{"as_of":"2026-08-20T11:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:259bff23e6a11a7b41b9093e0972c50443e7e249f9df14e67b3967dc9c997b87","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:17:30.437299Z","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":"2026-07-03T14:58:32.881977Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-16T12:17:30.437299Z","title":"Zhang, H.-B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.13247","last_updated":"2025-04-17T18:00:00Z","snapshot_observed_at":"2026-08-19T15:23:39.544498Z","submitted_at":"2025-04-17T18:00:00Z","title":"Darkness in the Crust: Searching for the truly \"Dark\" Subhalos with Paleo-detectors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-16T12:17:30.437299Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2504.13247"},"observation_digest":"sha256:3f49427c37c1b1e09362d17fec7232e8a7d97c6fe753eb6908aa54f54592908b","observation_id":"0036cf62-2384-476d-bf41-037fecb1c6a7","resolution":{"observed_at":"2026-08-16T12:17:30.437299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-15T21:44:12.752178Z","title":"Zhang, H.-B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.09219","last_updated":"2025-09-02T11:42:34Z","snapshot_observed_at":"2026-08-16T11:41:47.362058Z","submitted_at":"2025-05-14T08:40:19Z","title":"Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-15T21:44:12.752178Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2505.09219"},"observation_digest":"sha256:8a36d156a30642f921fe19a08c62536689650cedc74ce35bf932bd3e1361d07c","observation_id":"1a26a055-a4ff-4449-ba73-f32b7750d7ba","resolution":{"observed_at":"2026-08-15T21:44:12.752178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-15T21:20:27.383330Z","title":"Zhang, H.-B","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.10451","last_updated":"2025-05-15T16:08:57Z","snapshot_observed_at":"2026-08-18T04:47:09.490817Z","submitted_at":"2025-05-15T16:08:57Z","title":"Constraints on dark matter self-interaction from velocity distribution function in isolated halos","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-08-15T21:20:27.383330Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2505.10451"},"observation_digest":"sha256:dbeccd45ef3a10066ca442deb22931f2394243408acde425874662c4a826ebce","observation_id":"ee1d6821-995e-4d86-8204-f3599c827c92","resolution":{"observed_at":"2026-08-15T21:20:27.383330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-15T19:14:10.104896Z","title":"The GD-1 Stellar Stream Perturber as a Core-collapsed Self-interacting Dark Matter Halo,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.17641","last_updated":"2025-06-21T08:47:00Z","snapshot_observed_at":"2026-08-19T01:59:04.751695Z","submitted_at":"2025-06-21T08:47:00Z","title":"Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T19:14:10.104896Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2506.17641"},"observation_digest":"sha256:3f0a0df128ad1e496d9087434d76a46eb117ab03ec896df118f99034d7d5ce9d","observation_id":"14fa0d46-a5f7-440e-a2a9-d67cc25102a7","resolution":{"observed_at":"2026-08-15T19:14:10.104896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-04T12:56:22.841213Z","title":"Zhang, H.-B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.01491","last_updated":"2026-07-15T03:08:10Z","snapshot_observed_at":"2026-08-16T17:12:24.385104Z","submitted_at":"2025-10-01T22:06:50Z","title":"Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T12:56:22.841213Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2510.01491"},"observation_digest":"sha256:c18fc50edf8db4af7ee39c4cb5607b7b5a184b5378fcd568272042895010c6cc","observation_id":"64a74b19-a538-43fc-805a-9f834eeb3b8f","resolution":{"observed_at":"2026-08-04T12:56:22.841213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-03T06:13:43.171683Z","title":"Zhang, H.-B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.23264","last_updated":"2026-06-11T13:48:14Z","snapshot_observed_at":"2026-08-14T05:11:55.106926Z","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":140,"source":"pdf_text","source_observed_at":"2026-08-03T06:13:43.171683Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2601.23264"},"observation_digest":"sha256:aa1d6a2b0c0a2911c1371013a45a20cbab55c3e4734eb63a7961b5a46039d89e","observation_id":"9e8f59c4-5bc1-4652-80a4-f5b74c412fce","resolution":{"observed_at":"2026-08-03T06:13:43.171683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":"2409.19493","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-07-03T14:58:32.881977Z","title":"Zhang, H.-B","venue":null,"work_id":"e57d0125-3c44-4abe-b91c-f0dc3d056f42","year":2025},"citing_paper":{"arxiv_id":"2604.08647","last_updated":"2026-04-09T17:59:18Z","snapshot_observed_at":"2026-08-11T16:22:53.547478Z","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":48,"source":"pdf_text","source_observed_at":"2026-05-10T16:51:41.665607Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2604.08647"},"observation_digest":"sha256:6cc3530c5960adbcf20b5dc61268daa158b4f59b1f01a2e534aa2c653c9422c7","observation_id":"1678201b-7fce-44fd-8fb7-526c95c3afb4","resolution":{"observed_at":"2026-05-11T08:00:58.470718Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":"2409.19493","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-07-03T14:58:32.881977Z","title":"Zhang, H.-B","venue":null,"work_id":"e57d0125-3c44-4abe-b91c-f0dc3d056f42","year":2025},"citing_paper":{"arxiv_id":"2606.12909","last_updated":"2026-06-11T05:08:09Z","snapshot_observed_at":"2026-07-06T23:51:45.306189Z","submitted_at":"2026-06-11T05:08:09Z","title":"SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$\\mathcal{V}$","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-27T06:50:27.397229Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2606.12909"},"observation_digest":"sha256:cb5ce6d06dd50ad31291c2b4af95bcd73f8fc304170cf88084f44f3740405e43","observation_id":"174a8db4-31d2-4e11-ad0b-a2bdce3ea577","resolution":{"observed_at":"2026-07-03T14:58:32.883304Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-07-11T06:38:02.275303Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.05504","last_updated":"2026-07-06T18:00:03Z","snapshot_observed_at":"2026-08-18T22:50:59.172095Z","submitted_at":"2026-07-06T18:00:03Z","title":"A Novel Implementation of Self-Interacting Dark Matter in AREPO","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-11T06:38:02.275303Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2607.05504"},"observation_digest":"sha256:dbbf7441eb8f8e6dcc03370c8d31c9b1beba597cd0d01234828ec90ef091f930","observation_id":"3a6f061a-5a6a-4a2f-bbb4-a1870636f4ab","resolution":{"observed_at":"2026-07-11T06:38:02.275303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.19493","snapshot_observed_at":"2026-08-01T06:39:32.581968Z","title":"Zhang, H.-B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.21834","last_updated":"2026-07-23T21:52:06Z","snapshot_observed_at":"2026-08-18T09:43:43.238120Z","submitted_at":"2026-07-23T21:52:06Z","title":"The diffraction-lensing interpretation of GW231123 with astrophysical priors","version":1},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-01T06:39:32.581968Z"},"links":{"cited_paper":"/paper/2409.19493","citing_paper":"/paper/2607.21834"},"observation_digest":"sha256:5cd66dd1ca12d39783de94b053c6a81470f607e5db1e9550e411f9273948252e","observation_id":"841119f4-c61e-4aa3-be6a-ad836b3cc40e","resolution":{"observed_at":"2026-08-01T06:39:32.581968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2409.19493/citation-record","integrity":"/paper/2409.19493/integrity","json":"/paper/2409.19493/citation-record.json","paper":"/paper/2409.19493"},"outbound":[],"paper":{"arxiv_id":"2409.19493","last_updated":"2024-12-29T01:28:19Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-20T09:35:59.411828Z","submitted_at":"2024-09-29T00:12:12Z","title":"The GD-1 stellar stream perturber as a core-collapsed self-interacting dark matter halo"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2409.19493."}