{"as_of":"2026-08-11T13:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:262740b68d9d2914a302d6e9f69757058cdb44da63d1a84f486ea9abd2951c1c","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":"2026-08-11T06:34:44.6726+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":"2026-07-14T07:56:20.592048Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1604.02263","last_updated":"2016-06-28T07:20:22Z","snapshot_observed_at":"2026-07-06T04:52:09.602955Z","submitted_at":"2016-04-08T07:58:20Z","title":"Constraining particle dark matter using local galaxy distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.02263","snapshot_observed_at":"2026-07-14T07:56:20.592048Z","title":"Ando and K","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10974","last_updated":"2026-07-13T00:39:08Z","snapshot_observed_at":"2026-08-07T11:15:57.995251Z","submitted_at":"2026-07-13T00:39:08Z","title":"Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-14T07:56:20.592048Z"},"links":{"cited_paper":"/paper/1604.02263","citing_paper":"/paper/2607.10974"},"observation_digest":"sha256:27cc9f87f5d2ff329d3fa22c3ee43cb4d760ee79d3325aa4bd44f5a93e2721f7","observation_id":"f653fcca-0eb6-44e5-8bfa-1a2727d949a8","resolution":{"observed_at":"2026-07-14T07:56:20.592048Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1604.02263/citation-record","integrity":"/paper/1604.02263/integrity","json":"/paper/1604.02263/citation-record.json","paper":"/paper/1604.02263"},"outbound":[],"paper":{"arxiv_id":"1604.02263","last_updated":"2016-06-28T07:20:22Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-07-06T04:52:09.602955Z","submitted_at":"2016-04-08T07:58:20Z","title":"Constraining particle dark matter using local galaxy distribution"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1604.02263."}