{"as_of":"2026-08-17T03:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5e1062d31506c249b17f195739b25e19d93a117e122705aa491ce1bf1362914a","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:20:27.218285Z","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":"2026-05-19T08:47:12.801254Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2406.10753","last_updated":"2025-01-17T06:16:01Z","snapshot_observed_at":"2026-08-17T00:46:09.036012Z","submitted_at":"2024-06-15T22:48:57Z","title":"Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10753","snapshot_observed_at":"2026-08-15T21:20:27.218285Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.10451","last_updated":"2025-05-15T16:08:57Z","snapshot_observed_at":"2026-08-15T21:06:34.417349Z","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":58,"source":"pdf_text","source_observed_at":"2026-08-15T21:20:27.218285Z"},"links":{"cited_paper":"/paper/2406.10753","citing_paper":"/paper/2505.10451"},"observation_digest":"sha256:513fa875d03b05635ee1304fbdacc3f950360446cc11a8cfa3b1100a7c88af1e","observation_id":"f4a56d0b-faaa-41af-951b-e8a3f3ab7fc9","resolution":{"observed_at":"2026-08-15T21:20:27.218285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10753","last_updated":"2025-01-17T06:16:01Z","snapshot_observed_at":"2026-08-17T00:46:09.036012Z","submitted_at":"2024-06-15T22:48:57Z","title":"Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations","version":2},"cited_work":{"arxiv_id":"2406.10753","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.10753","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing the parametric model for self-interacting dark matter us- ing matched halos in cosmological simulations","venue":null,"work_id":"c8f9ca94-54f4-4e37-ae5e-3d5b2b9b360c","year":2025},"citing_paper":{"arxiv_id":"2506.14898","last_updated":"2026-02-04T14:06:10Z","snapshot_observed_at":"2026-08-16T23:49:49.266647Z","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":53,"source":"pdf_text","source_observed_at":"2026-05-19T08:45:57.029664Z"},"links":{"cited_paper":"/paper/2406.10753","citing_paper":"/paper/2506.14898"},"observation_digest":"sha256:5b86244b1f740110bc465be372301d229739a3a097dba6283ae4397774f5fd4b","observation_id":"8f9829ac-6ce2-40b6-b872-0d7d047d1bc6","resolution":{"observed_at":"2026-05-19T08:47:12.805854Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10753","last_updated":"2025-01-17T06:16:01Z","snapshot_observed_at":"2026-08-17T00:46:09.036012Z","submitted_at":"2024-06-15T22:48:57Z","title":"Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10753","snapshot_observed_at":"2026-08-04T12:56:22.107869Z","title":null,"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":49,"source":"pdf_text","source_observed_at":"2026-08-04T12:56:22.107869Z"},"links":{"cited_paper":"/paper/2406.10753","citing_paper":"/paper/2510.01491"},"observation_digest":"sha256:7a62d87a062a64c882d0611e9bf865d6dae923c4b3f1272c0f40b310d9f946e9","observation_id":"41c4ee63-8fa6-4906-9aaa-4195f92faf69","resolution":{"observed_at":"2026-08-04T12:56:22.107869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10753","last_updated":"2025-01-17T06:16:01Z","snapshot_observed_at":"2026-08-17T00:46:09.036012Z","submitted_at":"2024-06-15T22:48:57Z","title":"Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10753","snapshot_observed_at":"2026-08-03T06:13:41.115538Z","title":"Yang, E.O","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":119,"source":"pdf_text","source_observed_at":"2026-08-03T06:13:41.115538Z"},"links":{"cited_paper":"/paper/2406.10753","citing_paper":"/paper/2601.23264"},"observation_digest":"sha256:51fd1690b671acc95afab2ccd8a35d89ed5cad934b9ee24796b0390b0e7afb33","observation_id":"77a11207-262c-42f9-ab75-7dda33ce4631","resolution":{"observed_at":"2026-08-03T06:13:41.115538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10753","last_updated":"2025-01-17T06:16:01Z","snapshot_observed_at":"2026-08-17T00:46:09.036012Z","submitted_at":"2024-06-15T22:48:57Z","title":"Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations","version":2},"cited_work":{"arxiv_id":"2406.10753","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.10753","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing the parametric model for self-interacting dark matter us- ing matched halos in cosmological simulations","venue":null,"work_id":"c8f9ca94-54f4-4e37-ae5e-3d5b2b9b360c","year":2025},"citing_paper":{"arxiv_id":"2604.22013","last_updated":"2026-04-23T19:07:42Z","snapshot_observed_at":"2026-08-12T13:19:15.700541Z","submitted_at":"2026-04-23T19:07:42Z","title":"An Extended Parametric Model for Self-interacting Dark Matter Halos","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-05-09T20:37:08.191229Z"},"links":{"cited_paper":"/paper/2406.10753","citing_paper":"/paper/2604.22013"},"observation_digest":"sha256:fd322d2284a3f5dba37729388426812119264f0cdcb1289c4a327830996a0d09","observation_id":"58a57c4c-271b-4c66-ad6e-21d5e9ea5567","resolution":{"observed_at":"2026-05-11T15:11:05.256225Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2406.10753/citation-record","integrity":"/paper/2406.10753/integrity","json":"/paper/2406.10753/citation-record.json","paper":"/paper/2406.10753"},"outbound":[],"paper":{"arxiv_id":"2406.10753","last_updated":"2025-01-17T06:16:01Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T00:46:09.036012Z","submitted_at":"2024-06-15T22:48:57Z","title":"Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2406.10753."}