{"as_of":"2026-08-05T09:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:667b2cedefff7569e164ab22ab4902c35fd2c606431c4b7b5904ea7f9a40700a","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":"2026-08-05T06:32:48.257954+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":"2026-08-03T19:05:25.503922Z","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":"2026-05-23T03:32:28.164111Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.08290","last_updated":"2024-10-10T18:21:25Z","snapshot_observed_at":"2026-07-06T19:31:27.349925Z","submitted_at":"2024-10-10T18:21:25Z","title":"COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history","version":1},"cited_work":{"arxiv_id":"2410.08290","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08290","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2024, arXiv e-prints","venue":null,"work_id":"4954f6c5-9f82-42b7-b511-640b61633140","year":2024},"citing_paper":{"arxiv_id":"2502.02637","last_updated":"2026-01-16T16:03:52Z","snapshot_observed_at":"2026-08-02T05:15:17.075129Z","submitted_at":"2025-02-04T19:00:01Z","title":"Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS","version":2},"reference_index":114,"source":"arxiv_source","source_observed_at":"2026-05-23T03:31:06.488636Z"},"links":{"cited_paper":"/paper/2410.08290","citing_paper":"/paper/2502.02637"},"observation_digest":"sha256:61ce97f1fb03bd5baa2c0dea674470df8a899641ec2a7d690a00214017056bb6","observation_id":"e196dd83-d1dd-4929-8e22-3c283cbd8062","resolution":{"observed_at":"2026-05-23T03:32:28.167062Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08290","last_updated":"2024-10-10T18:21:25Z","snapshot_observed_at":"2026-07-06T19:31:27.349925Z","submitted_at":"2024-10-10T18:21:25Z","title":"COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08290","snapshot_observed_at":"2026-08-03T19:05:25.503922Z","title":"Shuntov et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.02642","last_updated":"2026-06-01T10:30:50Z","snapshot_observed_at":"2026-08-03T19:05:11.241582Z","submitted_at":"2025-12-02T10:54:49Z","title":"The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T19:05:25.503922Z"},"links":{"cited_paper":"/paper/2410.08290","citing_paper":"/paper/2512.02642"},"observation_digest":"sha256:52c88e85b23f5545f554bc7a167b29cd7d66094c86b3e6a0255287a0aec51a53","observation_id":"467d1017-4b43-4eb4-9a92-428341073a0a","resolution":{"observed_at":"2026-08-03T19:05:25.503922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08290","last_updated":"2024-10-10T18:21:25Z","snapshot_observed_at":"2026-07-06T19:31:27.349925Z","submitted_at":"2024-10-10T18:21:25Z","title":"COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history","version":1},"cited_work":{"arxiv_id":"2410.08290","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08290","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2024, arXiv e-prints","venue":null,"work_id":"4954f6c5-9f82-42b7-b511-640b61633140","year":2024},"citing_paper":{"arxiv_id":"2604.24431","last_updated":"2026-04-27T12:58:55Z","snapshot_observed_at":"2026-07-06T23:10:29.508602Z","submitted_at":"2026-04-27T12:58:55Z","title":"CSST Preparations: Galaxy Completeness and S\\'ersic Profile Fitting across the Wide, Deep, and Extreme Fields","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-05-08T02:46:19.282636Z"},"links":{"cited_paper":"/paper/2410.08290","citing_paper":"/paper/2604.24431"},"observation_digest":"sha256:89ca58b09c3e6458b5230ba27ffb7b602f481dfe029ad85b2df7c6f3e66637de","observation_id":"f526e845-a3a9-458e-a68e-523d37894be6","resolution":{"observed_at":"2026-05-11T22:26:14.231201Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08290","last_updated":"2024-10-10T18:21:25Z","snapshot_observed_at":"2026-07-06T19:31:27.349925Z","submitted_at":"2024-10-10T18:21:25Z","title":"COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08290","snapshot_observed_at":"2026-08-02T12:34:35.121962Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.02773","last_updated":"2026-07-21T13:31:25Z","snapshot_observed_at":"2026-08-02T12:34:24.050336Z","submitted_at":"2026-06-01T18:35:41Z","title":"Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution","version":2},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-02T12:34:35.121962Z"},"links":{"cited_paper":"/paper/2410.08290","citing_paper":"/paper/2606.02773"},"observation_digest":"sha256:94eab49c21559b10ee656bccb5ee0aa3074cfef29f0aedafacc7cb60685d842d","observation_id":"88c089b6-4a0c-459d-8111-e98ba8f1ea9b","resolution":{"observed_at":"2026-08-02T12:34:35.121962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.08290/citation-record","integrity":"/paper/2410.08290/integrity","json":"/paper/2410.08290/citation-record.json","paper":"/paper/2410.08290"},"outbound":[],"paper":{"arxiv_id":"2410.08290","last_updated":"2024-10-10T18:21:25Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T19:31:27.349925Z","submitted_at":"2024-10-10T18:21:25Z","title":"COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2410.08290."}