{"as_of":"2026-08-05T20:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bc37cc26efc18a72eb7c0dd2c68ef4af478efc0ae2a8adaddf48812da5003a87","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T10:55:46.250178Z","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":"2026-08-05T10:55:46.646484Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1108.5176","last_updated":"2012-02-09T22:50:02Z","snapshot_observed_at":"2026-07-06T02:32:57.774902Z","submitted_at":"2011-08-25T20:00:06Z","title":"Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance","version":2},"cited_work":{"arxiv_id":"1108.5176","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.5176","snapshot_observed_at":"2026-08-05T10:55:46.646484Z","title":"Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance","venue":"astro-ph.CO","work_id":"52c4da73-5126-4b62-a074-a2ca0489324a","year":2011},"citing_paper":{"arxiv_id":"2509.03595","last_updated":"2025-09-03T18:00:41Z","snapshot_observed_at":"2026-08-05T14:00:46.052520Z","submitted_at":"2025-09-03T18:00:41Z","title":"Tracing the Neutrino-Induced Phase Shift in the 21-cm Spectrum","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-05T10:55:46.250178Z"},"links":{"cited_paper":"/paper/1108.5176","citing_paper":"/paper/2509.03595"},"observation_digest":"sha256:cb0b2aacbd76d3c6844b92e8fe3dccd18577cffb9d32fd8cff8ed238fdc9abc9","observation_id":"1dd03cb0-52e5-4795-9651-5b2888d5d83e","resolution":{"observed_at":"2026-08-05T10:55:46.649435Z","resolver_source":"local_arxiv","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":"1108.5176","last_updated":"2012-02-09T22:50:02Z","snapshot_observed_at":"2026-07-06T02:32:57.774902Z","submitted_at":"2011-08-25T20:00:06Z","title":"Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.5176","snapshot_observed_at":"2026-07-14T15:06:13.177523Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.09846","last_updated":"2026-07-10T18:00:00Z","snapshot_observed_at":"2026-08-03T18:30:48.547340Z","submitted_at":"2026-07-10T18:00:00Z","title":"The Rise and Fall of Acoustic Oscillations at Cosmic Dawn","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-14T15:06:13.177523Z"},"links":{"cited_paper":"/paper/1108.5176","citing_paper":"/paper/2607.09846"},"observation_digest":"sha256:df31fda8aa418a256f9a0eb9ea1f81294ba1be7896ee675fd05dd15fe9676ef1","observation_id":"74c9bc1f-f1f1-4066-892b-0df06e52d70b","resolution":{"observed_at":"2026-07-14T15:06:13.177523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1108.5176/citation-record","integrity":"/paper/1108.5176/integrity","json":"/paper/1108.5176/citation-record.json","paper":"/paper/1108.5176"},"outbound":[],"paper":{"arxiv_id":"1108.5176","last_updated":"2012-02-09T22:50:02Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:32:57.774902Z","submitted_at":"2011-08-25T20:00:06Z","title":"Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance"},"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 2 inbound Pith citation observations for arXiv:1108.5176."}