{"as_of":"2026-08-04T23:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d911006089a6c69b37c5075b0d1dd79279ddc911f6f7bb50f7c0265bfae675ba","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":"2026-08-04T06:34:03.388597+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":"2026-07-13T02:04:26.563148Z","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":"2026-05-21T22:34:23.909359Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.07346","last_updated":"2025-07-25T13:32:05Z","snapshot_observed_at":"2026-07-06T21:54:48.150241Z","submitted_at":"2025-07-10T00:19:11Z","title":"CLASS_SZ II: Notes and Examples of Fast and Accurate Calculations of Halo Model, Large Scale Structure and Cosmic Microwave Background Observables","version":3},"cited_work":{"arxiv_id":"2507.07346","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.07346","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolliet, A","venue":null,"work_id":"71c47557-8346-49f2-afaa-7ebd8ffc86a1","year":2025},"citing_paper":{"arxiv_id":"2509.03458","last_updated":"2026-05-20T11:45:49Z","snapshot_observed_at":"2026-08-02T08:36:03.690606Z","submitted_at":"2025-09-03T16:33:04Z","title":"Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-21T22:33:13.258551Z"},"links":{"cited_paper":"/paper/2507.07346","citing_paper":"/paper/2509.03458"},"observation_digest":"sha256:fd539e49b25b31a513154f727d1d3098d3594b4900c68aab536b6c83b898dbe8","observation_id":"91f80b31-4bda-4deb-b563-2ad7e47e3b8e","resolution":{"observed_at":"2026-05-21T22:34:23.911133Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.07346","last_updated":"2025-07-25T13:32:05Z","snapshot_observed_at":"2026-07-06T21:54:48.150241Z","submitted_at":"2025-07-10T00:19:11Z","title":"CLASS_SZ II: Notes and Examples of Fast and Accurate Calculations of Halo Model, Large Scale Structure and Cosmic Microwave Background Observables","version":3},"cited_work":{"arxiv_id":"2507.07346","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.07346","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolliet, A","venue":null,"work_id":"71c47557-8346-49f2-afaa-7ebd8ffc86a1","year":2025},"citing_paper":{"arxiv_id":"2511.04733","last_updated":"2026-04-23T09:59:53Z","snapshot_observed_at":"2026-08-04T11:42:42.587585Z","submitted_at":"2025-11-06T19:00:00Z","title":"Combining CMB datasets with consistent foreground modelling","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-18T00:43:15.825063Z"},"links":{"cited_paper":"/paper/2507.07346","citing_paper":"/paper/2511.04733"},"observation_digest":"sha256:409b59ef4743d4710c38ddc879839cdb0bc89b8f69700755e1836e34428c477d","observation_id":"f27e7417-012b-4cbb-ab41-6f54f19ba96c","resolution":{"observed_at":"2026-05-18T00:45:33.150961Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.07346","last_updated":"2025-07-25T13:32:05Z","snapshot_observed_at":"2026-07-06T21:54:48.150241Z","submitted_at":"2025-07-10T00:19:11Z","title":"CLASS_SZ II: Notes and Examples of Fast and Accurate Calculations of Halo Model, Large Scale Structure and Cosmic Microwave Background Observables","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.07346","snapshot_observed_at":"2026-07-13T02:04:26.563148Z","title":"arXiv , author =:2507.07346 , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09571","last_updated":"2026-07-10T16:18:53Z","snapshot_observed_at":"2026-07-29T14:03:34.440737Z","submitted_at":"2026-07-10T16:18:53Z","title":"CHEFT: A Hybrid Effective Field Theory halo model","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-13T02:04:26.563148Z"},"links":{"cited_paper":"/paper/2507.07346","citing_paper":"/paper/2607.09571"},"observation_digest":"sha256:cd41f3d7d85d0a5928ef641b3499fccec1653cb1a3037ca7b86fe081a0154392","observation_id":"11480178-760d-4d72-ab49-c5facfaa7f44","resolution":{"observed_at":"2026-07-13T02:04:26.563148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2507.07346/citation-record","integrity":"/paper/2507.07346/integrity","json":"/paper/2507.07346/citation-record.json","paper":"/paper/2507.07346"},"outbound":[],"paper":{"arxiv_id":"2507.07346","last_updated":"2025-07-25T13:32:05Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T21:54:48.150241Z","submitted_at":"2025-07-10T00:19:11Z","title":"CLASS_SZ II: Notes and Examples of Fast and Accurate Calculations of Halo Model, Large Scale Structure and Cosmic Microwave Background Observables"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2507.07346."}