{"as_of":"2026-08-08T12:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ac8cd06d455f767aa2cd0c4bb31d87a6a52d084362b2789c145f58e272f52755","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":"2026-08-08T06:32:00.761636+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":"2026-08-07T13:28:11.940951Z","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":"1405.7943","last_updated":"2016-04-08T01:18:13Z","snapshot_observed_at":"2026-07-06T03:45:07.524590Z","submitted_at":"2014-05-30T18:21:51Z","title":"Questioning a 3.5 keV dark matter emission line","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.7943","snapshot_observed_at":"2026-08-07T13:28:11.940951Z","title":"Riemer-Sørensen, Astron","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.22463","last_updated":"2025-11-07T22:51:03Z","snapshot_observed_at":"2026-08-07T22:17:53.654097Z","submitted_at":"2025-05-28T15:17:25Z","title":"Opening up New Parameter Space for Sterile Neutrino Dark Matter","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T13:28:11.940951Z"},"links":{"cited_paper":"/paper/1405.7943","citing_paper":"/paper/2505.22463"},"observation_digest":"sha256:decffce51ca511136e15066403d501f604e6c1ecc3287c2c1c3950467ad67c6b","observation_id":"9c1fde00-1699-4689-8d3d-c3d97c3c0539","resolution":{"observed_at":"2026-08-07T13:28:11.940951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1405.7943/citation-record","integrity":"/paper/1405.7943/integrity","json":"/paper/1405.7943/citation-record.json","paper":"/paper/1405.7943"},"outbound":[],"paper":{"arxiv_id":"1405.7943","last_updated":"2016-04-08T01:18:13Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T03:45:07.524590Z","submitted_at":"2014-05-30T18:21:51Z","title":"Questioning a 3.5 keV dark matter emission line"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1405.7943."}