{"as_of":"2026-08-07T05:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:21b858ac5d524e992da1cf6d16f6ce533788e740e916f9e5c1ad8c43f5a1ac73","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T23:42:37.950621Z","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":"2026-07-02T07:26:45.130410Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1306.3993","last_updated":"2013-10-01T21:24:57Z","snapshot_observed_at":"2026-07-06T03:16:01.396351Z","submitted_at":"2013-06-17T20:00:05Z","title":"Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias","version":2},"cited_work":{"arxiv_id":"1306.3993","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.3993","snapshot_observed_at":"2026-07-02T07:26:45.130410Z","title":"Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias","venue":"astro-ph.CO","work_id":"028a0570-1c01-4839-96ac-75a9417ac30f","year":2013},"citing_paper":{"arxiv_id":"2606.05355","last_updated":"2026-06-03T18:56:30Z","snapshot_observed_at":"2026-07-06T23:45:23.749718Z","submitted_at":"2026-06-03T18:56:30Z","title":"Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1306.3993","citing_paper":"/paper/2606.05355"},"observation_digest":"sha256:687e614bceb2515c368fbb9aaa04f9b2cadd04fee1f4c0171c707ad46a96e6f2","observation_id":"a24a3207-4305-4ac9-bb01-aa7101f30299","resolution":{"observed_at":"2026-06-28T05:01:39.372326Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1306.3993","last_updated":"2013-10-01T21:24:57Z","snapshot_observed_at":"2026-07-06T03:16:01.396351Z","submitted_at":"2013-06-17T20:00:05Z","title":"Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias","version":2},"cited_work":{"arxiv_id":"1306.3993","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.3993","snapshot_observed_at":"2026-07-02T07:26:45.130410Z","title":"Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias","venue":"astro-ph.CO","work_id":"028a0570-1c01-4839-96ac-75a9417ac30f","year":2013},"citing_paper":{"arxiv_id":"2607.00610","last_updated":"2026-07-01T08:35:07Z","snapshot_observed_at":"2026-07-07T00:06:14.968413Z","submitted_at":"2026-07-01T08:35:07Z","title":"Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches","version":1},"reference_index":239,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1306.3993","citing_paper":"/paper/2607.00610"},"observation_digest":"sha256:ce23d0dcc5ed4214cbeb42c6c77b15852580a74b9814c1cfec996cc97a761f23","observation_id":"7eb251db-e991-4a90-bae4-e240398de79b","resolution":{"observed_at":"2026-07-02T07:26:45.131786Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1306.3993","last_updated":"2013-10-01T21:24:57Z","snapshot_observed_at":"2026-07-06T03:16:01.396351Z","submitted_at":"2013-06-17T20:00:05Z","title":"Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.3993","snapshot_observed_at":"2026-08-01T23:42:37.950621Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15340","last_updated":"2026-07-16T18:00:27Z","snapshot_observed_at":"2026-08-05T12:18:29.663527Z","submitted_at":"2026-07-16T18:00:27Z","title":"How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-01T23:42:37.950621Z"},"links":{"cited_paper":"/paper/1306.3993","citing_paper":"/paper/2607.15340"},"observation_digest":"sha256:c6e29b26e7a8e9a08e0b857720f4f79873ce8e2adb1f64be5f873eb5f27fd9ee","observation_id":"8712b96c-9b7f-4ddc-a828-96c9b30d8a29","resolution":{"observed_at":"2026-08-01T23:42:37.950621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1306.3993/citation-record","integrity":"/paper/1306.3993/integrity","json":"/paper/1306.3993/citation-record.json","paper":"/paper/1306.3993"},"outbound":[],"paper":{"arxiv_id":"1306.3993","last_updated":"2013-10-01T21:24:57Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T03:16:01.396351Z","submitted_at":"2013-06-17T20:00:05Z","title":"Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1306.3993."}