{"as_of":"2026-08-09T07:18:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b3330a15fa086b49dc1bcf285ab92a507d5d098b38b5bb0cbcdf86c463b4579d","coverage":[{"denominator":56,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":56,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T06:01:07.635848Z","state":"measured"},{"denominator":59,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":59,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T18:54:48.018973Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-19T08:47:13.121897Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"cited_work":{"arxiv_id":"2506.06272","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.06272","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark mat- ter mass segregation","venue":null,"work_id":"e048fb6c-e9a0-4014-a3b6-af502d343d72","year":2025},"citing_paper":{"arxiv_id":"2506.14898","last_updated":"2026-02-04T14:06:10Z","snapshot_observed_at":"2026-07-06T21:43:50.059555Z","submitted_at":"2025-06-17T18:13:07Z","title":"Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-19T08:45:57.029664Z"},"links":{"cited_paper":"/paper/2506.06272","citing_paper":"/paper/2506.14898"},"observation_digest":"sha256:248f99996612323d1fcede719d18e2eafbea3f27fcb3d3abad6912ce814f2c93","observation_id":"b39326df-a453-4f8d-bdf2-94b11c6fc7af","resolution":{"observed_at":"2026-05-19T08:47:13.125730Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.06272","snapshot_observed_at":"2026-08-02T18:54:48.018973Z","title":"& Fischer, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.04508","last_updated":"2026-06-26T21:34:55Z","snapshot_observed_at":"2026-08-07T23:43:56.060663Z","submitted_at":"2026-03-04T19:00:20Z","title":"The dark fate of ultra-faint dwarfs: Gravothermal collapse in action","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-02T18:54:48.018973Z"},"links":{"cited_paper":"/paper/2506.06272","citing_paper":"/paper/2603.04508"},"observation_digest":"sha256:d04b79b07caa729280809edac15f9243c01115ad2f513cc3dcb50f520b715830","observation_id":"b79b8252-703c-437d-b53a-ea3620260b1d","resolution":{"observed_at":"2026-08-02T18:54:48.018973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.06272","snapshot_observed_at":"2026-07-31T04:54:06.828298Z","title":"Patil and M.S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28517","last_updated":"2026-07-30T16:55:29Z","snapshot_observed_at":"2026-08-06T02:08:11.250516Z","submitted_at":"2026-07-30T16:55:29Z","title":"Dynamical flattening of halo density cusps by Q-ball dark matter","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-31T04:54:06.828298Z"},"links":{"cited_paper":"/paper/2506.06272","citing_paper":"/paper/2607.28517"},"observation_digest":"sha256:ddb484aa75d92d473674b1898b34b1207add05d795048d2cb1c3dcc83d082b7c","observation_id":"e29387f7-579a-4f85-b10e-3050d931159f","resolution":{"observed_at":"2026-07-31T04:54:06.828298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2506.06272/citation-record","integrity":"/paper/2506.06272/integrity","json":"/paper/2506.06272/citation-record.json","paper":"/paper/2506.06272"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.329428Z","title":"K., et al","venue":null,"work_id":"12637746-3400-4bac-b3a9-340ed3f2791c","year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.418070Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:d5e16f212630b6f49ed075152a91455cbbef01d629d6165c43fbbbc9a7414bf6","observation_id":"193daaa1-e493-47a7-b3c9-5c010cebfefb","resolution":{"observed_at":"2026-08-07T06:01:08.332975Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.422341Z","title":"J., Goodwin, S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.422341Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:5d310530d3618d6ebc4286b54e98aa4bd2a79faba31f2d540d06f9ae21733dcb","observation_id":"c1420e95-a5ef-43e6-ae75-7e858101264e","resolution":{"observed_at":"2026-08-07T06:01:07.422341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.311258Z","title":"S., & Garny, M","venue":null,"work_id":"3221bbeb-b9e5-4c70-b7e3-e9714b99ee8b","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.426901Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:30191de712bb2928dc2eaf538ece1fef0b211b8ca5941b43968f061abdb2a50d","observation_id":"6c094077-9e60-4523-8265-9b7326658284","resolution":{"observed_at":"2026-08-07T06:01:08.314930Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.300155Z","title":"Y ., et al","venue":null,"work_id":"d314bb92-b1a4-4900-af37-030f7ab5b121","year":2020},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.431621Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:f1c52a1e4064dc90412cec8ca0d716c73b6c31f6058465fa68f660aa95b8b562","observation_id":"d01d2c3d-f3a9-4c70-92d3-9fa0408137d8","resolution":{"observed_at":"2026-08-07T06:01:08.303783Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.436716Z","title":"W., Price-Whelan, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.436716Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:1c3e4b06b7e3fd3470ecea87bed5300e8d9c2438a5a084d4ba80b10d31560c3a","observation_id":"a83ec48d-4991-4273-a43a-953213b6b3d8","resolution":{"observed_at":"2026-08-07T06:01:07.436716Z","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":"2026-08-07T06:01:07.441277Z","title":"1952, MNRAS, 112, 195","venue":null,"work_id":null,"year":1952},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.441277Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:c7a09ccd69b47e1d8b4a2f5aa8f47d3426057a409fa5a9050d005edf1681b0de","observation_id":"f9248465-88d1-45ad-b012-c2dc57b2763f","resolution":{"observed_at":"2026-08-07T06:01:07.441277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.274889Z","title":"W., et al","venue":null,"work_id":"1202ad19-85b4-4e9d-ae75-2cbc7db2fb64","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.446101Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:18151895be3eacacd9e508c54cc06c8b7425bbbe26d21fa0be2ce56840a5b1ec","observation_id":"54cf8158-0980-40ae-b9a6-887a77cd3995","resolution":{"observed_at":"2026-08-07T06:01:08.278424Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.264870Z","title":"2024, Dark Matter","venue":null,"work_id":"6df91407-718e-4f20-bbb2-f64470e0ebea","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.450456Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:f2e2695919fa9259b7babaa2dd97ef3fed101b6501b8d0a50e482c0f4f84f4a2","observation_id":"4194a223-21df-4f54-940d-5929379873ef","resolution":{"observed_at":"2026-08-07T06:01:08.268360Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.254290Z","title":"A., Schaller, M., Schaye, J., et al","venue":null,"work_id":"8817e07d-dc5c-4192-8936-3d839b66b3f0","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.454486Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:d93a073cab6d765c798029dd2767d2e886829a552cdf81a516c3cbbc917a6295","observation_id":"6d6f116d-accd-46ea-99c7-f4c5c3f5099a","resolution":{"observed_at":"2026-08-07T06:01:08.257969Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.243341Z","title":"M., Fassnacht, C","venue":null,"work_id":"2e0de145-50ea-4c14-b86e-3ede8351e33f","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.458742Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:5d0091a58bab8a5b382292d2e24ee2266cd0310d2e425d5fa3c08f9bd5e0bda9","observation_id":"8a6f2d1f-08e5-40f0-aad9-e2cf7c7e412f","resolution":{"observed_at":"2026-08-07T06:01:08.246875Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.232223Z","title":"2025, A&A, 697, A213","venue":null,"work_id":"d9c77f11-eb84-4fa2-9d59-7fe16ae4a9e0","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.462543Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:1c7af43be45476823c682aaaf6e00653df43fe4f2afd552dc60a2ad79115d4f8","observation_id":"cb8c5ac1-e906-4144-bd77-6b69428e2f1c","resolution":{"observed_at":"2026-08-07T06:01:08.236025Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.221481Z","title":"2014, Phys","venue":null,"work_id":"729f0892-1243-47cb-8e17-3569c2156776","year":2014},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.466165Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:8238ff3938193ffdfacf7d97fb9b4766dd013e1566ad1dda46fed489084765b8","observation_id":"714c817a-284e-410f-9902-7f32ff4eadcd","resolution":{"observed_at":"2026-08-07T06:01:08.225032Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.210476Z","title":null,"venue":null,"work_id":"6cfb650a-4876-4aed-8031-1427ff5b8e5e","year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.469778Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b0703aa0e060a6802e9b199ed50416b9a51832d8fbd8001e756a1926c4cc9ee4","observation_id":"137655a1-331e-4a5b-9432-2fdd0f4cd8d6","resolution":{"observed_at":"2026-08-07T06:01:08.213956Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.198089Z","title":"2025, Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots","venue":null,"work_id":"80dd1951-f9eb-4b52-9de9-123b515a5854","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.473147Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:5548159688231f008ab54d6b4e0005273b665918e75c859c9a95668c91a62ebd","observation_id":"d00753df-3cad-475d-a74a-d2503a4fb64b","resolution":{"observed_at":"2026-08-07T06:01:08.202353Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.184814Z","title":"S., Brüggen, M., Schmidt-Hoberg, K., et al","venue":null,"work_id":"336e8bb9-ac1c-4c7c-9786-12ff83ae1cb9","year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.476504Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b57d6dcbfb71f2ad91ab71bcba591b8fc7c0fe0b720e768971207cd01a0a34cc","observation_id":"c7e67e35-8acd-4e29-a80f-23835552f413","resolution":{"observed_at":"2026-08-07T06:01:08.189155Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.173779Z","title":"S., Dolag, K., & Yu, H.-B","venue":null,"work_id":"b6551436-686f-4b50-9d3b-a79e409460f5","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.480180Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:3abfa68efac0d33a2ec91efe13e613c782eb962eac38ddd4667ea9b68bcdc044","observation_id":"e747a460-cd37-4e5c-ae9e-4878b7273259","resolution":{"observed_at":"2026-08-07T06:01:08.177834Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.163134Z","title":"S., Kasselmann, L., Brüggen, M., et al","venue":null,"work_id":"c4f3eb6e-e5dd-4786-a5cb-1ade5134526b","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.483832Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:fa5c8e4b5673ac8d5de9b4cdb909e70459d111f6fea210147d7e6b426b389cb8","observation_id":"732fb124-0f6d-464c-92a0-f9c5f455efbb","resolution":{"observed_at":"2026-08-07T06:01:08.166773Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.152147Z","title":"S., & Lally, J","venue":null,"work_id":"e79fec59-9beb-4352-9310-4c707056e7dc","year":2013},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.487427Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:002608e89ad74c6a2b8bbce250aa638ae1c2c2a4ab16b13c1ff052a922d15104","observation_id":"b6304ebe-ca39-43ca-b8be-5d5f8bab324c","resolution":{"observed_at":"2026-08-07T06:01:08.155777Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.141112Z","title":"2022, A&A, 659, A24","venue":null,"work_id":"a86bf792-504d-4ccb-97a2-b026415633dc","year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.491005Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b8763141d615c13b9792214aa92b156d5b29ebe1342cc74df78ca9ba12e2bbab","observation_id":"086ff9ea-3bb7-4dd3-b10d-6b9c53d49f7e","resolution":{"observed_at":"2026-08-07T06:01:08.144723Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.494490Z","title":"P., Valentini, M., & Dolag, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.494490Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:a54e06d38862f76e26154731a9d66b458195fe1836f74e490f9475653f88c04d","observation_id":"837a38e6-c044-47a2-b9cc-d1cf393f221f","resolution":{"observed_at":"2026-08-07T06:01:07.494490Z","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":"2026-08-07T06:01:07.498396Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.498396Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b8926fa75c2f96b78390af37565261926a423cc6dba6b5a9fe0d366c09978f75","observation_id":"0a069f38-0ed0-462f-a54d-6efdeb1d7f44","resolution":{"observed_at":"2026-08-07T06:01:07.498396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.115222Z","title":"W., et al","venue":null,"work_id":"8c735988-739b-44fe-8a79-73570ef6822c","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.502087Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:099737e5d41a21c9f32fdd4e0265776661774f51e0894c255c1b3f393bd5b4f3","observation_id":"34394d52-fd5e-4e8f-841a-37ac64b12f21","resolution":{"observed_at":"2026-08-07T06:01:08.119157Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.103783Z","title":null,"venue":null,"work_id":"a7dc562b-a37e-4bff-bcd6-a52561d6feea","year":2007},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.505867Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:3e4986a32c18157aa89985571680a91d461db8e2bd55f1575d98b1cd1ee87b94","observation_id":"39c8285e-3657-41bb-b214-d6b83c3d77be","resolution":{"observed_at":"2026-08-07T06:01:08.107718Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.093253Z","title":"T., & Sarkar, S","venue":null,"work_id":"ee9bab5e-4e26-424e-a867-4fb71dd666b0","year":2014},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.509548Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:10cf0dbb524c7674047cd9ed31f1771de775b9d809f8c27bc0ecdfff4edc4ba1","observation_id":"557a9ae6-7014-4229-8da2-cf68c40d771a","resolution":{"observed_at":"2026-08-07T06:01:08.096813Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.082500Z","title":"Little Dark Dot","venue":null,"work_id":"da8ecc0d-89b7-4d79-b7dc-75965fa73dda","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.513393Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:e6e0bf10b4c1d4d6e584206a683f5eb0b4215c1a7a0ea8b3f48426d8091986b4","observation_id":"3d1ba0ec-625f-47bd-b218-7bb7914b728e","resolution":{"observed_at":"2026-08-07T06:01:08.086048Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.070273Z","title":"D., Fall, S","venue":null,"work_id":"b8c43255-a8e0-40b4-b636-b09999730c9f","year":2023},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.517144Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:d64b3a09cc03e49b285082939d0cd70476a35a703029875116e2f0932341f07e","observation_id":"3d1252b3-d30a-41b8-9f41-70dfa8b4ec0e","resolution":{"observed_at":"2026-08-07T06:01:08.074181Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.058894Z","title":"D., Schaye, J., Schaller, M., & Richings, J","venue":null,"work_id":"9b6a90a2-e82c-4afc-9fe9-d960cb3541fe","year":2019},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.520682Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:88a66dcc30919c082df4925914085d2ed5f21da77fab6fa55f7ebb94da553622","observation_id":"2a53068c-af81-421c-bac7-44164ac6f451","resolution":{"observed_at":"2026-08-07T06:01:08.062737Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.047155Z","title":"C., Peter, A","venue":null,"work_id":"d3df98ec-58f1-4a28-86b4-522aecb0d4e7","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.524551Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:04007a0464df0204e88d061eede884f1024ea24ff88780668d64292f09ac2cdc","observation_id":"44850638-beea-4d8c-9392-71b001422f30","resolution":{"observed_at":"2026-08-07T06:01:08.051026Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.034996Z","title":"2020, Science, 369, 1347–1351","venue":null,"work_id":"2bc6fe93-9c71-433c-89a0-3dd13e28a441","year":2020},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.528998Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:e8ce4606169382d8ecdafb8323c6cb94efc208e24921c1a45a1517c58ec1ea95","observation_id":"f09b4938-749f-4ebf-8d97-226522e36798","resolution":{"observed_at":"2026-08-07T06:01:08.039127Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.023276Z","title":"2021, MNRAS, 507, 1662–1683","venue":null,"work_id":"3177819b-32fe-4a29-8e63-303337122f0f","year":2021},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.534752Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:6af3d52759f373f4bf732a46c528ede904860f62749244db63c419000622fac7","observation_id":"722bd87b-9b02-425d-8364-312ba89f1908","resolution":{"observed_at":"2026-08-07T06:01:08.027057Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:08.011648Z","title":null,"venue":null,"work_id":"b84c8c98-c64c-4f0c-8db5-fafee704dbf1","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.539899Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:ab3e52393d14d703b3a7c0c40ab542d514314d09cc8b2cce2ba782fb4ee7384d","observation_id":"073196e8-5152-4690-89ca-2232fe9ff167","resolution":{"observed_at":"2026-08-07T06:01:08.015908Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.544275Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.544275Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:1a122500135d76a4c93fff22164cbaef78e56d6798a27b4740231692d117d45f","observation_id":"b17185b4-7929-4d57-a2d8-cedc077a019b","resolution":{"observed_at":"2026-08-07T06:01:07.544275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.989454Z","title":null,"venue":null,"work_id":"a2bac653-d022-4f36-bc79-e0e7cbd4a494","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.548527Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:9593d8f7e5292249af770e493b375ff198237d89f8c24a2951e5043bbc96aeeb","observation_id":"005a845e-0706-4dd0-9dca-521358751e7a","resolution":{"observed_at":"2026-08-07T06:01:07.994728Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.971848Z","title":"O., Yang, D., & Yu, H.-B","venue":null,"work_id":"4e71eaa6-c4c3-4a12-9ffa-b7ed6a613810","year":2023},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.552254Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:ad97e369710a31443ba6ec77e7599654221ce8ce89a8126d6bddfd233aa0249e","observation_id":"476fe8f1-fdea-43c7-a353-20978748d35c","resolution":{"observed_at":"2026-08-07T06:01:07.976623Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.555732Z","title":"F., Frenk, C","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.555732Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:5e77fed6cbecab3c8e8ea428438ea743fe03b111a5cae9a1b8d61ad3d98b3b6d","observation_id":"6fc06b89-37af-4019-9c75-724081b5db78","resolution":{"observed_at":"2026-08-07T06:01:07.555732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.949546Z","title":"2011, A&A, 532, A119","venue":null,"work_id":"e670fe0a-f797-471d-944e-f898c3d68c78","year":2011},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.559644Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:8cf092bcc60c5c56a4338837733ec94d3d02ef3a9475ed6d58177d251fcf79a5","observation_id":"e1bc9ab5-2152-4571-8ea5-8fc8a75ac3f7","resolution":{"observed_at":"2026-08-07T06:01:07.953451Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.936830Z","title":null,"venue":null,"work_id":"357687aa-9b0a-4b12-8fe7-d8c8756c7f19","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.563539Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:1d1e0a91f9247b031e139decbe5bb34c93ff9d9a2ab25aa4b01b9aeb5245b58b","observation_id":"4f9a5586-e140-4b70-a893-77d720e19046","resolution":{"observed_at":"2026-08-07T06:01:07.941343Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.921661Z","title":"2024, Digital Image Processing in Signatures of Self-Interacting Dark Matter Halo Mergers and Isolated Evolution","venue":null,"work_id":"6f1b569b-7ee5-4777-8b0f-86be41827482","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.566925Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:56c96aad41f9d1a03826733cc4249bae1b1237e527827027143a799ac707fbca","observation_id":"2d67cdb5-d2f6-451a-996e-cc5ef843d694","resolution":{"observed_at":"2026-08-07T06:01:07.926999Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.906145Z","title":"N., & Steinhardt, P","venue":null,"work_id":"70096a20-8570-47e3-8f3f-0f1db2884d1f","year":2015},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.570337Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b680eb390746ff8bc2ece6bcfe861ecd26337abafa9a41bd0867391c405104a8","observation_id":"9919042c-fe96-4775-ba1d-90255900fc9f","resolution":{"observed_at":"2026-08-07T06:01:07.910799Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.894395Z","title":"2024, A&A, 687, A270","venue":null,"work_id":"1d764ac1-a462-4908-99e7-36136712e415","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.573945Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b25419de501fb1bc793ea2e4fe29a121903a198c61f9eec86346d980194aa4a7","observation_id":"0917e67d-4a8d-4ae4-9dc5-6e75aae0e1d8","resolution":{"observed_at":"2026-08-07T06:01:07.898462Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.577884Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.577884Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:12cfec20ffb93c2ac55701fdb6b773090e417b9308735e5de9f5dc0552ca92b7","observation_id":"2f0d09a7-ba84-4add-8b26-203406fe3b49","resolution":{"observed_at":"2026-08-07T06:01:07.577884Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.876093Z","title":"2025, Gravothermalizing into primor- dial black holes, boson stars, and cannibal stars","venue":null,"work_id":"4fb950e5-5155-45e4-b84b-2e847690d0a1","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.581469Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:ff1106f771ccc237c595a96a33196ba53ea1d3d5a1234095fb58de8457240ce9","observation_id":"33388307-6fa9-41d2-84ac-08fc22fb8e21","resolution":{"observed_at":"2026-08-07T06:01:07.880258Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.864467Z","title":"2017, MNRAS, 467, 4719","venue":null,"work_id":"150b495f-eccc-4f5c-9658-bf85fd7d7245","year":2017},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.585463Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:7820f68254e0de28fb8161c7d3ed6558c715cfdb3315357467ebe2e462ffbaf1","observation_id":"3edc9d38-d0b8-4aed-ab8a-b483d52479e5","resolution":{"observed_at":"2026-08-07T06:01:07.868308Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.853032Z","title":null,"venue":null,"work_id":"ef1fc861-e847-4b5d-ba6e-f19fdc0a2ba9","year":2013},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.589694Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:51b2568f95c769d661e3bf2f8bd5a85e35dec0585abb1cf9c24f89c6ae013b35","observation_id":"30b6e961-9415-4fdc-b206-f9e52f9f6403","resolution":{"observed_at":"2026-08-07T06:01:07.856727Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.842112Z","title":"C., Torrey, P., V ogelsberger, M., & O’Neil, S","venue":null,"work_id":"384a31f6-d82d-4300-ab2e-0fe2be492c0c","year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.594459Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:36073476c12971293d069d736bc0f1f147dff6dc121cba5fcd7619c987494bcd","observation_id":"76e17c39-296a-4dd6-b16f-32b4d232c245","resolution":{"observed_at":"2026-08-07T06:01:07.845851Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.598574Z","title":"M., Brüggen, M., Schmidt-Hoberg, K., & Fischer, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.598574Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:a381040d5112e6c6b36f871e412f53627765ce73694cd3d22889649922979848","observation_id":"1e9f7dd1-ea57-4e1f-8d10-d9345bf42c57","resolution":{"observed_at":"2026-08-07T06:01:07.598574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.830218Z","title":"M., Brüggen, M., Schmidt-Hoberg, K., Fischer, M","venue":null,"work_id":"85e70b06-7fa1-48cd-91e0-c67129dced4b","year":2024},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.602340Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:c1ef18d1e4e85e6e47b94828897ed048895af95ad92d68153da83a7ba8f6a923","observation_id":"247d9d42-d54b-4187-9c53-4a7552ea8d6f","resolution":{"observed_at":"2026-08-07T06:01:07.834450Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.605920Z","title":"V ., Wetzel, A., & Fattahi, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.605920Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:b8affce50e23768d8867f4c056fa32d6df3d41f6f5497d89a3e8d09620dc4059","observation_id":"241888ee-6d30-4a8b-854e-31862c8dea91","resolution":{"observed_at":"2026-08-07T06:01:07.605920Z","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":"2026-08-07T06:01:07.610802Z","title":"2005, MNRAS, 364, 1105","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.610802Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:72881a4597c72c4bda9e4cf63185635b27b221b3bf11c3a34f9120224fd06b8a","observation_id":"ebe878fa-2175-4b26-a7f5-0fd337a70f81","resolution":{"observed_at":"2026-08-07T06:01:07.610802Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.801298Z","title":"C., Boylan-Kolchin, M., Bullock, J","venue":null,"work_id":"26751c6e-64b6-43a3-9130-5a77e2e49525","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.614203Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:25ec23b197df0712ae9f89053b4ea1b8e5f93fec87fce8b158b362f224a95c00","observation_id":"9e82c18a-695a-4772-b0c4-4a009d43b4b2","resolution":{"observed_at":"2026-08-07T06:01:07.805160Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.788749Z","title":"M., et al","venue":null,"work_id":"75408689-3f83-4eed-8be9-978b755cb71e","year":2025},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.617929Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:fc17860cb040b03e6a1ac7f514d4f521d46ee819c78d91cf0b7907e0aa3db1b0","observation_id":"513f0356-03bc-4f47-a618-1cabb6be7831","resolution":{"observed_at":"2026-08-07T06:01:07.792617Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.621405Z","title":"& Yu, H.-B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.621405Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:e17483b4ff70e83d5ddb94153e9e6e84682826bd68ba5011614bfff5a914a58f","observation_id":"db02f9da-c959-4ca9-8bc2-a94daafe7b62","resolution":{"observed_at":"2026-08-07T06:01:07.621405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.769127Z","title":null,"venue":null,"work_id":"ca936e3f-d994-4773-8d1d-093dc1c373b9","year":2012},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.625229Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:a05a7297111a7f62894fee046ca97df87ca24f073734a09c97163a4a27a08668","observation_id":"c7ac6416-33c0-455c-bf5a-c858781bf0ba","resolution":{"observed_at":"2026-08-07T06:01:07.773336Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.757583Z","title":null,"venue":null,"work_id":"28d04873-ca85-420d-b3f3-0262fb3a9bc3","year":2010},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.628773Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:8c869125b52495ccd5666f37fca16ca00d4e58fc52c14edef546b37bbab98a38","observation_id":"8867fbaa-3cbc-4218-9966-4597909f4fa2","resolution":{"observed_at":"2026-08-07T06:01:07.761444Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.745972Z","title":"& Yu, H.-B","venue":null,"work_id":"cb7fc190-49e7-4e5e-b37a-3d6fdf63277a","year":2022},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.632361Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:32c13072fca475da04db229f8728d26f746447637086233764bfcf891d134628","observation_id":"c6d83c71-9c70-4992-b6d2-080d27d4417b","resolution":{"observed_at":"2026-08-07T06:01:07.749791Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T06:01:07.731732Z","title":"2023, MNRAS, 526, 758–770 Article number, page 11 of 13 A&A proofs: manuscript no","venue":null,"work_id":"0ee0d468-f398-4951-95ef-f4749aba47ca","year":2023},"citing_paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T06:01:07.635848Z"},"links":{"citing_paper":"/paper/2506.06272"},"observation_digest":"sha256:77969d2636ae496bf2229c7aae4f8605b0100a156237c2af6c6a82adee3bc776","observation_id":"7e0f63f2-bb7a-4cd3-88ad-1ec3df4f790b","resolution":{"observed_at":"2026-08-07T06:01:07.737070Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2506.06272","last_updated":"2025-06-30T10:48:18Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T05:54:47.055824Z","submitted_at":"2025-06-06T17:56:09Z","title":"To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation"},"reference_resolution":{"displayed":56,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":20,"verified_exact":0,"verified_fuzzy":35},"total_outbound_references":56},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 56 of 56 outbound references and 3 inbound Pith citation observations for arXiv:2506.06272."}