{"as_of":"2026-08-16T23:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:43d234c2f3940f680ec4efdd168eb621ac2b876c666a21796e9e285eabeb39e4","coverage":[{"denominator":100,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T13:07:59.040501Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.19244/citation-record","integrity":"/paper/2607.19244/integrity","json":"/paper/2607.19244/citation-record.json","paper":"/paper/2607.19244"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-01T13:07:44.975474Z","title":"and others","venue":null,"work_id":null,"year":2018},"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":1,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:44.975474Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:aab5ea0ed8ad1a512f263169fb34c3049dec308e4ae97b09e98fe45782d3341d","observation_id":"49eedf55-ec73-41ba-b8db-79a911573fe8","resolution":{"observed_at":"2026-08-01T13:07:44.975474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.11265","last_updated":"2019-03-27T21:18:27Z","snapshot_observed_at":"2026-08-14T17:09:26.210181Z","submitted_at":"2019-02-28T18:11:04Z","title":"The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.11265","snapshot_observed_at":"2026-08-01T13:07:45.068639Z","title":"and others","venue":null,"work_id":null,"year":2019},"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":2,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.068639Z"},"links":{"cited_paper":"/paper/1902.11265","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:e0a5023f75781372405c2dfb689e3d4a024446ed3918a35e7ddef07647aef4ac","observation_id":"0c14d41d-e905-43ce-bb0c-67609ea63226","resolution":{"observed_at":"2026-08-01T13:07:45.068639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.01845","last_updated":"2020-12-08T17:49:59Z","snapshot_observed_at":"2026-08-13T22:13:57.143272Z","submitted_at":"2020-07-03T17:54:18Z","title":"KiDS-1000 catalogue: Weak gravitational lensing shear measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.01845","snapshot_observed_at":"2026-08-01T13:07:45.212475Z","title":"KiDS-1000 catalogue: Weak gravitational lensing shear measurements","venue":null,"work_id":null,"year":2021},"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":3,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.212475Z"},"links":{"cited_paper":"/paper/2007.01845","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:176661d19a95e6da8b37948813b69e366a1dc6f6058451a3878de466804329a7","observation_id":"8d9d23c7-fc8c-44d8-a4e3-cd4f7b11cd7c","resolution":{"observed_at":"2026-08-01T13:07:45.212475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02396","last_updated":"2022-04-05T17:59:45Z","snapshot_observed_at":"2026-08-16T17:09:05.196858Z","submitted_at":"2022-04-05T17:59:45Z","title":"KiDS-1000: cosmic shear with enhanced redshift calibration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02396","snapshot_observed_at":"2026-08-01T13:07:45.326431Z","title":null,"venue":null,"work_id":null,"year":2022},"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":4,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.326431Z"},"links":{"cited_paper":"/paper/2204.02396","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:aca8934575241030b8bdb6bc8927fa6426094c300a6dbc6705b15714e6942ab7","observation_id":"3e6a4fc0-c408-4ae6-bca0-3ea57d41af83","resolution":{"observed_at":"2026-08-01T13:07:45.326431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:45.497241Z","title":"and others","venue":null,"work_id":null,"year":2022},"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":5,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.497241Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:0f5b9872b8cf787173a2b19a952ecd1a2c507acff25209d13d4617dc3b922820","observation_id":"7df48a9d-ee60-4f37-a286-fb700d2f8a46","resolution":{"observed_at":"2026-08-01T13:07:45.497241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.06041","last_updated":"2022-01-10T05:23:03Z","snapshot_observed_at":"2026-08-14T16:15:45.300920Z","submitted_at":"2019-06-14T06:12:37Z","title":"Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.06041","snapshot_observed_at":"2026-08-01T13:07:45.622263Z","title":"and others","venue":null,"work_id":null,"year":2020},"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":6,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.622263Z"},"links":{"cited_paper":"/paper/1906.06041","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:ebc8a706fea87a10d5724072cf1a663cd3451d791fd07100f790ce5875686da1","observation_id":"4d73a322-9be4-4b85-8d96-4481b21d5082","resolution":{"observed_at":"2026-08-01T13:07:45.622263Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-08-14T23:39:27.638377Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13549","snapshot_observed_at":"2026-08-01T13:07:45.695291Z","title":null,"venue":null,"work_id":null,"year":2022},"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":7,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.695291Z"},"links":{"cited_paper":"/paper/2105.13549","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:13eb22809cad32a74408f2bb84670b4da3da824ea7389e45b0ca6fe225e30a16","observation_id":"75d72e17-8002-4bc1-a3eb-208b8957effe","resolution":{"observed_at":"2026-08-01T13:07:45.695291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:45.747400Z","title":"KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes","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":8,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.747400Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:5b0aa1abf1739aed27ed68bc4b49baedb42b41c37953c2d26f93b84ff5f816ca","observation_id":"51dcb6d5-873f-4a4e-84aa-478518ed3b31","resolution":{"observed_at":"2026-08-01T13:07:45.747400Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:45.819438Z","title":null,"venue":null,"work_id":null,"year":2026},"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":9,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.819438Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:09c104995a0b561c61114fdf6e63cc447c1b3467b5b86a056d5e108c9a7fbaa4","observation_id":"e0a86533-2f61-4979-83ff-b360aff9027b","resolution":{"observed_at":"2026-08-01T13:07:45.819438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2366","last_updated":"2018-05-23T19:18:23Z","snapshot_observed_at":"2026-08-12T13:36:12.529300Z","submitted_at":"2008-05-15T18:10:13Z","title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.2366","snapshot_observed_at":"2026-08-01T13:07:45.871171Z","title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","venue":null,"work_id":null,"year":2019},"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":10,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.871171Z"},"links":{"cited_paper":"/paper/0805.2366","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:f90a9d7e2b89d0fd9c78c0c7b982206b2a455049215af53999be0defdd41c5d9","observation_id":"7f535378-2e01-453c-bfcc-a1d5427ff854","resolution":{"observed_at":"2026-08-01T13:07:45.871171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:45.988806Z","title":"and others","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":11,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:45.988806Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:9b9f0c775c35d4340ed36052b698862392c72d499fd919ab83552586b008c5f7","observation_id":"547d1394-dd6d-435c-a749-f4b19bb58493","resolution":{"observed_at":"2026-08-01T13:07:45.988806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.03757","last_updated":"2015-03-13T20:16:08Z","snapshot_observed_at":"2026-08-14T22:56:35.748290Z","submitted_at":"2015-03-12T14:57:27Z","title":"Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.03757","snapshot_observed_at":"2026-08-01T13:07:46.116867Z","title":"and others","venue":null,"work_id":null,"year":2015},"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":12,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.116867Z"},"links":{"cited_paper":"/paper/1503.03757","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:718da731e9682403fdc2938ee45b5e51c316404a68403f37df7a1c6fb8fb3579","observation_id":"a1f14a60-b034-41d9-91d6-32978d051470","resolution":{"observed_at":"2026-08-01T13:07:46.116867Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.04634","last_updated":"2019-08-07T15:33:57Z","snapshot_observed_at":"2026-08-14T17:30:58.844503Z","submitted_at":"2019-01-15T01:54:59Z","title":"Cosmology from the Chinese Space Station Optical Survey (CSS-OS)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.04634","snapshot_observed_at":"2026-08-01T13:07:46.252101Z","title":"Cosmology from the Chinese Space Station Optical Survey (CSS-OS)","venue":null,"work_id":null,"year":2019},"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":13,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.252101Z"},"links":{"cited_paper":"/paper/1901.04634","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:62aa7d54e10ce03cbaa63e11bce9cb9047bd27df00068b394d05c1b6a9161564","observation_id":"771246ab-0906-4461-92c7-1226e41b2d6d","resolution":{"observed_at":"2026-08-01T13:07:46.252101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03598","last_updated":"2022-07-07T21:57:57Z","snapshot_observed_at":"2026-08-16T16:47:31.840244Z","submitted_at":"2022-07-07T21:57:57Z","title":"Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03598","snapshot_observed_at":"2026-08-01T13:07:46.366315Z","title":"Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys","venue":null,"work_id":null,"year":2023},"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":14,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.366315Z"},"links":{"cited_paper":"/paper/2207.03598","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:6039c8f90d824db1d6508883a94f6748767a9c392c573f70511c0c2004244988","observation_id":"45618540-ea65-4d71-83c9-042b3db640c9","resolution":{"observed_at":"2026-08-01T13:07:46.366315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11794","last_updated":"2022-06-23T15:59:13Z","snapshot_observed_at":"2026-08-16T16:50:50.015577Z","submitted_at":"2022-06-23T15:59:13Z","title":"A non-linear solution to the $S_8$ tension?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11794","snapshot_observed_at":"2026-08-01T13:07:46.469334Z","title":"A non-linear solution to the S_8 tension?","venue":null,"work_id":null,"year":2022},"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":15,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.469334Z"},"links":{"cited_paper":"/paper/2206.11794","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:f46f5e23d8a6d3e8e7f77c217bfadd86b3a4a065a387c9e0c958a759981dfb26","observation_id":"6aba75cf-95b3-4606-a8e7-cb1a3b109900","resolution":{"observed_at":"2026-08-01T13:07:46.469334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.05537","last_updated":"2023-08-07T09:26:56Z","snapshot_observed_at":"2026-08-16T15:49:24.561709Z","submitted_at":"2023-03-09T19:01:02Z","title":"DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.05537","snapshot_observed_at":"2026-08-01T13:07:46.581636Z","title":"and Zennaro, Matteo and Contreras, Sergio and Chen, Angela and Hern \\'a ndez-Monteagudo, Carlos","venue":null,"work_id":null,"year":2023},"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":16,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.581636Z"},"links":{"cited_paper":"/paper/2303.05537","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:12055d8ed5d80b3f11caf8611095e2b5d8fd29938f10d3d48b8cf6dec315dd2b","observation_id":"a0b6a224-f512-47cc-b0ff-94b85dc60e24","resolution":{"observed_at":"2026-08-01T13:07:46.581636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.08494","last_updated":"2020-03-30T10:37:19Z","snapshot_observed_at":"2026-08-09T09:37:50.849641Z","submitted_at":"2019-11-19T19:00:02Z","title":"Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.08494","snapshot_observed_at":"2026-08-01T13:07:46.692749Z","title":"Baryonic effects for weak lensing","venue":null,"work_id":null,"year":2020},"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":17,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.692749Z"},"links":{"cited_paper":"/paper/1911.08494","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:28aefd8d99b938ad8c5f7d52c28ec75b7830490a36345ffe5e0fb6a6fc202efd","observation_id":"e6d8d144-ca33-42e5-bede-5ae9f7a97a50","resolution":{"observed_at":"2026-08-01T13:07:46.692749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.08486","last_updated":"2020-09-07T11:44:41Z","snapshot_observed_at":"2026-08-14T23:14:26.008744Z","submitted_at":"2020-08-19T14:55:06Z","title":"Cannibalism hinders growth: Cannibal Dark Matter and the $S_8$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.08486","snapshot_observed_at":"2026-08-01T13:07:46.805485Z","title":"Cannibalism hinders growth: Cannibal Dark Matter and the S_8 tension","venue":null,"work_id":null,"year":2020},"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":18,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.805485Z"},"links":{"cited_paper":"/paper/2008.08486","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:b1bea044daf3f39d9f555dd715b1cd37630f9ce06ee92602776fee3ae51532ee","observation_id":"97147378-cc31-47ad-ba66-f40722ff5a01","resolution":{"observed_at":"2026-08-01T13:07:46.805485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03500","last_updated":"2023-07-24T17:08:22Z","snapshot_observed_at":"2026-08-16T16:47:34.387924Z","submitted_at":"2022-07-07T18:00:03Z","title":"A Step in Understanding the $S_8$ Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03500","snapshot_observed_at":"2026-08-01T13:07:46.983465Z","title":"and Weiner, Neal","venue":null,"work_id":null,"year":2023},"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":19,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:46.983465Z"},"links":{"cited_paper":"/paper/2207.03500","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:355ac46d37d7b2875ba4ffc188446a412b47ad86bc6106630cc1dd3168a0c1ca","observation_id":"2076388d-1cbf-477c-ae30-39fbfff4f4fe","resolution":{"observed_at":"2026-08-01T13:07:46.983465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.06217","last_updated":"2023-10-11T16:36:50Z","snapshot_observed_at":"2026-08-16T16:32:46.880565Z","submitted_at":"2022-09-13T18:00:00Z","title":"The Sigma-8 Tension is a Drag","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.06217","snapshot_observed_at":"2026-08-01T13:07:47.126963Z","title":"and Kamionkowski, Marc","venue":null,"work_id":null,"year":2023},"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":20,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.126963Z"},"links":{"cited_paper":"/paper/2209.06217","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:42e01452d8f25c6cc07046ed8a8ab5f3a130fcf4770a8de09f0b72ad3e10ed2d","observation_id":"cefc76b5-3cfe-4ca7-8b70-64d5dba2b44c","resolution":{"observed_at":"2026-08-01T13:07:47.126963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.04528","last_updated":"2022-03-08T09:19:34Z","snapshot_observed_at":"2026-08-16T17:28:46.831294Z","submitted_at":"2022-01-12T15:56:47Z","title":"Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.04528","snapshot_observed_at":"2026-08-01T13:07:47.298974Z","title":"and Baldi, Marco","venue":null,"work_id":null,"year":2022},"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":21,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.298974Z"},"links":{"cited_paper":"/paper/2201.04528","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:f96a6050c5e591fcb6f3b7ff7c3e783fea066269d14dcec8f08fec3c5df11545","observation_id":"0037c103-44a2-40a5-a351-ce8f3c16df02","resolution":{"observed_at":"2026-08-01T13:07:47.298974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03244","last_updated":"2024-08-07T21:26:25Z","snapshot_observed_at":"2026-08-16T14:03:43.829814Z","submitted_at":"2024-04-04T07:01:14Z","title":"Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03244","snapshot_observed_at":"2026-08-01T13:07:47.439644Z","title":"Scale-dependent local primordial non-Gaussianity as a solution to the S8 tension","venue":null,"work_id":null,"year":2024},"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":22,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.439644Z"},"links":{"cited_paper":"/paper/2404.03244","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:21624b9a639a25072897826d85d08e22cfbe39f850e23ee4f08feeedd3cd28d3","observation_id":"cff78e97-acc8-4c04-aa9e-db6291216555","resolution":{"observed_at":"2026-08-01T13:07:47.439644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05511","last_updated":"2015-10-02T05:40:28Z","snapshot_observed_at":"2026-08-14T23:14:58.866225Z","submitted_at":"2015-05-20T20:00:36Z","title":"Decaying dark matter and the tension in $\\sigma_8$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.05511","snapshot_observed_at":"2026-08-01T13:07:47.523019Z","title":"Decaying dark matter and the tension in _8","venue":null,"work_id":null,"year":2015},"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":23,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.523019Z"},"links":{"cited_paper":"/paper/1505.05511","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:89427c8a4f683f6c47341b98ea0dd1637e5de68a1fbc1805fce244df74da16ad","observation_id":"a1eb20f9-5860-4911-8b43-143c96000cac","resolution":{"observed_at":"2026-08-01T13:07:47.523019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.09112","last_updated":"2019-06-21T13:04:57Z","snapshot_observed_at":"2026-08-14T23:14:26.399209Z","submitted_at":"2019-06-21T13:04:57Z","title":"Constraints on decaying dark matter from weak lensing and cluster counts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.09112","snapshot_observed_at":"2026-08-01T13:07:47.603496Z","title":"Constraints on decaying dark matter from weak lensing and cluster counts","venue":null,"work_id":null,"year":2020},"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":24,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.603496Z"},"links":{"cited_paper":"/paper/1906.09112","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:002e977497d3877beac4b9432fee407060cfefd20f2319a15a17b3ffc5b12360","observation_id":"a98dbdc0-d920-4364-bb09-763e8cfdaf6a","resolution":{"observed_at":"2026-08-01T13:07:47.603496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.07838","last_updated":"2017-11-24T17:09:58Z","snapshot_observed_at":"2026-08-14T21:04:46.982798Z","submitted_at":"2017-04-25T18:00:35Z","title":"\"Non-cold\" dark matter at small scales: a general approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.07838","snapshot_observed_at":"2026-08-01T13:07:47.665772Z","title":"''Non-cold'' dark matter at small scales: a general approach","venue":null,"work_id":null,"year":2017},"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":25,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.665772Z"},"links":{"cited_paper":"/paper/1704.07838","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:5abdf25027d5da3f647f31e8e19ba3fd4fc8ab7fa86c8ab8f6e0bf720bc9f038","observation_id":"f028f7d2-5ffa-425d-a23e-712e18c20b14","resolution":{"observed_at":"2026-08-01T13:07:47.665772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.12498","last_updated":"2022-01-03T13:27:29Z","snapshot_observed_at":"2026-08-16T18:43:13.581087Z","submitted_at":"2021-02-24T19:00:06Z","title":"Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.12498","snapshot_observed_at":"2026-08-01T13:07:47.749278Z","title":"Linear cosmological constraints on two-body decaying dark matter scenarios and the S8 tension","venue":null,"work_id":null,"year":2021},"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":26,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.749278Z"},"links":{"cited_paper":"/paper/2102.12498","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:33a906119aa4fa1b01c3de00c1c1a3eb145113841e136e61abe445028a0bb694","observation_id":"da77756d-cd14-4724-a2ce-7a8d6f35f8af","resolution":{"observed_at":"2026-08-01T13:07:47.749278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.04606","last_updated":"2022-09-27T04:28:00Z","snapshot_observed_at":"2026-08-16T19:07:06.483669Z","submitted_at":"2020-11-09T18:00:54Z","title":"Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.04606","snapshot_observed_at":"2026-08-01T13:07:47.835251Z","title":"and others","venue":null,"work_id":null,"year":2021},"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":27,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.835251Z"},"links":{"cited_paper":"/paper/2011.04606","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:305be305f76cfa94c8c9012616f4d9f2c246e942cb61e877c94ac4440cf15510","observation_id":"1d75c607-b4f0-4aab-87f1-145f8fedc07b","resolution":{"observed_at":"2026-08-01T13:07:47.835251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:47.946674Z","title":"Gravitino cosmology helped by a right handed (s)neutrino","venue":null,"work_id":null,"year":2022},"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":28,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:47.946674Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:998897457135e0c02d6add85b611778458f7e78290dc9006a22e13fd86483dac","observation_id":"4cfb60f6-f029-48f3-b90e-a6180001411b","resolution":{"observed_at":"2026-08-01T13:07:47.946674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03939","last_updated":"2023-06-15T00:27:08Z","snapshot_observed_at":"2026-08-16T16:03:21.957021Z","submitted_at":"2023-01-10T12:46:24Z","title":"Testing decaying dark matter models as a solution to the $S_8$ tension with the thermal Sunyaev-Zel'dovich effect","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03939","snapshot_observed_at":"2026-08-01T13:07:48.000180Z","title":"Testing decaying dark matter models as a solution to the S8 tension with the thermal Sunyaev-Zel dovich effect","venue":null,"work_id":null,"year":2023},"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":29,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.000180Z"},"links":{"cited_paper":"/paper/2301.03939","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:365d9ff5a9e1d9cf8f1f8123d159b799d4930c01641f1dfef501e1946bc6f812","observation_id":"cee37be6-c50c-43a3-a6df-83644b9b6928","resolution":{"observed_at":"2026-08-01T13:07:48.000180Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.14334","last_updated":"2023-03-01T13:44:31Z","snapshot_observed_at":"2026-08-16T16:13:15.453689Z","submitted_at":"2022-11-25T19:00:04Z","title":"Constraining dark matter decays with cosmic microwave background and weak lensing shear observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.14334","snapshot_observed_at":"2026-08-01T13:07:48.076074Z","title":"and Schneider, Aurel","venue":null,"work_id":null,"year":2023},"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":30,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.076074Z"},"links":{"cited_paper":"/paper/2211.14334","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:6206865fb99c65193866df940d90805b80523e12007f2d161028ee0823172e4c","observation_id":"439a0cd4-0b27-4784-a4f5-086f73ce324f","resolution":{"observed_at":"2026-08-01T13:07:48.076074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.4587","last_updated":"2010-12-21T10:10:12Z","snapshot_observed_at":"2026-08-15T04:59:22.588110Z","submitted_at":"2010-12-21T10:10:12Z","title":"On the stability of particle dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.4587","snapshot_observed_at":"2026-08-01T13:07:48.155873Z","title":"On the stability of particle dark matter","venue":null,"work_id":null,"year":2011},"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":31,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.155873Z"},"links":{"cited_paper":"/paper/1012.4587","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:60e45fe9cb2e031cd5752fab3b7ae5fe65e1e3ed0d367107fb9190aad7e57640","observation_id":"603d8645-4e78-4e66-9991-4b6d163136e2","resolution":{"observed_at":"2026-08-01T13:07:48.155873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.5379","last_updated":"2012-04-18T17:10:12Z","snapshot_observed_at":"2026-08-15T12:58:16.604028Z","submitted_at":"2012-04-18T17:10:12Z","title":"Light Sterile Neutrinos: A White Paper","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.5379","snapshot_observed_at":"2026-08-01T13:07:48.230656Z","title":null,"venue":null,"work_id":null,"year":2012},"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":32,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.230656Z"},"links":{"cited_paper":"/paper/1204.5379","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:b2fdc529db0836fea5527370908bd444e99556a7421e8e42b046a39a08add593","observation_id":"dd31f05d-8509-4103-b4b4-9573e1b30d95","resolution":{"observed_at":"2026-08-01T13:07:48.230656Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.04816","last_updated":"2017-02-09T14:07:58Z","snapshot_observed_at":"2026-08-15T02:27:11.531591Z","submitted_at":"2016-02-15T21:00:03Z","title":"A White Paper on keV Sterile Neutrino Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.04816","snapshot_observed_at":"2026-08-01T13:07:48.341713Z","title":"and others","venue":null,"work_id":null,"year":2017},"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":33,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.341713Z"},"links":{"cited_paper":"/paper/1602.04816","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:532ef8cd3ed8bd444a054eb4454792467d4c0f6e38741c01630142dc8814e9a1","observation_id":"c5fa4d12-3e8b-4504-b3b0-29b8761ae59f","resolution":{"observed_at":"2026-08-01T13:07:48.341713Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:48.509116Z","title":null,"venue":null,"work_id":null,"year":1984},"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":34,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.509116Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:d6144c8f25c718e2d212cfa12b443feda422d4cd0a18c14ff0be3eaf884fda34","observation_id":"f7712aa8-b5bd-4938-bcce-a4d20dc2236b","resolution":{"observed_at":"2026-08-01T13:07:48.509116Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:48.680407Z","title":null,"venue":null,"work_id":null,"year":1989},"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":35,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.680407Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:cf48959c89718200f91a74259bc797a71817bbadd046a7abe48e640c654dda69","observation_id":"df8ed05a-5507-4e35-9a7d-02df68f78f15","resolution":{"observed_at":"2026-08-01T13:07:48.680407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:48.798742Z","title":null,"venue":null,"work_id":null,"year":1995},"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":36,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.798742Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:3a4602c3a64255bfb4f127b09f94f0d95181db011de913555cc5d710f44b4239","observation_id":"777521df-6305-4aed-bbfa-899f006b3b3f","resolution":{"observed_at":"2026-08-01T13:07:48.798742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/0370-2693(91)91055-z","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Masiero, A","venue":"Physics Letters B","work_id":"eceb98e4-cccb-45a0-ad81-cf4e0936548b","year":1991},"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":37,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:48.904784Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:5c09bfbb6463188aa4c8defacd207029a80e1c5fd7d309716da6c6d06f18be7d","observation_id":"d7393c07-671d-4a42-bc44-cb043a29b832","resolution":{"observed_at":"2026-08-01T13:08:20.731826Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9905212","last_updated":"1999-05-03T16:52:08Z","snapshot_observed_at":"2026-08-13T09:51:14.311220Z","submitted_at":"1999-05-03T16:52:08Z","title":"Axinos as Cold Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9905212","snapshot_observed_at":"2026-08-01T13:07:49.003796Z","title":"and Roszkowski, Leszek","venue":null,"work_id":null,"year":1999},"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":38,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.003796Z"},"links":{"cited_paper":"/paper/hep-ph/9905212","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:40be2aa05d6e53271402fc9c26db1e24a55edf01101a57a01f7826aeb3ddf6b9","observation_id":"83a043de-b3bd-4467-bad5-2535c9123d78","resolution":{"observed_at":"2026-08-01T13:07:49.003796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0108101","last_updated":"2001-08-12T23:31:22Z","snapshot_observed_at":"2026-08-16T03:19:17.958247Z","submitted_at":"2001-08-10T19:00:55Z","title":"Late decaying axino as CDM and its lifetime bound","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0108101","snapshot_observed_at":"2026-08-01T13:07:49.092201Z","title":"Late decaying axino as CDM and its lifetime bound","venue":null,"work_id":null,"year":2002},"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":39,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.092201Z"},"links":{"cited_paper":"/paper/hep-ph/0108101","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:321fe41366d727e277b0baf45f151c37db60f13d5a10e11e7a8ab7f2367f95f9","observation_id":"dab9fba4-6352-4c81-b2cf-32ff345820e1","resolution":{"observed_at":"2026-08-01T13:07:49.092201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306437","last_updated":"2004-05-03T02:04:09Z","snapshot_observed_at":"2026-07-07T00:34:21.783204Z","submitted_at":"2003-06-22T12:49:19Z","title":"Decaying Superheavy Dark Matter and Subgalactic Structure of the Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0306437","snapshot_observed_at":"2026-08-01T13:07:49.188505Z","title":"Decaying superheavy dark matter and subgalactic structure of the universe","venue":null,"work_id":null,"year":2004},"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":40,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.188505Z"},"links":{"cited_paper":"/paper/astro-ph/0306437","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:0775cd1014fab27624bf3dcc51172ee9c87c564192341a121432d602cadc14bb","observation_id":"041b0441-700b-4c94-a69c-b5b27673b0bf","resolution":{"observed_at":"2026-08-01T13:07:49.188505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0306024","last_updated":"2003-08-11T16:53:28Z","snapshot_observed_at":"2026-08-02T01:00:14.223987Z","submitted_at":"2003-06-02T22:18:51Z","title":"SuperWIMP Dark Matter Signals from the Early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0306024","snapshot_observed_at":"2026-08-01T13:07:49.268035Z","title":"and Rajaraman, Arvind and Takayama, Fumihiro","venue":null,"work_id":null,"year":2003},"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":41,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.268035Z"},"links":{"cited_paper":"/paper/hep-ph/0306024","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:ed6db5e64753d2e6ead7d3a83c99a976d6b956668ed56856157281e978b6b54e","observation_id":"da428a8d-c7bb-4074-96dd-4d24e7e00c47","resolution":{"observed_at":"2026-08-01T13:07:49.268035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.08235","last_updated":"2020-09-04T11:42:13Z","snapshot_observed_at":"2026-08-10T11:48:16.443597Z","submitted_at":"2020-01-22T19:08:51Z","title":"Search for decaying heavy dark matter in an effective interaction framework: a comparison of $\\gamma$-ray and radio observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.08235","snapshot_observed_at":"2026-08-01T13:07:49.397757Z","title":"Search for decaying heavy dark matter in an effective interaction framework: a comparison of -ray and radio observations","venue":null,"work_id":null,"year":2020},"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":42,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.397757Z"},"links":{"cited_paper":"/paper/2001.08235","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:0c8b211eb74117d121f46cdc04bc51d369cd0a055fd3aa342abdab848f25dde2","observation_id":"238354c7-fdb3-4d0d-89ec-adf4e30e4819","resolution":{"observed_at":"2026-08-01T13:07:49.397757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06024","last_updated":"2022-09-01T18:04:52Z","snapshot_observed_at":"2026-08-16T17:07:22.215730Z","submitted_at":"2022-04-12T18:07:23Z","title":"A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.06024","snapshot_observed_at":"2026-08-01T13:07:49.422354Z","title":"A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA","venue":null,"work_id":null,"year":2022},"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":43,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.422354Z"},"links":{"cited_paper":"/paper/2204.06024","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:27dd1b48452ab0b8fe494f121463a91fc078606607adc2df6308fc364d461be6","observation_id":"60697a7f-cb51-4ea2-aefe-5046ec47f3cb","resolution":{"observed_at":"2026-08-01T13:07:49.422354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.15543","last_updated":"2024-03-22T18:00:09Z","snapshot_observed_at":"2026-08-16T14:07:14.418502Z","submitted_at":"2024-03-22T18:00:09Z","title":"Minimal decaying dark matter: from cosmological tensions to neutrino signatures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.15543","snapshot_observed_at":"2026-08-01T13:07:49.427452Z","title":"Minimal decaying dark matter: from cosmological tensions to neutrino signatures","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":44,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.427452Z"},"links":{"cited_paper":"/paper/2403.15543","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:6df6a84663513ebd8e666d8964b8c3a1e7d2758a67fd172951cc3fdb05ae33f1","observation_id":"66bca469-b389-44de-9d01-0bdbda100dfc","resolution":{"observed_at":"2026-08-01T13:07:49.427452Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2426","last_updated":"2012-01-11T21:24:58Z","snapshot_observed_at":"2026-08-15T04:22:43.488554Z","submitted_at":"2012-01-11T21:24:58Z","title":"Effects of Unstable Dark Matter on Large-Scale Structure and Constraints from Future Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2426","snapshot_observed_at":"2026-08-01T13:07:49.505618Z","title":"Effects of Unstable Dark Matter on Large-Scale Structure and Constraints from Future Surveys","venue":null,"work_id":null,"year":2012},"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":45,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.505618Z"},"links":{"cited_paper":"/paper/1201.2426","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:194efacd792d63ae8e62dc88a25684539507e77797032adc4a983e3031a16ed4","observation_id":"0518fe3e-5082-4aec-81ea-4e6600b01a1f","resolution":{"observed_at":"2026-08-01T13:07:49.505618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.05682","last_updated":"2015-11-03T02:58:35Z","snapshot_observed_at":"2026-08-14T22:55:43.712981Z","submitted_at":"2015-03-19T09:40:47Z","title":"Cosmological Structure Formation in Decaying Dark Matter Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.05682","snapshot_observed_at":"2026-08-01T13:07:49.702391Z","title":null,"venue":null,"work_id":null,"year":2015},"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":46,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.702391Z"},"links":{"cited_paper":"/paper/1503.05682","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:c1829ba174b55a04da96738ec481efed73f15dad7b83667bb929105cec6c1d36","observation_id":"17016713-bcc3-4050-a5f8-d0f561935948","resolution":{"observed_at":"2026-08-01T13:07:49.702391Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03222","last_updated":"2024-04-17T08:36:47Z","snapshot_observed_at":"2026-08-16T15:18:08.756714Z","submitted_at":"2023-07-06T18:00:01Z","title":"Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03222","snapshot_observed_at":"2026-08-01T13:07:49.775466Z","title":"and Peters, Fabian Hervas and Schneider, Aurel","venue":null,"work_id":null,"year":2024},"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":47,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.775466Z"},"links":{"cited_paper":"/paper/2307.03222","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:5e8deb30388850662dd8b2b5f7ffd2fa65e556b8a954028c3491061dfe7badfe","observation_id":"8033d718-401f-4dfc-b2b5-ac0f90191315","resolution":{"observed_at":"2026-08-01T13:07:49.775466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01632","last_updated":"2021-05-12T08:23:56Z","snapshot_observed_at":"2026-08-16T19:08:27.977728Z","submitted_at":"2020-11-03T11:18:10Z","title":"Updated constraints on decaying cold dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01632","snapshot_observed_at":"2026-08-01T13:07:49.907110Z","title":"Updated constraints on decaying cold dark matter","venue":null,"work_id":null,"year":2021},"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":48,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:49.907110Z"},"links":{"cited_paper":"/paper/2011.01632","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:127895b3fa2bd8d04600d616fe5a4720342660b5156876ad08df119d3fafbe89","observation_id":"d5aef4a5-e628-4616-b992-e77fc412fa26","resolution":{"observed_at":"2026-08-01T13:07:49.907110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01935","last_updated":"2022-11-03T16:21:09Z","snapshot_observed_at":"2026-08-16T16:18:49.094444Z","submitted_at":"2022-11-03T16:21:09Z","title":"Discovering a new well: Decaying dark matter with profile likelihoods","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.01935","snapshot_observed_at":"2026-08-01T13:07:50.007568Z","title":"Decaying dark matter with profile likelihoods","venue":null,"work_id":null,"year":2023},"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":49,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.007568Z"},"links":{"cited_paper":"/paper/2211.01935","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:d31358a8dc86475ee6ea9e2932aef748a2b69b58e2de713a2a7d4a34475e9097","observation_id":"a83dd61b-d0d7-4ddb-82a9-234058051502","resolution":{"observed_at":"2026-08-01T13:07:50.007568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.07440","last_updated":"2022-07-06T10:29:34Z","snapshot_observed_at":"2026-08-16T17:14:38.040072Z","submitted_at":"2022-03-14T19:00:03Z","title":"Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.07440","snapshot_observed_at":"2026-08-01T13:07:50.180525Z","title":"Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures","venue":null,"work_id":null,"year":2022},"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":50,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.180525Z"},"links":{"cited_paper":"/paper/2203.07440","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:8984566f089ca0db7979c22f6ab523925ccbe300e6bead362994ef3223b0263b","observation_id":"28d8b5fb-7a88-4f36-9771-4fc6cc41b701","resolution":{"observed_at":"2026-08-01T13:07:50.180525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20193","last_updated":"2025-08-25T12:54:13Z","snapshot_observed_at":"2026-08-13T18:56:48.381737Z","submitted_at":"2025-05-26T16:38:29Z","title":"A frequentist view on the two-body decaying dark matter model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20193","snapshot_observed_at":"2026-08-01T13:07:50.305907Z","title":"and Poudou, Ad \\`e le and Poulin, Vivian","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":51,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.305907Z"},"links":{"cited_paper":"/paper/2505.20193","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:461d62d48b02a596033c15ea7509128801696e13e02b9eb33f8c6bd61ca3d561","observation_id":"1f5ad9c3-efd4-4fa4-806f-052ba3733e2d","resolution":{"observed_at":"2026-08-01T13:07:50.305907Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.7354","last_updated":"2013-09-27T20:00:59Z","snapshot_observed_at":"2026-08-15T00:01:29.341362Z","submitted_at":"2013-09-27T20:00:59Z","title":"Lyman-alpha Forest Constraints on Decaying Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.7354","snapshot_observed_at":"2026-08-01T13:07:50.399724Z","title":null,"venue":null,"work_id":null,"year":2013},"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":52,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.399724Z"},"links":{"cited_paper":"/paper/1309.7354","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:097f587ae7ed49cadbcb94850773c807da196bebb4b5bec6fdb658bc21fda8fe","observation_id":"efa1ad5e-c38e-4a51-a0b9-dbdeae17a1a9","resolution":{"observed_at":"2026-08-01T13:07:50.399724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.06117","last_updated":"2022-10-12T12:22:30Z","snapshot_observed_at":"2026-08-16T16:44:44.374234Z","submitted_at":"2022-10-12T12:22:30Z","title":"Decaying Dark Matter and Lyman-$\\alpha$ forest constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.06117","snapshot_observed_at":"2026-08-01T13:07:50.473375Z","title":"Decaying Dark Matter and Lyman- forest constraints","venue":null,"work_id":null,"year":2023},"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":53,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.473375Z"},"links":{"cited_paper":"/paper/2210.06117","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:8280fbbf20d5bbe2be5a17eff906a648b658b8cc293b8268cbbc40c60d634091","observation_id":"71198d12-db98-41d3-a23a-0032d9a665bd","resolution":{"observed_at":"2026-08-01T13:07:50.473375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.1912","last_updated":"2010-09-09T23:07:54Z","snapshot_observed_at":"2026-08-15T05:09:11.078904Z","submitted_at":"2010-09-09T23:07:54Z","title":"Dark-matter decays and Milky Way satellite galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.1912","snapshot_observed_at":"2026-08-01T13:07:50.626267Z","title":null,"venue":null,"work_id":null,"year":2010},"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":54,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.626267Z"},"links":{"cited_paper":"/paper/1009.1912","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:3f455eb46ef074610d19587029a49c95b694c5aaed78f33d69bcd74885ce9b98","observation_id":"a3146f11-7a64-46ed-8124-c0f0f1771fdf","resolution":{"observed_at":"2026-08-01T13:07:50.626267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.0527","last_updated":"2014-06-12T17:39:04Z","snapshot_observed_at":"2026-08-14T23:31:50.141971Z","submitted_at":"2014-06-02T20:19:41Z","title":"Cosmological Simulations of Decaying Dark Matter: Implications for Small-scale Structure of Dark Matter Halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.0527","snapshot_observed_at":"2026-08-01T13:07:50.745268Z","title":null,"venue":null,"work_id":null,"year":2014},"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":55,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.745268Z"},"links":{"cited_paper":"/paper/1406.0527","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:235eaf23f2476b0bbd2f17c46738cb827fe34ffaf2bda2ee172cf7a982f71223","observation_id":"d1463d3d-bb17-45c0-bbea-ed1bff82cb01","resolution":{"observed_at":"2026-08-01T13:07:50.745268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.11740","last_updated":"2022-06-27T17:11:53Z","snapshot_observed_at":"2026-08-16T17:25:26.435456Z","submitted_at":"2022-01-27T18:58:33Z","title":"Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.11740","snapshot_observed_at":"2026-08-01T13:07:50.866407Z","title":"and others","venue":null,"work_id":null,"year":2022},"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":56,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.866407Z"},"links":{"cited_paper":"/paper/2201.11740","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:8aec3cda075285a186dda6b0ea8cdaa2f2738f4bce06315de7a8693bfa0a4b7e","observation_id":"a1306727-040d-45a4-b6a1-09d5df1f1232","resolution":{"observed_at":"2026-08-01T13:07:50.866407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.14607","last_updated":"2020-08-06T17:22:16Z","snapshot_observed_at":"2026-08-15T15:26:52.394112Z","submitted_at":"2020-05-29T14:45:44Z","title":"Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.14607","snapshot_observed_at":"2026-08-01T13:07:50.975208Z","title":"Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations","venue":null,"work_id":null,"year":2020},"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":57,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:50.975208Z"},"links":{"cited_paper":"/paper/2005.14607","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:8e5151fc03dfdd45969269eb2c68778c1e65525684f976a26ea23b38786f18b8","observation_id":"3c5f8fcb-de13-40ed-83b7-d03bcb75385b","resolution":{"observed_at":"2026-08-01T13:07:50.975208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.13800","last_updated":"2022-02-15T08:49:14Z","snapshot_observed_at":"2026-08-16T19:10:30.066410Z","submitted_at":"2020-10-26T18:00:03Z","title":"Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.13800","snapshot_observed_at":"2026-08-01T13:07:51.044476Z","title":"and others","venue":null,"work_id":null,"year":2021},"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":58,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.044476Z"},"links":{"cited_paper":"/paper/2010.13800","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:1eff8fecb0d9174aa41f3c0fae0a02c7c6de5affc821b5660291417c8e1b6e3b","observation_id":"facb5809-548f-4460-857e-6b06603375d0","resolution":{"observed_at":"2026-08-01T13:07:51.044476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03606","last_updated":"2022-09-12T10:41:41Z","snapshot_observed_at":"2026-08-16T17:36:30.837827Z","submitted_at":"2021-12-07T09:55:14Z","title":"Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03606","snapshot_observed_at":"2026-08-01T13:07:51.155185Z","title":"and others","venue":null,"work_id":null,"year":2022},"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":59,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.155185Z"},"links":{"cited_paper":"/paper/2112.03606","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:558d925bbdcbb17f5bd47b3ee97260ae17e32bbdc9d81786464f6a4479b2f112","observation_id":"814cd0e5-45a0-46b1-b0d6-6b468b2430db","resolution":{"observed_at":"2026-08-01T13:07:51.155185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.13025","last_updated":"2023-09-22T17:41:12Z","snapshot_observed_at":"2026-08-16T14:58:22.055610Z","submitted_at":"2023-09-22T17:41:12Z","title":"Optical Cluster Cosmology with SDSS redMaPPer clusters and HSC-Y3 lensing measurements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.13025","snapshot_observed_at":"2026-08-01T13:07:51.265372Z","title":"Optical cluster cosmology with SDSS redMaPPer clusters and HSC-Y3 lensing measurements","venue":null,"work_id":null,"year":2024},"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":60,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.265372Z"},"links":{"cited_paper":"/paper/2309.13025","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:a5e8a132020ca8ebd8f87d67e153c6dda0b1a15dc42de45351aca207188db9a7","observation_id":"7378d419-5bfb-483e-b9a0-e24f482cae7a","resolution":{"observed_at":"2026-08-01T13:07:51.265372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.02075","last_updated":"2024-06-21T09:24:52Z","snapshot_observed_at":"2026-08-16T14:29:56.823971Z","submitted_at":"2024-01-04T05:56:27Z","title":"SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.02075","snapshot_observed_at":"2026-08-01T13:07:51.375421Z","title":"and others","venue":null,"work_id":null,"year":2024},"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":61,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.375421Z"},"links":{"cited_paper":"/paper/2401.02075","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:6689325cc270e8d3b4615658a3695b1cc10447b73a7c9641e575b32e32cff129","observation_id":"3e8f735d-5082-44da-bb19-7f41a7e2a725","resolution":{"observed_at":"2026-08-01T13:07:51.375421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04006","last_updated":"2024-10-03T13:29:16Z","snapshot_observed_at":"2026-08-16T14:21:00.556807Z","submitted_at":"2024-02-06T14:01:33Z","title":"Cosmological constraints from the Chandra-Planck galaxy cluster sample","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04006","snapshot_observed_at":"2026-08-01T13:07:51.460087Z","title":"and others","venue":null,"work_id":null,"year":2024},"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":62,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.460087Z"},"links":{"cited_paper":"/paper/2402.04006","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:ab02375ca65e6078f03d65b3f116462b441bfd47ba85ac175a467816bbc53b76","observation_id":"f3b8ef2c-04fa-40a2-bf2b-1375761c6c47","resolution":{"observed_at":"2026-08-01T13:07:51.460087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09499","last_updated":"2024-10-12T11:27:32Z","snapshot_observed_at":"2026-08-16T13:10:03.977621Z","submitted_at":"2024-10-12T11:27:32Z","title":"The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.09499","snapshot_observed_at":"2026-08-01T13:07:51.577335Z","title":"and others","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":63,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.577335Z"},"links":{"cited_paper":"/paper/2410.09499","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:1c97abb4691cdee50667cc662b0a7636661055ed81162bb585a9936e704cf4f8","observation_id":"2d7febc8-6fe8-459e-8767-ebe43b468314","resolution":{"observed_at":"2026-08-01T13:07:51.577335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.12636","last_updated":"2025-05-15T14:45:04Z","snapshot_observed_at":"2026-08-16T14:38:32.551471Z","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":"sha256:2bfab6df830934e6d38b5434f76262a393215cdfbde8ab7373784023492c1960","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:51.747126Z","title":"and Schechter, Paul","venue":null,"work_id":null,"year":1974},"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":65,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.747126Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:48572530b5246c529cfbc78f9bf17f2b87e9b02cc83700e434be0a7acac5e555","observation_id":"cf5b39b5-fe60-46da-bb02-00ebe92d9dd1","resolution":{"observed_at":"2026-08-01T13:07:51.747126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:51.804896Z","title":null,"venue":null,"work_id":null,"year":1991},"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":66,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.804896Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:0e38d00153d19a541f37e047ff0c2fcf97744bc4485ad993d7f4cac89714e85d","observation_id":"dde7c842-e1d6-4c15-92d7-75039aa30683","resolution":{"observed_at":"2026-08-01T13:07:51.804896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:51.872832Z","title":"and Gott, III, J","venue":null,"work_id":null,"year":1972},"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":67,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.872832Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:21e002a7789450427ed840c06574cd394630667983bb1f7851e855cdf848b465","observation_id":"59b4afcc-0780-43dc-9147-e7c0d29418f7","resolution":{"observed_at":"2026-08-01T13:07:51.872832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:51.995300Z","title":"and Primack, Joel R","venue":null,"work_id":null,"year":1991},"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":68,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:51.995300Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:40bf8bcb2d64703267799ab6c830b0b1ce25d0c804dd21ee5e35c478c001930e","observation_id":"9ae63136-723d-4add-af18-2fba075121e2","resolution":{"observed_at":"2026-08-01T13:07:51.995300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9601088","last_updated":"1996-01-16T15:43:21Z","snapshot_observed_at":"2026-07-07T01:12:36.776963Z","submitted_at":"1996-01-16T15:43:21Z","title":"Using the Evolution of Clusters to Constrain Omega","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9601088","snapshot_observed_at":"2026-08-01T13:07:52.095000Z","title":"and Cole, Shaun and Frenk, Carlos S","venue":null,"work_id":null,"year":1996},"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":69,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.095000Z"},"links":{"cited_paper":"/paper/astro-ph/9601088","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:c66c576c22d64424f05adbcdf224d533dd7dedec8cf1dbb706927fd56bf047e3","observation_id":"32649607-984e-419f-9ff7-69bb20de7909","resolution":{"observed_at":"2026-08-01T13:07:52.095000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0206508","last_updated":"2002-06-28T16:31:31Z","snapshot_observed_at":"2026-07-07T00:27:08.422279Z","submitted_at":"2002-06-28T16:31:31Z","title":"Halo Models of Large Scale Structure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0206508","snapshot_observed_at":"2026-08-01T13:07:52.282091Z","title":"Halo Models of Large Scale Structure","venue":null,"work_id":null,"year":2002},"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":70,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.282091Z"},"links":{"cited_paper":"/paper/astro-ph/0206508","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:517f0513074ba62f93b0033fa4229ba477f5bc134239ba84f72d298e6416a3ac","observation_id":"a93e7202-accc-4b61-aa63-97b660d2b49f","resolution":{"observed_at":"2026-08-01T13:07:52.282091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:52.365690Z","title":"and Tormen, Giuseppe","venue":null,"work_id":null,"year":1999},"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":71,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.365690Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:b01a9954c9dc48c7d27b53bcd262809fc03218271044e4f97b8eb83bff2a6795","observation_id":"5257563b-37eb-4d5d-a08a-3d9b1a008c8c","resolution":{"observed_at":"2026-08-01T13:07:52.365690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:52.461741Z","title":"and Tormen, Giuseppe","venue":null,"work_id":null,"year":2002},"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":72,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.461741Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:2132d1101dbaf422b6e1c2f4bd9f36949fe2cb2d0abdf8aeda4f3b9002bf962f","observation_id":"c17d5389-984b-427a-9a78-b4e6f9349383","resolution":{"observed_at":"2026-08-01T13:07:52.461741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.1249","last_updated":"2009-10-21T08:29:05Z","snapshot_observed_at":"2026-08-15T05:53:28.218075Z","submitted_at":"2009-03-06T17:36:58Z","title":"The Halo Mass Function from Excursion Set Theory. I. Gaussian fluctuations with non-markovian dependence on the smoothing scale","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.1249","snapshot_observed_at":"2026-08-01T13:07:52.535176Z","title":"The Halo Mass Function from Excursion Set Theory","venue":null,"work_id":null,"year":2010},"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":73,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.535176Z"},"links":{"cited_paper":"/paper/0903.1249","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:a58d01f9bee155b40bf15470264f12a8bc14bf20deb761e7699924cb24123d48","observation_id":"d9b5d0e9-e44a-423e-bea6-bfdd8fa57ef3","resolution":{"observed_at":"2026-08-01T13:07:52.535176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.1250","last_updated":"2009-10-21T10:36:24Z","snapshot_observed_at":"2026-08-15T05:53:28.173670Z","submitted_at":"2009-03-06T17:27:50Z","title":"The Halo Mass Function from Excursion Set Theory. II. The Diffusing Barrier","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.1250","snapshot_observed_at":"2026-08-01T13:07:52.676232Z","title":"The Halo mass function from excursion set theory","venue":null,"work_id":null,"year":2010},"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":74,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.676232Z"},"links":{"cited_paper":"/paper/0903.1250","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:8b0be9b7161a740079caadb8e5da39c9cd52a15e0770e2e19d151356b7fb2f15","observation_id":"4556e0ce-afae-4180-9224-8bcebb293e98","resolution":{"observed_at":"2026-08-01T13:07:52.676232Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:52.784765Z","title":"One step beyond: The excursion set approach with correlated steps","venue":null,"work_id":null,"year":2012},"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":75,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.784765Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:e1e63fd19954fa6b3fee751ce405d8570c2948442cbd47168a300e7e52f6fc2f","observation_id":"f147aa48-20ed-4bb7-8d26-779e42e1f27c","resolution":{"observed_at":"2026-08-01T13:07:52.784765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.09147","last_updated":"2021-10-27T09:58:55Z","snapshot_observed_at":"2026-08-14T16:03:52.881703Z","submitted_at":"2019-07-22T06:24:19Z","title":"Excursion set peaks in energy as a model for haloes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.09147","snapshot_observed_at":"2026-08-01T13:07:52.917040Z","title":"Excursion set peaks in energy as a model for haloes","venue":null,"work_id":null,"year":2021},"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":77,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:52.917040Z"},"links":{"cited_paper":"/paper/1907.09147","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:f33dccc22e94e4b1c1dff7712ca1fba7975645cc59aeaa33489839bab23fac37","observation_id":"4be07050-76e6-4d38-96fb-52d3106e73c2","resolution":{"observed_at":"2026-08-01T13:07:52.917040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07735","last_updated":"2025-03-10T18:00:14Z","snapshot_observed_at":"2026-08-16T12:51:23.844963Z","submitted_at":"2025-03-10T18:00:14Z","title":"Excursion Sets with a \"Perfect\" Collapse Model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.07735","snapshot_observed_at":"2026-08-01T13:07:53.019167Z","title":"Excursion sets with a perfect collapse model","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":78,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.019167Z"},"links":{"cited_paper":"/paper/2503.07735","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:5895f5752e45ef6afb3d3ee3b7f0a4d2de89130e1ebdbc93ccbd0127c5314e6f","observation_id":"2078ac8d-8384-4bde-8f70-4395600d98d8","resolution":{"observed_at":"2026-08-01T13:07:53.019167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:53.100216Z","title":"and Frenk, C","venue":null,"work_id":null,"year":2001},"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":79,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.100216Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:aaeda95fa38188d6cb4a714ee33b75eec3f254f90f54b88aa44e4d298811cefb","observation_id":"f70f1238-66a1-4ddd-bcc2-9ec3daaf34e1","resolution":{"observed_at":"2026-08-01T13:07:53.100216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0110246","last_updated":"2002-03-12T04:50:29Z","snapshot_observed_at":"2026-07-07T00:22:15.812463Z","submitted_at":"2001-10-10T19:31:49Z","title":"Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey Populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0110246","snapshot_observed_at":"2026-08-01T13:07:53.161757Z","title":null,"venue":null,"work_id":null,"year":2002},"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":80,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.161757Z"},"links":{"cited_paper":"/paper/astro-ph/0110246","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:64c4b7778e65691fbeaa0f5d50ead64f62ed1fee73286ce1a1949b8dca843439","observation_id":"be9922b5-f0e1-469c-a7d5-eea7113d733b","resolution":{"observed_at":"2026-08-01T13:07:53.161757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:53.292197Z","title":"and Stadel, Joachim and Fardal, Mark and Lake, George and Governato, Fabio","venue":null,"work_id":null,"year":2003},"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":81,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.292197Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:d8bf67358f0a3a5a4fcb40aa8a5849ad98078cc23b8f03017346ab7260036602","observation_id":"3428283c-26c3-4753-b59f-efd1423dd6e1","resolution":{"observed_at":"2026-08-01T13:07:53.292197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:53.492424Z","title":"Universal halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions","venue":null,"work_id":null,"year":2010},"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":83,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.492424Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:1efc67dad45b8e4dd39c87bd8d465ae341bc9d8c0ecaaa68a172b767bbea5458","observation_id":"9e90747a-7948-4b3e-8b80-444f125aa26c","resolution":{"observed_at":"2026-08-01T13:07:53.492424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.2706","last_updated":"2008-03-18T22:17:55Z","snapshot_observed_at":"2026-08-15T10:19:18.668493Z","submitted_at":"2008-03-18T22:17:55Z","title":"Toward a halo mass function for precision cosmology: the limits of universality","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.2706","snapshot_observed_at":"2026-08-01T13:07:53.544938Z","title":"and Kravtsov, Andrey V","venue":null,"work_id":null,"year":2008},"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":84,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.544938Z"},"links":{"cited_paper":"/paper/0803.2706","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:ea546b33f9d25da222c224d59bc3ca36b730b7bc6579cf45781f2fb7e69227c8","observation_id":"429aae23-58ee-44eb-b811-4839f584ddf2","resolution":{"observed_at":"2026-08-01T13:07:53.544938Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:53.636244Z","title":null,"venue":null,"work_id":null,"year":2012},"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":85,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.636244Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:e8a729668c26d8483942a45620fb9b3dbc8aa942d28fbcd4f570c1e5461aa30d","observation_id":"5f86e7de-08a0-4b81-bb8e-a31d3287c0b0","resolution":{"observed_at":"2026-08-01T13:07:53.636244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.0095","last_updated":"2013-11-09T09:42:51Z","snapshot_observed_at":"2026-08-15T00:37:29.083278Z","submitted_at":"2012-12-01T11:17:28Z","title":"The halo mass function through the cosmic ages","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.0095","snapshot_observed_at":"2026-08-01T13:07:53.714102Z","title":"and Iliev, Ilian T","venue":null,"work_id":null,"year":2013},"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":86,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.714102Z"},"links":{"cited_paper":"/paper/1212.0095","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:bb1b86d0754ce0b8da0baa79fe80368c870f999fc8b71370098f6fd796706f93","observation_id":"8037b268-f613-42b8-98e4-21eb0dda2bdb","resolution":{"observed_at":"2026-08-01T13:07:53.714102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07357","last_updated":"2015-12-22T09:42:15Z","snapshot_observed_at":"2026-08-15T03:10:42.701789Z","submitted_at":"2015-02-25T21:00:14Z","title":"Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07357","snapshot_observed_at":"2026-08-01T13:07:53.847865Z","title":"Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology","venue":null,"work_id":null,"year":2016},"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":87,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.847865Z"},"links":{"cited_paper":"/paper/1502.07357","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:0fdd9414180e80b43b34d50f64a5feb089f945b1d5768cb3a563a7dc45d49365","observation_id":"c5982da8-4df6-43cc-9d69-b591dbb9fc2b","resolution":{"observed_at":"2026-08-01T13:07:53.847865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.05627","last_updated":"2015-12-09T10:05:05Z","snapshot_observed_at":"2026-08-14T22:39:42.309473Z","submitted_at":"2015-07-20T20:01:10Z","title":"The universality of the virial halo mass function and models for non-universality of other halo definitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.05627","snapshot_observed_at":"2026-08-01T13:07:53.951213Z","title":"and Tormen, Giuseppe and Sheth, Ravi K","venue":null,"work_id":null,"year":2016},"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":88,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:53.951213Z"},"links":{"cited_paper":"/paper/1507.05627","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:2e18384dbd981f066f1a00e949160e557e80a3fcff1fdf1e91a4dcdacd375554","observation_id":"6b9e5705-a152-419c-9b7e-611b8b9bf3bd","resolution":{"observed_at":"2026-08-01T13:07:53.951213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.12116","last_updated":"2020-08-05T13:35:20Z","snapshot_observed_at":"2026-08-15T15:59:28.298636Z","submitted_at":"2020-03-26T19:23:24Z","title":"The Mira-Titan Universe. III. Emulation of the Halo Mass Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.12116","snapshot_observed_at":"2026-08-01T13:07:54.056860Z","title":"The Mira-Titan Universe","venue":null,"work_id":null,"year":2020},"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":89,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:54.056860Z"},"links":{"cited_paper":"/paper/2003.12116","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:b54da1194360568a40497caccb995f3d19f5421c7d29c730ea9e2370bfd07513","observation_id":"cdfa885f-a38f-49fd-b2b2-476f60e48722","resolution":{"observed_at":"2026-08-01T13:07:54.056860Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.03074","last_updated":"2025-07-03T18:00:02Z","snapshot_observed_at":"2026-08-16T04:24:12.123006Z","submitted_at":"2025-07-03T18:00:02Z","title":"Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.03074","snapshot_observed_at":"2026-08-01T13:07:54.163697Z","title":"Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions","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":90,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:54.163697Z"},"links":{"cited_paper":"/paper/2507.03074","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:249ba00f71e75b539a9064fa606ee6be7c577d1ae2c8a7471471bd180cc638cb","observation_id":"661c2019-cda2-4f04-bc12-fcbc155c511c","resolution":{"observed_at":"2026-08-01T13:07:54.163697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.0839","last_updated":"2013-06-11T10:21:04Z","snapshot_observed_at":"2026-08-15T00:26:38.214919Z","submitted_at":"2013-03-04T21:00:02Z","title":"Halo Mass Function and the Free Streaming Scale","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.0839","snapshot_observed_at":"2026-08-01T13:07:54.321545Z","title":"and Reed, Darren","venue":null,"work_id":null,"year":2013},"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":91,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:54.321545Z"},"links":{"cited_paper":"/paper/1303.0839","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:d31959708959fa669085ec4340d5a9e386afaa2086fa5695507080912e53bbee","observation_id":"bfc7fea2-a281-4300-b4ec-96bd4fe6ef25","resolution":{"observed_at":"2026-08-01T13:07:54.321545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.2133","last_updated":"2015-04-10T10:36:46Z","snapshot_observed_at":"2026-08-14T23:08:44.818027Z","submitted_at":"2014-12-05T21:00:05Z","title":"Structure formation with suppressed small-scale perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.2133","snapshot_observed_at":"2026-08-01T13:07:54.453594Z","title":"Structure formation with suppressed small-scale perturbations","venue":null,"work_id":null,"year":2015},"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":92,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:54.453594Z"},"links":{"cited_paper":"/paper/1412.2133","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:ac97dfbc63523a70953070293eabe65b996fd28962258857339908e6af095988","observation_id":"d060051f-5a57-45ed-bd74-da8ca4e292e9","resolution":{"observed_at":"2026-08-01T13:07:54.453594Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09787","last_updated":"2019-01-14T18:30:24Z","snapshot_observed_at":"2026-08-14T21:28:02.510116Z","submitted_at":"2016-11-29T18:57:56Z","title":"Large-Scale Galaxy Bias","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09787","snapshot_observed_at":"2026-08-01T13:07:55.681851Z","title":"Large-Scale Galaxy Bias","venue":null,"work_id":null,"year":2018},"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":93,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:55.681851Z"},"links":{"cited_paper":"/paper/1611.09787","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:03e475f29df90758e4b48c507f35c28b339d8c631fe218c47aef281e5f487caf","observation_id":"77897a66-7fef-4ef7-8732-2f738600956b","resolution":{"observed_at":"2026-08-01T13:07:55.681851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508156","last_updated":"2005-09-20T11:38:05Z","snapshot_observed_at":"2026-07-07T00:52:50.750906Z","submitted_at":"2005-08-05T13:16:37Z","title":"Cosmological structure formation in a homogeneous dark energy background","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508156","snapshot_observed_at":"2026-08-01T13:07:58.367289Z","title":"Cosmological structure formation in a homogeneous dark energy background","venue":null,"work_id":null,"year":2005},"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":94,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.367289Z"},"links":{"cited_paper":"/paper/astro-ph/0508156","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:7e1ded77e309af9b717f2a5f30b8fdcb75f04b2a74ad281b498393404ff8640c","observation_id":"372af385-9548-4041-b69a-289bdddbe015","resolution":{"observed_at":"2026-08-01T13:07:58.367289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2932","last_updated":"2011-05-14T09:45:16Z","snapshot_observed_at":"2026-08-15T04:49:17.337493Z","submitted_at":"2011-04-14T22:06:14Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2932","snapshot_observed_at":"2026-08-01T13:07:58.439195Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview","venue":null,"work_id":null,"year":2011},"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":95,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.439195Z"},"links":{"cited_paper":"/paper/1104.2932","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:389ae7098a62e5e312c9fab64bb72225da458d8f33baac3179fb720bdf06d700","observation_id":"243892b5-1b0c-4578-9e6c-a37ee9cbf3b7","resolution":{"observed_at":"2026-08-01T13:07:58.439195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2933","last_updated":"2011-08-17T09:25:04Z","snapshot_observed_at":"2026-08-09T14:29:15.405022Z","submitted_at":"2011-04-14T22:06:43Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2933","snapshot_observed_at":"2026-08-01T13:07:58.516724Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes","venue":null,"work_id":null,"year":2011},"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":96,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.516724Z"},"links":{"cited_paper":"/paper/1104.2933","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:fa989e35497f9dd89cbd1352b6f9f7b8e22c78a103ac2763aa5ba46cb878da7a","observation_id":"16a8d14b-47c3-49ff-8d73-82d9ba353831","resolution":{"observed_at":"2026-08-01T13:07:58.516724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.08621","last_updated":"2016-09-27T20:00:02Z","snapshot_observed_at":"2026-08-14T21:37:54.309312Z","submitted_at":"2016-09-27T20:00:02Z","title":"PKDGRAV3: Beyond Trillion Particle Cosmological Simulations for the Next Era of Galaxy Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.08621","snapshot_observed_at":"2026-08-01T13:07:58.606595Z","title":"PKDGRAV3: beyond trillion particle cosmological simulations for the next era of galaxy surveys","venue":null,"work_id":null,"year":2017},"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":97,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.606595Z"},"links":{"cited_paper":"/paper/1609.08621","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:55b55e96e7cabb9be62d00deccc3bcdbb59bbe030b2347099151f17254042021","observation_id":"c4c0611f-11c6-4733-b027-4f04af489859","resolution":{"observed_at":"2026-08-01T13:07:58.606595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611107","last_updated":"1997-10-21T23:14:37Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-13T22:59:55Z","title":"A Universal Density Profile from Hierarchical Clustering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611107","snapshot_observed_at":"2026-08-01T13:07:58.685102Z","title":"and Frenk, Carlos S","venue":null,"work_id":null,"year":1997},"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":98,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.685102Z"},"links":{"cited_paper":"/paper/astro-ph/9611107","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:14dfae7e76dfe61e37e3e209deffcd06b139c9991abf000e13abf9a420388f3f","observation_id":"0607e94d-619e-44ff-9a2b-6043c5de13ec","resolution":{"observed_at":"2026-08-01T13:07:58.685102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.04512","last_updated":"2018-12-18T23:10:45Z","snapshot_observed_at":"2026-08-15T21:39:07.739465Z","submitted_at":"2017-12-12T20:57:28Z","title":"COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.04512","snapshot_observed_at":"2026-08-01T13:07:58.760870Z","title":"COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos","venue":null,"work_id":null,"year":2018},"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":99,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.760870Z"},"links":{"cited_paper":"/paper/1712.04512","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:1a032ae0788711a2e9a16561c5e6f20a17a94d8dd66a16658fd06004a7d8d1c1","observation_id":"2be96c00-1912-4cfb-8a71-edbcf6245f33","resolution":{"observed_at":"2026-08-01T13:07:58.760870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.09615","last_updated":"2022-03-22T00:11:53Z","snapshot_observed_at":"2026-08-10T11:52:36.670902Z","submitted_at":"2020-08-21T18:00:03Z","title":"Implications of the $S_8$ tension for decaying dark matter with warm decay products","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.09615","snapshot_observed_at":"2026-08-01T13:07:58.862743Z","title":"Implications of the S_8 tension for decaying dark matter with warm decay products","venue":null,"work_id":null,"year":2022},"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":100,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.862743Z"},"links":{"cited_paper":"/paper/2008.09615","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:56c5efa2d2868b95c281f4a15fc262f8bbc6d72683d321dcb45c5a38131d6c98","observation_id":"881a3350-f14d-4d29-8589-980cefc8805a","resolution":{"observed_at":"2026-08-01T13:07:58.862743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T13:07:58.929364Z","title":null,"venue":null,"work_id":null,"year":null},"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":101,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:58.929364Z"},"links":{"citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:94b934f5d0705c589c0716f2c137117f645ee5c5d604f42d28024c210948b50b","observation_id":"0fff7ee0-21b0-4faa-adb2-308d2997b7b8","resolution":{"observed_at":"2026-08-01T13:07:58.929364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.3662","last_updated":"2009-04-23T11:34:08Z","snapshot_observed_at":"2026-08-15T05:49:56.625151Z","submitted_at":"2009-04-23T11:34:08Z","title":"Ahf: Amiga's Halo Finder","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.3662","snapshot_observed_at":"2026-08-01T13:07:59.040501Z","title":"and Knebe, Alexander","venue":null,"work_id":null,"year":2009},"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":102,"source":"arxiv_source","source_observed_at":"2026-08-01T13:07:59.040501Z"},"links":{"cited_paper":"/paper/0904.3662","citing_paper":"/paper/2607.19244"},"observation_digest":"sha256:27779e859ae458a0179d7ee62ef0b23c6e6da2ee29f586cd2d14ab8428b31715","observation_id":"5c1c0383-212c-4c94-b443-4505be7dce19","resolution":{"observed_at":"2026-08-01T13:07:59.040501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.19244","last_updated":"2026-07-21T16:15:17Z","latest_version":1,"primary_category":"astro-ph.CO","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"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":100},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 100 outbound references and 0 inbound Pith citation observations for arXiv:2607.19244."}