{"as_of":"2026-08-12T17:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:131c2a197faca9bd341f68b3547c2dbfd67417c18c292ffc62583ba16d7245c4","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":"2026-08-12T06:34:41.77262+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":"2026-08-01T06:39:34.606369Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-06-28T21:52:40.310672Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1501.04382","last_updated":"2015-08-03T04:17:13Z","snapshot_observed_at":"2026-08-10T12:23:46.631758Z","submitted_at":"2015-01-19T04:14:58Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","version":2},"cited_work":{"arxiv_id":"1501.04382","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.04382","snapshot_observed_at":"2026-06-28T21:52:40.310672Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","venue":"astro-ph.CO","work_id":"5d386500-f50a-4bac-9f1c-4aa517ed1d40","year":2015},"citing_paper":{"arxiv_id":"2606.00205","last_updated":"2026-05-29T18:00:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-29T18:00:00Z","title":"Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages","version":1},"reference_index":296,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1501.04382","citing_paper":"/paper/2606.00205"},"observation_digest":"sha256:37bb806b4db126fc2eeb18a6f791e0cb3e21153cf9b352aa8460fbd060e7f558","observation_id":"bdbe88e6-c13f-42ed-8af5-1b22a211e2f4","resolution":{"observed_at":"2026-06-28T21:52:40.312002Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.04382","last_updated":"2015-08-03T04:17:13Z","snapshot_observed_at":"2026-08-10T12:23:46.631758Z","submitted_at":"2015-01-19T04:14:58Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","version":2},"cited_work":{"arxiv_id":"1501.04382","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.04382","snapshot_observed_at":"2026-06-28T21:52:40.310672Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","venue":"astro-ph.CO","work_id":"5d386500-f50a-4bac-9f1c-4aa517ed1d40","year":2015},"citing_paper":{"arxiv_id":"2606.10027","last_updated":"2026-06-08T18:08:03Z","snapshot_observed_at":"2026-08-06T02:11:38.412927Z","submitted_at":"2026-06-08T18:08:03Z","title":"Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations","version":1},"reference_index":107,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1501.04382","citing_paper":"/paper/2606.10027"},"observation_digest":"sha256:2937b2849b1e6df9b4ff77edbaf0048b82145345e8d65fac76eb89b7f968f393","observation_id":"43f2b7de-1c83-48a5-baad-d2768d9cf24b","resolution":{"observed_at":"2026-06-27T15:51:01.836412Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.04382","last_updated":"2015-08-03T04:17:13Z","snapshot_observed_at":"2026-08-10T12:23:46.631758Z","submitted_at":"2015-01-19T04:14:58Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","version":2},"cited_work":{"arxiv_id":"1501.04382","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.04382","snapshot_observed_at":"2026-06-28T21:52:40.310672Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","venue":"astro-ph.CO","work_id":"5d386500-f50a-4bac-9f1c-4aa517ed1d40","year":2015},"citing_paper":{"arxiv_id":"2606.13393","last_updated":"2026-06-11T14:24:11Z","snapshot_observed_at":"2026-07-06T23:52:09.853158Z","submitted_at":"2026-06-11T14:24:11Z","title":"Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1501.04382","citing_paper":"/paper/2606.13393"},"observation_digest":"sha256:385b85c0fbd9257b59c99966200beb8573cc4c375bf4c1a48039c8d63c0b93f9","observation_id":"1f54f992-019a-4339-9786-efeb3fd4b459","resolution":{"observed_at":"2026-06-27T06:30:38.128047Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.04382","last_updated":"2015-08-03T04:17:13Z","snapshot_observed_at":"2026-08-10T12:23:46.631758Z","submitted_at":"2015-01-19T04:14:58Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.04382","snapshot_observed_at":"2026-08-01T06:39:34.606369Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.21834","last_updated":"2026-07-23T21:52:06Z","snapshot_observed_at":"2026-08-09T15:55:40.823637Z","submitted_at":"2026-07-23T21:52:06Z","title":"The diffraction-lensing interpretation of GW231123 with astrophysical priors","version":1},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-08-01T06:39:34.606369Z"},"links":{"cited_paper":"/paper/1501.04382","citing_paper":"/paper/2607.21834"},"observation_digest":"sha256:c5c8a92c142a6a8d262517bbe773f36d22992a658500f0ae5559ecc9f854d0a4","observation_id":"b7f0020c-9de9-4a69-a5f2-fe091368fd26","resolution":{"observed_at":"2026-08-01T06:39:34.606369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1501.04382/citation-record","integrity":"/paper/1501.04382/integrity","json":"/paper/1501.04382/citation-record.json","paper":"/paper/1501.04382"},"outbound":[],"paper":{"arxiv_id":"1501.04382","last_updated":"2015-08-03T04:17:13Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-10T12:23:46.631758Z","submitted_at":"2015-01-19T04:14:58Z","title":"The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1501.04382."}