{"as_of":"2026-08-13T13:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:27de1bd9c03590e8c82e3029a026c1b152e985febf5abd06c861cecdc59f8bdf","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":"2026-08-13T06:32:02.005865+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":"2026-08-12T14:34:19.917670Z","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":"2026-05-19T10:22:14.408009Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.24026","last_updated":"2025-03-18T14:18:21Z","snapshot_observed_at":"2026-08-12T22:10:36.837645Z","submitted_at":"2024-10-31T15:27:08Z","title":"Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.24026","snapshot_observed_at":"2026-08-12T14:34:19.917670Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.15307","last_updated":"2025-03-13T08:10:48Z","snapshot_observed_at":"2026-08-12T14:24:10.998285Z","submitted_at":"2024-11-22T19:00:44Z","title":"A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-12T14:34:19.917670Z"},"links":{"cited_paper":"/paper/2410.24026","citing_paper":"/paper/2411.15307"},"observation_digest":"sha256:4dae8f5aacac9e1776fe65342d6c6f6ce4ab056d83eb95c8f434784014781dc6","observation_id":"e4339c86-7f25-45f1-b10f-39cae0b29358","resolution":{"observed_at":"2026-08-12T14:34:19.917670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.24026","last_updated":"2025-03-18T14:18:21Z","snapshot_observed_at":"2026-08-12T22:10:36.837645Z","submitted_at":"2024-10-31T15:27:08Z","title":"Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?","version":2},"cited_work":{"arxiv_id":"2410.24026","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.24026","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Toscano, F","venue":null,"work_id":"ac7328f7-ae38-48e9-9b56-591fd849625e","year":2025},"citing_paper":{"arxiv_id":"2506.08833","last_updated":"2026-04-16T15:05:13Z","snapshot_observed_at":"2026-08-11T09:59:29.940526Z","submitted_at":"2025-06-10T14:20:53Z","title":"Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-19T10:19:52.764412Z"},"links":{"cited_paper":"/paper/2410.24026","citing_paper":"/paper/2506.08833"},"observation_digest":"sha256:9d620c4e0a14d860ac714f8b65df38dd03f8b77b22c9cca0afb9da0133ce905c","observation_id":"8d1bfe83-c553-492b-94f9-825c2d897268","resolution":{"observed_at":"2026-05-19T10:22:14.409589Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2410.24026/citation-record","integrity":"/paper/2410.24026/integrity","json":"/paper/2410.24026/citation-record.json","paper":"/paper/2410.24026"},"outbound":[],"paper":{"arxiv_id":"2410.24026","last_updated":"2025-03-18T14:18:21Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-12T22:10:36.837645Z","submitted_at":"2024-10-31T15:27:08Z","title":"Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.24026."}