435-929a-d07413997830","resolution":{"observed_at":"2026-08-10T17:03:07.671139Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.650904Z","title":null,"venue":null,"work_id":"382c8e45-b393-4fe7-a45e-caf472362f8b","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.683925Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:aeb758f58468a36093765f7fa9fe6af57ae64964d53afe5709bf1394349c8213","observation_id":"c58efb58-b21f-4dbc-8070-a2f718dd243a","resolution":{"observed_at":"2026-08-10T17:03:07.656025Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.632484Z","title":"Du et al., Phys","venue":null,"work_id":"a1173f67-c142-45a7-a3da-6d336a16c4bc","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.688646Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:c0c11187da1d3a9624a86094f8b13e179c7db75abad3842c011b550c537697c6","observation_id":"37137620-0c39-4339-8cd5-07477a0d192c","resolution":{"observed_at":"2026-08-10T17:03:07.638087Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.613340Z","title":"Errani and J","venue":null,"work_id":"fdd2c646-fc13-4f5e-8911-aa660641899c","year":2020},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.693084Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:9175258838026ad645214d51cc50daa9b79911fb8bb38ee317c881f48ded8f2e","observation_id":"e39c06e8-082c-4e7d-a5bf-19633dd8d101","resolution":{"observed_at":"2026-08-10T17:03:07.620044Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.597233Z","title":"Errani, J","venue":null,"work_id":"a5f640b6-aa94-425e-bb1f-57e2445bfb47","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.697585Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:b3d6ecfe5904b644e452d9746ba7f0b657e54f5cec4501c7c86c8dddd4e65112","observation_id":"f0643e3b-156a-4261-9884-55412f54fd11","resolution":{"observed_at":"2026-08-10T17:03:07.602241Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.580935Z","title":null,"venue":null,"work_id":"8ef5926c-2ee5-475f-8069-e7a551157d5c","year":2018},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.702844Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:9347a773fa0755c5532e933f7cf0f88dd60aa13032f4bd9c6df8ccc3dfb594a6","observation_id":"1446fc49-0327-47a2-a74d-d82b77110d13","resolution":{"observed_at":"2026-08-10T17:03:07.586150Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.564176Z","title":null,"venue":null,"work_id":"a002319f-fa19-4c2c-94bc-122dd5ade10e","year":2018},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.707307Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:b0137ed6b537a1e1f272407dc210bb1d1cb62d0096cd734a6bd0a63f8d60fcda","observation_id":"baac7223-d5d5-46fa-98e5-89d573f3bc79","resolution":{"observed_at":"2026-08-10T17:03:07.569715Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.547939Z","title":null,"venue":null,"work_id":"123721a1-482a-4802-9ffe-fa4e9bab1c63","year":2018},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.711699Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2b45455808081ad082074e6e67160ed43158fd66fbbda3b6de8d72447201c351","observation_id":"809a54bc-38a1-47ba-93aa-fa99bb77de77","resolution":{"observed_at":"2026-08-10T17:03:07.553147Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.532022Z","title":null,"venue":null,"work_id":"b642fb7e-3c0d-4ac4-97e2-78f14390d4cf","year":2021},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.717153Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:3f2befba6def7fcbc3f3f8bf097db116e7739d350b40f104c300dece11877b67","observation_id":"8a2f5d81-afd6-4720-99ea-de75bee6d2b7","resolution":{"observed_at":"2026-08-10T17:03:07.536766Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.514827Z","title":"Mansfield, E","venue":null,"work_id":"93d15eb1-8e31-4bdc-8cbd-91bd311adb43","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.722659Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:0e1e62c25155389b07488228949480232d4ab28d739a78fab547406e7727e3f2","observation_id":"a4db548e-bb41-44b7-ad5d-064b4505d9b4","resolution":{"observed_at":"2026-08-10T17:03:07.520279Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.496129Z","title":null,"venue":null,"work_id":"b981d932-37c7-474d-9a19-4fae8b18c6bc","year":2025},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.727630Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:3dd786ac9576db1c46c60a13ee3e7659b27fdfbfffff2710d3d7c5f034b4f0dd","observation_id":"f84e60e9-7bbe-4433-8350-a064784bfb63","resolution":{"observed_at":"2026-08-10T17:03:07.501273Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.477974Z","title":null,"venue":null,"work_id":"838db298-713b-450a-b05b-23d544cb170c","year":1998},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.732190Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:64adc17cbcb73cdd068e883e5c2f6b6f88cf58510a7bd8da0876453073001173","observation_id":"9f50c78c-bee0-453e-b6ea-79f27e73408b","resolution":{"observed_at":"2026-08-10T17:03:07.485040Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.462016Z","title":null,"venue":null,"work_id":"a5ac29da-c430-429f-8f38-f871b893dcd5","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.737029Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:9b5633170f34aa0369526e118dd16d69316652fba9762514a07a926c33c6a79b","observation_id":"54b4d704-3f47-46d0-8a57-bb70e0b6aca0","resolution":{"observed_at":"2026-08-10T17:03:07.466596Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.445710Z","title":null,"venue":null,"work_id":"701c59ab-79ed-44d7-8243-b4d3c35b6c00","year":2017},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.742175Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:8f6a297b1ec8a0f46cba24c5f8e6a3544e691abc864efb7a2bbf636ef0d100d6","observation_id":"3e281d2a-9d5d-436c-a8e0-138391cf36e4","resolution":{"observed_at":"2026-08-10T17:03:07.450494Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.428713Z","title":null,"venue":null,"work_id":"6c74f75e-5603-44b4-8896-4c0d4056338c","year":2020},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.752645Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:caa55b35e2567e9a3a6169f824c22c7337b95f51399bfc0695711d16e3aaf8db","observation_id":"98d8b1f2-a7e1-4904-8c2e-73f1c22c1f04","resolution":{"observed_at":"2026-08-10T17:03:07.434006Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.407584Z","title":"Parkinson, S","venue":null,"work_id":"9104040c-7b37-4357-b3b9-0ff0ad732092","year":2008},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.757414Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:6f72f695a7e88bc2aa98102a4a174aa851f5f8161a99c903e7ff033cb15f34d7","observation_id":"49dd176f-32a0-4185-b0bc-a3601013072e","resolution":{"observed_at":"2026-08-10T17:03:07.413930Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.384958Z","title":null,"venue":null,"work_id":"17cfa624-a796-4836-a49b-e789543f15c6","year":2013},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.762044Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:49cc89c98e285e38af7be2bff3144640f010878233131649423c982dcfdf9e9d","observation_id":"c518ae5d-6f70-4dd5-aca9-162bec957981","resolution":{"observed_at":"2026-08-10T17:03:07.390186Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.369334Z","title":null,"venue":null,"work_id":"038e6c65-6bc4-4908-91bb-8eb495e0129d","year":2016},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.767241Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:c33d7d8c4517b1c336ee6eb55d80173fb72586c64206652932581be2bff3e937","observation_id":"e9b9a208-785a-406d-9522-bf04b3b3711a","resolution":{"observed_at":"2026-08-10T17:03:07.374357Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.353196Z","title":null,"venue":null,"work_id":"b87d4202-8c9b-4324-964f-6b3e8f842280","year":2019},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.772062Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2e2e885caaa3d37f1631fa4d5163a5ad0a25637340da5c967681be198a3f8ad8","observation_id":"3c9a149f-83ac-45c9-b4c3-5c6ff07f5438","resolution":{"observed_at":"2026-08-10T17:03:07.358080Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.332807Z","title":"Diemer and M","venue":null,"work_id":"b9cb5970-c212-4b2f-8c45-03e8a823b109","year":2019},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.776980Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:19be1a12968c96f558bd10bd876d174dc29f462d4b46b030b3b50922e03b3d54","observation_id":"df0d059c-4f6b-4972-ae7a-1fd12553a41c","resolution":{"observed_at":"2026-08-10T17:03:07.339074Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.312836Z","title":"Diemer, S","venue":null,"work_id":"41be9042-bce7-4edc-9d6f-a870ebe796f2","year":2013},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.782193Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:aecbf97d27b879c1436577403f1b09fe36b4c5993e0fd877c06ec756d533a9ae","observation_id":"3c16ee7f-0573-4189-aff9-f2383a17b065","resolution":{"observed_at":"2026-08-10T17:03:07.319718Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.167446Z","title":null,"venue":null,"work_id":"7c815a15-63f0-44ab-abed-1b28cc8c710f","year":1997},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.788095Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:33c2993fde8471194ce316f7df4c3978b66f10f728b479faa821c50c6fe214b2","observation_id":"47160a98-b9d4-4c61-b184-0cdca7c2df49","resolution":{"observed_at":"2026-08-10T17:03:07.172318Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.150148Z","title":null,"venue":null,"work_id":"ad6554aa-5fcc-41c7-8412-69983618cfd9","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.793583Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:f24e9960aa6d4792ceb03e9d448c009798445f79c481a8d526319a49ea67bb8e","observation_id":"6078f578-b80d-4395-9541-7e088598e219","resolution":{"observed_at":"2026-08-10T17:03:07.156417Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.129312Z","title":null,"venue":null,"work_id":"fbc7210f-4885-40bd-a35e-97b4e03d2637","year":2025},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.798887Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:abdc3f2088957bc163c9f1cda4b0932b115449ab5e5daee9169429aaaf4f71db","observation_id":"8b569aac-f4f4-40bb-8e5e-e2d5f88a2a63","resolution":{"observed_at":"2026-08-10T17:03:07.135038Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.105597Z","title":null,"venue":null,"work_id":"c8a9ca6b-bcd5-4b3b-8e9d-6fc6cfd97a45","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.804571Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2dbf868eb86bc2857a88101c3a307c584d40f576225b95a78d6713c1ec2212c7","observation_id":"7b055b1b-4afe-4a30-a974-f40bddaeba67","resolution":{"observed_at":"2026-08-10T17:03:07.113489Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.088780Z","title":null,"venue":null,"work_id":"9c9d7cd5-4051-4dc5-a1fe-594beb9de4ff","year":2006},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.809404Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:2f7e9a8f880ab2974a0871a31ff30a58913c0e08731410ab0c17449504c6d345","observation_id":"c834abb5-58c7-444d-ae2a-b9a481f04edf","resolution":{"observed_at":"2026-08-10T17:03:07.093407Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.068700Z","title":"Banik and F","venue":null,"work_id":"9f1dac7c-5cf6-4564-a176-59875daba492","year":2022},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.814756Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:90e070636a3f16ced2d4377e162f1147a787cbb65939f3c1ae3cd6e3922547be","observation_id":"245a1511-97d4-4d93-9281-21cf99946469","resolution":{"observed_at":"2026-08-10T17:03:07.074901Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.051333Z","title":"Chandrasekhar, ApJ 97, 255 (1943)","venue":null,"work_id":"df3d53e7-cdde-4779-9ac2-b3d8187c24fc","year":1943},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.820072Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:395b65ed4254d1f66a9288cd52a70d66d0d0730f55ce6cadecf8e35bd92eb226","observation_id":"041578ec-c587-495f-a433-e6e2c34e5ef9","resolution":{"observed_at":"2026-08-10T17:03:07.056611Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.033235Z","title":null,"venue":null,"work_id":"6441b86b-2649-4160-9acc-e44144425b40","year":2023},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.825294Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:6fe51da5f06a959b997cff1111766a3a5d3d9f029ce22aa58d32f7b5291a4ee1","observation_id":"f4de7865-d9b6-4b9c-91ee-a0bc17d7e861","resolution":{"observed_at":"2026-08-10T17:03:07.039641Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.11680","last_updated":"2024-10-15T15:18:46Z","snapshot_observed_at":"2026-08-16T13:09:08.857834Z","submitted_at":"2024-10-15T15:18:46Z","title":"Population synthesis and astrophysical inference for high-$z$ JWST galaxies","version":1},"cited_work":{"arxiv_id":"2410.11680","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.11680","snapshot_observed_at":"2026-08-10T17:03:06.915734Z","title":"Population synthesis and astrophysical inference for high-$z$ JWST galaxies","venue":"astro-ph.GA","work_id":"8f40d940-c153-4fbf-869a-ca95be4dbb36","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.830585Z"},"links":{"cited_paper":"/paper/2410.11680","citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:ba8848473eeb38fc3fe238ba649550714d794fa751bb2b4ba702713c88ca3114","observation_id":"6971105e-a661-4f7b-90ef-e38bf9387a1f","resolution":{"observed_at":"2026-08-10T17:03:06.924085Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:07.012085Z","title":"Weerasooriya, M","venue":null,"work_id":"5d319289-f869-4e0d-b268-4f20dbee96e7","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.835709Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:a783ef6df0e6dd70e6ecf6502d87d5cbc8e2edd709c2512899ef4f23dd2861ec","observation_id":"b30e7ec6-fef2-460c-9b4f-142aca3c2e5d","resolution":{"observed_at":"2026-08-10T17:03:07.019226Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:06.994349Z","title":"Ahvazi, A","venue":null,"work_id":"a1ac92a3-984d-4bae-9ff0-99963725c96f","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.841942Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:5c828dac43a64783aef185fd62d50ea1f6b6eb7f3abb0b34782f2c60d94bc9bb","observation_id":"7aea55cd-7878-4b6d-95b5-e3b3fdfd6ae5","resolution":{"observed_at":"2026-08-10T17:03:07.000168Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:06.976569Z","title":"Menker and A","venue":null,"work_id":"fa20daf9-8eb0-435c-b729-7ee9afe01d45","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.846594Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:6cff8cb00393f67467df510cba7d6f39e60e2eb7f4ee25a605972dd6835581ea","observation_id":"3645d107-5433-43d3-b7ad-2e2a599a1dae","resolution":{"observed_at":"2026-08-10T17:03:06.982324Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:06.957181Z","title":null,"venue":null,"work_id":"8f36dd48-49f5-41d4-82ef-d3ba6d9c01c8","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.851879Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:b1223b7f3b832e14108ea3d11625662498731607e9578fb60d8d1f2c5070b7e6","observation_id":"b1f76ef4-299f-4e71-a9d3-928a884a7ae1","resolution":{"observed_at":"2026-08-10T17:03:06.962842Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-10T17:03:06.937812Z","title":"galacticus,","venue":null,"work_id":"d135fc4a-27c1-433d-b643-5d1bcc2132f5","year":2024},"citing_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-10T17:03:06.856926Z"},"links":{"citing_paper":"/paper/2501.12636"},"observation_digest":"sha256:c951f28a61538564823b068d1f7210b6e229c1333a74d7475df95d64af580af0","observation_id":"65abcfe9-4f1b-477f-8f18-c73e64259d82","resolution":{"observed_at":"2026-08-10T17:03:06.944739Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T00:49:38.238557Z","submitted_at":"2025-01-22T04:52:49Z","title":"Semianalytic model for decaying dark matter halos"},"reference_resolution":{"displayed":81,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":40,"verified_exact":1,"verified_fuzzy":39},"total_outbound_references":81},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 81 of 81 outbound references and 1 inbound Pith citation observation for arXiv:2501.12636."}