{"as_of":"2026-08-11T05:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:19ba783ecce609501d8da15c85bafacb44ad17d66d57000de2fa04e0a6ccf59c","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":"2026-08-10T06:31:04.303077+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":"2026-08-10T05:47:29.592195Z","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":"2026-05-12T00:36:17.502400Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1907.05424","last_updated":"2019-07-11T18:00:02Z","snapshot_observed_at":"2026-08-10T22:50:45.048247Z","submitted_at":"2019-07-11T18:00:02Z","title":"On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.05424","snapshot_observed_at":"2026-08-10T05:47:29.592195Z","title":"Zehavi, S.E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16908","last_updated":"2025-01-29T13:08:33Z","snapshot_observed_at":"2026-08-10T16:53:04.112608Z","submitted_at":"2025-01-28T12:51:50Z","title":"Impact of light sterile neutrinos on cosmological large scale structure","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T05:47:29.592195Z"},"links":{"cited_paper":"/paper/1907.05424","citing_paper":"/paper/2501.16908"},"observation_digest":"sha256:d29dbf7ff364c6348500dfe95b5cf7babd3802f8c2bdd07c6eacdb952580d5e1","observation_id":"d53ec31d-2aa4-4606-a29a-f5f3d23a4f7e","resolution":{"observed_at":"2026-08-10T05:47:29.592195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.05424","last_updated":"2019-07-11T18:00:02Z","snapshot_observed_at":"2026-08-10T22:50:45.048247Z","submitted_at":"2019-07-11T18:00:02Z","title":"On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection","version":1},"cited_work":{"arxiv_id":"1907.05424","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.05424","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zehavi, S.E","venue":null,"work_id":"ffa53c03-5e4a-47d3-bf53-6c319684f471","year":2019},"citing_paper":{"arxiv_id":"2604.26022","last_updated":"2026-04-30T00:23:11Z","snapshot_observed_at":"2026-07-06T23:11:48.524898Z","submitted_at":"2026-04-28T18:05:05Z","title":"Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-07T14:53:02.246257Z"},"links":{"cited_paper":"/paper/1907.05424","citing_paper":"/paper/2604.26022"},"observation_digest":"sha256:5e829fb311740bd846bc0f160406f8136a7cb2719b75a076da77f93a02504b7d","observation_id":"dd1768bb-9233-4be2-8881-15b51830e0de","resolution":{"observed_at":"2026-05-12T00:36:17.506063Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1907.05424/citation-record","integrity":"/paper/1907.05424/integrity","json":"/paper/1907.05424/citation-record.json","paper":"/paper/1907.05424"},"outbound":[],"paper":{"arxiv_id":"1907.05424","last_updated":"2019-07-11T18:00:02Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-10T22:50:45.048247Z","submitted_at":"2019-07-11T18:00:02Z","title":"On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1907.05424."}