{"as_of":"2026-08-10T13:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:817d3368a5efb6722ebb3d48f14ff89d508086f0e7e22a50c5112a3a896a88c2","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T23:34:35.137636Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-01T20:36:11.592073Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-08T23:34:35.137636Z","title":"Nadler, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04108","last_updated":"2026-07-04T09:02:06Z","snapshot_observed_at":"2026-08-09T05:16:57.332180Z","submitted_at":"2025-02-06T14:33:36Z","title":"Can a secluded self-interacting dark sector generate detectable gravitational waves?","version":3},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-08-08T23:34:35.137636Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2502.04108"},"observation_digest":"sha256:eb4cc165f33c774437d420cc0f751619e22f122ccabf385e7c717eedb8c24f16","observation_id":"abab9484-eb4c-4c39-a39f-a8f198f06d7c","resolution":{"observed_at":"2026-08-08T23:34:35.137636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-07T10:52:20.202156Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.04334","last_updated":"2025-06-04T18:00:11Z","snapshot_observed_at":"2026-08-10T03:57:10.001709Z","submitted_at":"2025-06-04T18:00:11Z","title":"Numerical evolution of self-gravitating halos of self-interacting dark matter","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:20.202156Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2506.04334"},"observation_digest":"sha256:842d131595db95bbf91f6e8b266a89ad0381bee9c8ca12964a24d0df579864ad","observation_id":"c3176168-4954-45ae-8b4d-0a1ad33ff83e","resolution":{"observed_at":"2026-08-07T10:52:20.202156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":"2306.01830","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-07-01T20:36:11.592073Z","title":"A Self- interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","venue":null,"work_id":"66df25ae-29c0-45b2-a73e-b2feeae66450","year":2023},"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":34,"source":"pdf_text","source_observed_at":"2026-05-19T08:45:57.029664Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2506.14898"},"observation_digest":"sha256:c7ab9cb9718f7c97c11fd9d5f19060a93ab2886db242a64c32000b3af541aab7","observation_id":"1a71aef6-5526-484f-8584-19b4cafc79ac","resolution":{"observed_at":"2026-05-19T08:47:13.091666Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-05T14:45:20.909194Z","title":"Nadler, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.21121","last_updated":"2025-08-28T18:00:05Z","snapshot_observed_at":"2026-08-06T23:02:59.094956Z","submitted_at":"2025-08-28T18:00:05Z","title":"Pion dark matter in a $\\theta$ vacuum: a thermal relic with sharp velocity-dependent self-interactions","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-05T14:45:20.909194Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2508.21121"},"observation_digest":"sha256:a532734f9c981cca1e0ce1876048c091e1352a6d2670109ea8d93e577d0ba83f","observation_id":"c825f2bb-9210-436f-81bd-8a143a9da273","resolution":{"observed_at":"2026-08-05T14:45:20.909194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-04T20:07:03.191448Z","title":"Coun- terfactual world modeling for physical dynamics.arXiv preprint arXiv:2306.01830, 2023","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.09737","last_updated":"2025-09-10T18:01:04Z","snapshot_observed_at":"2026-08-08T13:38:01.687801Z","submitted_at":"2025-09-10T18:01:04Z","title":"World Modeling with Probabilistic Structure Integration","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T20:07:03.191448Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2509.09737"},"observation_digest":"sha256:0c5f4678deccf16c723786383e49ba7ae024c304e001d4b430f0372ac6469871","observation_id":"006df00c-f6f3-4bfe-81e3-2581343f6907","resolution":{"observed_at":"2026-08-04T20:07:03.191448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-04T12:56:18.178135Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.01491","last_updated":"2026-07-15T03:08:10Z","snapshot_observed_at":"2026-08-08T05:40:04.337530Z","submitted_at":"2025-10-01T22:06:50Z","title":"Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-04T12:56:18.178135Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2510.01491"},"observation_digest":"sha256:06558d01c0701c025ca91336a15c618c220961442e5aa3fa539a05c4e4241462","observation_id":"9d0022c0-c41f-4180-9d04-1732a45f4b80","resolution":{"observed_at":"2026-08-04T12:56:18.178135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":"2306.01830","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-07-01T20:36:11.592073Z","title":"A Self- interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","venue":null,"work_id":"66df25ae-29c0-45b2-a73e-b2feeae66450","year":2023},"citing_paper":{"arxiv_id":"2512.00145","last_updated":"2026-04-22T15:48:08Z","snapshot_observed_at":"2026-07-06T22:37:16.933664Z","submitted_at":"2025-11-28T19:00:00Z","title":"Role of prompt cusps in driving the core collapse of SIDM halos","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-17T03:26:00.496818Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2512.00145"},"observation_digest":"sha256:a670e950a5b279ce04de1cc5f326c7479047d1955585b5d3c89385259abc9300","observation_id":"98cdf09f-0507-4b9f-b9e9-337d21a3197d","resolution":{"observed_at":"2026-05-17T03:28:57.983507Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-03T06:13:45.832104Z","title":"Nadler, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2601.23264","last_updated":"2026-06-11T13:48:14Z","snapshot_observed_at":"2026-08-08T02:09:33.954242Z","submitted_at":"2026-01-30T18:33:03Z","title":"MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM","version":3},"reference_index":171,"source":"pdf_text","source_observed_at":"2026-08-03T06:13:45.832104Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2601.23264"},"observation_digest":"sha256:9e99ef3fddd0a3ec825f588873013adf9a57b7ded133e62434a4d8d584f4b788","observation_id":"fdaf1a1f-386d-4775-84f8-5956fefe393a","resolution":{"observed_at":"2026-08-03T06:13:45.832104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":"2306.01830","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-07-01T20:36:11.592073Z","title":"A Self- interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","venue":null,"work_id":"66df25ae-29c0-45b2-a73e-b2feeae66450","year":2023},"citing_paper":{"arxiv_id":"2604.08647","last_updated":"2026-04-09T17:59:18Z","snapshot_observed_at":"2026-08-01T03:59:27.972333Z","submitted_at":"2026-04-09T17:59:18Z","title":"Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-10T16:51:41.665607Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2604.08647"},"observation_digest":"sha256:fb9b8e28cf360c8eb4474346ae48899bac1990515bc5c5ce9f90fec5d561490a","observation_id":"76c4fd56-f8b8-445c-a8f2-5ea72c565d9c","resolution":{"observed_at":"2026-05-11T08:00:58.372273Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":"2306.01830","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-07-01T20:36:11.592073Z","title":"A Self- interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","venue":null,"work_id":"66df25ae-29c0-45b2-a73e-b2feeae66450","year":2023},"citing_paper":{"arxiv_id":"2604.15006","last_updated":"2026-04-27T10:40:26Z","snapshot_observed_at":"2026-08-09T14:47:51.870484Z","submitted_at":"2026-04-16T13:33:16Z","title":"Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-10T10:08:33.578196Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2604.15006"},"observation_digest":"sha256:6f4ee6aff316a57af34f59900da7a074097d82805bfbdfd8fdd0087a0e283913","observation_id":"753167b1-95c0-406b-add7-7bc78a86eeda","resolution":{"observed_at":"2026-05-10T10:09:06.838732Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":"2306.01830","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-07-01T20:36:11.592073Z","title":"A Self- interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","venue":null,"work_id":"66df25ae-29c0-45b2-a73e-b2feeae66450","year":2023},"citing_paper":{"arxiv_id":"2605.31335","last_updated":"2026-05-29T14:16:44Z","snapshot_observed_at":"2026-08-02T13:53:50.544392Z","submitted_at":"2026-05-29T14:16:44Z","title":"Gravothermal Collapse: Robust Against Baryonic Feedback","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-06-28T20:58:05.796638Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2605.31335"},"observation_digest":"sha256:f37cd9c78c762b3616d59869f4086e650ab093746aa4262d46c2faf68cf316a8","observation_id":"e53017e5-3bac-4267-b042-6edc3e8b6e19","resolution":{"observed_at":"2026-07-01T20:36:11.593594Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-02T06:19:14.304623Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.13141","last_updated":"2026-07-14T18:00:04Z","snapshot_observed_at":"2026-08-09T12:40:07.883915Z","submitted_at":"2026-07-14T18:00:04Z","title":"S-matrix bootstrap bounds on self-interacting dark matter","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-02T06:19:14.304623Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2607.13141"},"observation_digest":"sha256:2c32b0b0fdb9de629a5896d37d546395677943441fe316b053df96cbba3caccc","observation_id":"b2ba5eb8-4b48-4def-a27c-5dc70d1dbc02","resolution":{"observed_at":"2026-08-02T06:19:14.304623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-08-01T05:25:22.159323Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.22787","last_updated":"2026-07-24T12:25:13Z","snapshot_observed_at":"2026-08-05T20:06:33.852338Z","submitted_at":"2026-07-24T12:25:13Z","title":"Probing Dark Matter Substructure with Wave-Optics Distortions of Strongly Lensed LISA Gravitational Waves","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-01T05:25:22.159323Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2607.22787"},"observation_digest":"sha256:5a04f4722303d6b0199b821ed2da5556309a598112927905679fa4d2d7864bab","observation_id":"44c58a90-1989-4e70-bc40-e32970b08bcd","resolution":{"observed_at":"2026-08-01T05:25:22.159323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.01830","snapshot_observed_at":"2026-07-31T04:54:06.804811Z","title":"Nadler, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28517","last_updated":"2026-07-30T16:55:29Z","snapshot_observed_at":"2026-08-09T14:20:10.461308Z","submitted_at":"2026-07-30T16:55:29Z","title":"Dynamical flattening of halo density cusps by Q-ball dark matter","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-31T04:54:06.804811Z"},"links":{"cited_paper":"/paper/2306.01830","citing_paper":"/paper/2607.28517"},"observation_digest":"sha256:66c8ca7101a4ebb18a81100a4e1347afcac4156d8521a164f2c6b2137a5d99aa","observation_id":"7263b1cc-a6cd-4081-8966-42689076f7d9","resolution":{"observed_at":"2026-07-31T04:54:06.804811Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2306.01830/citation-record","integrity":"/paper/2306.01830/integrity","json":"/paper/2306.01830/citation-record.json","paper":"/paper/2306.01830"},"outbound":[],"paper":{"arxiv_id":"2306.01830","last_updated":"2023-11-30T18:26:04Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-08T19:41:30.491344Z","submitted_at":"2023-06-02T18:00:01Z","title":"A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2306.01830."}