{"as_of":"2026-08-15T06:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f7f43e0216b26fede8fc9e6cc6d0b1701583942156f6deca1fb506d59773d416","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T10:44:58.080052Z","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":"2026-08-14T10:44:58.216699Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1002.0148","last_updated":"2010-09-02T11:28:03Z","snapshot_observed_at":"2026-08-15T05:27:43.940986Z","submitted_at":"2010-01-31T19:21:10Z","title":"Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?","version":6},"cited_work":{"arxiv_id":"1002.0148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1002.0148","snapshot_observed_at":"2026-08-14T10:44:58.216699Z","title":"Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?","venue":"astro-ph.CO","work_id":"64d28b82-d1c5-4e16-93f5-4e53945c822a","year":2010},"citing_paper":{"arxiv_id":"1908.10637","last_updated":"2020-03-10T16:59:42Z","snapshot_observed_at":"2026-08-14T20:11:58.871595Z","submitted_at":"2019-08-28T10:57:36Z","title":"Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane?","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T10:44:58.080052Z"},"links":{"cited_paper":"/paper/1002.0148","citing_paper":"/paper/1908.10637"},"observation_digest":"sha256:556b88827a2c3a2102cd7f018dde273147fcac5e074d9fd2a9fe5cd999b1cde6","observation_id":"8a000b0d-afd7-408b-9fb7-9feef9922182","resolution":{"observed_at":"2026-08-14T10:44:58.221096Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1002.0148/citation-record","integrity":"/paper/1002.0148/integrity","json":"/paper/1002.0148/citation-record.json","paper":"/paper/1002.0148"},"outbound":[],"paper":{"arxiv_id":"1002.0148","last_updated":"2010-09-02T11:28:03Z","latest_version":6,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T05:27:43.940986Z","submitted_at":"2010-01-31T19:21:10Z","title":"Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1002.0148."}