{"as_of":"2026-08-20T19:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7aad0376b006f2e9c92ca6a0d527a39b81f7cd9321daa64a7385ae487e0f613f","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T19:54:48.358960Z","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":"2026-05-11T08:00:58.463069Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2007.13780","last_updated":"2020-10-27T17:09:14Z","snapshot_observed_at":"2026-07-06T09:42:14.127872Z","submitted_at":"2020-07-27T18:00:27Z","title":"Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.13780","snapshot_observed_at":"2026-08-04T19:54:48.358960Z","title":"Diversity of Dark Matter Density Profiles in the Galactic Dwarf Spheroidal Satellites,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.09012","last_updated":"2025-09-10T21:15:04Z","snapshot_observed_at":"2026-08-18T20:05:39.746694Z","submitted_at":"2025-09-10T21:15:04Z","title":"Decays and annihilation of galactic dark matter: determine $D$-, $J_s$-, $J_p$- and $J_d$-factors with dark matter profiles inferred from GravSphere fit to stellar observations","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T19:54:48.358960Z"},"links":{"cited_paper":"/paper/2007.13780","citing_paper":"/paper/2509.09012"},"observation_digest":"sha256:ead718c08f512150484d6a22850b8e05cc925edcf6963c03bb81c7b313d225f7","observation_id":"87755758-e2ee-4e10-8a4c-fca70fb1f631","resolution":{"observed_at":"2026-08-04T19:54:48.358960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.13780","last_updated":"2020-10-27T17:09:14Z","snapshot_observed_at":"2026-07-06T09:42:14.127872Z","submitted_at":"2020-07-27T18:00:27Z","title":"Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites","version":2},"cited_work":{"arxiv_id":"2007.13780","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.13780","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"31ab7ad4-b580-41e7-a903-63a320d01319","year":2020},"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":36,"source":"pdf_text","source_observed_at":"2026-05-10T16:51:41.665607Z"},"links":{"cited_paper":"/paper/2007.13780","citing_paper":"/paper/2604.08647"},"observation_digest":"sha256:d3d5f645e623405fb7096884136eeaf7f31176d5928d252ccd4808065d3b9882","observation_id":"90470317-3925-4d60-83dd-433734df1786","resolution":{"observed_at":"2026-05-11T08:00:58.466366Z","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":"2007.13780","last_updated":"2020-10-27T17:09:14Z","snapshot_observed_at":"2026-07-06T09:42:14.127872Z","submitted_at":"2020-07-27T18:00:27Z","title":"Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.13780","snapshot_observed_at":"2026-07-11T11:50:44.784525Z","title":"Hayashi, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.04893","last_updated":"2026-07-06T10:22:37Z","snapshot_observed_at":"2026-08-14T18:39:59.999538Z","submitted_at":"2026-07-06T10:22:37Z","title":"Collisionless damping of the gravitational instability in fuzzy dark matter: spectral shape and quantum-to-thermal crossover","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:44.784525Z"},"links":{"cited_paper":"/paper/2007.13780","citing_paper":"/paper/2607.04893"},"observation_digest":"sha256:be3b8ee553fc34a551d1ae7b35b12eff299c2f942112fe77322bf87ace358edc","observation_id":"24f503fe-ad08-4d4e-a01a-be94bbeabad0","resolution":{"observed_at":"2026-07-11T11:50:44.784525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.13780","last_updated":"2020-10-27T17:09:14Z","snapshot_observed_at":"2026-07-06T09:42:14.127872Z","submitted_at":"2020-07-27T18:00:27Z","title":"Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.13780","snapshot_observed_at":"2026-07-13T06:28:17.325404Z","title":", keywords =","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.08818","last_updated":"2026-07-09T18:00:01Z","snapshot_observed_at":"2026-08-19T18:38:32.208200Z","submitted_at":"2026-07-09T18:00:01Z","title":"Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-13T06:28:17.325404Z"},"links":{"cited_paper":"/paper/2007.13780","citing_paper":"/paper/2607.08818"},"observation_digest":"sha256:d9f1217a7cd1558d701efbb3cd3993d1120744547803c26fb231e1792e5640f8","observation_id":"05b16a33-fcb5-4b40-a9ce-04ba574a8262","resolution":{"observed_at":"2026-07-13T06:28:17.325404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2007.13780/citation-record","integrity":"/paper/2007.13780/integrity","json":"/paper/2007.13780/citation-record.json","paper":"/paper/2007.13780"},"outbound":[],"paper":{"arxiv_id":"2007.13780","last_updated":"2020-10-27T17:09:14Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T09:42:14.127872Z","submitted_at":"2020-07-27T18:00:27Z","title":"Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites"},"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 4 inbound Pith citation observations for arXiv:2007.13780."}