{"as_of":"2026-08-15T20:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:13bef4b2fdc04cd7af9a53f4dbd5ec4d503a86e684eb89e556c064241b91a944","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":"2026-08-15T06:32:42.880941+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":"2026-08-14T10:44:58.064478Z","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":"2026-08-14T10:44:58.271966Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0808.0341","last_updated":"2008-08-03T19:06:14Z","snapshot_observed_at":"2026-08-15T10:09:37.767662Z","submitted_at":"2008-08-03T19:06:14Z","title":"Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation","version":1},"cited_work":{"arxiv_id":"0808.0341","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.0341","snapshot_observed_at":"2026-08-14T10:44:58.271966Z","title":"Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation","venue":"astro-ph","work_id":"11af2255-ff77-4686-8b39-bfac9dd0a14f","year":2008},"citing_paper":{"arxiv_id":"1908.10637","last_updated":"2020-03-10T16:59:42Z","snapshot_observed_at":"2026-08-15T11:43:39.962433Z","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":14,"source":"pdf_text","source_observed_at":"2026-08-14T10:44:58.064478Z"},"links":{"cited_paper":"/paper/0808.0341","citing_paper":"/paper/1908.10637"},"observation_digest":"sha256:a7810b350dcd44cdbd5fdad99ac3ab6eea927cb2fa2ab0e2108194562af04cb6","observation_id":"882e638c-ad44-492f-96fd-57d34687175c","resolution":{"observed_at":"2026-08-14T10:44:58.276110Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/0808.0341/citation-record","integrity":"/paper/0808.0341/integrity","json":"/paper/0808.0341/citation-record.json","paper":"/paper/0808.0341"},"outbound":[],"paper":{"arxiv_id":"0808.0341","last_updated":"2008-08-03T19:06:14Z","latest_version":1,"primary_category":"astro-ph","snapshot_observed_at":"2026-08-15T10:09:37.767662Z","submitted_at":"2008-08-03T19:06:14Z","title":"Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+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:0808.0341."}