{"as_of":"2026-08-07T10:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:35602e0abf49a2cd08c2c9b26c426359aa90dc83ddd3e4e7ed47bd28467ec915","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":"2026-08-07T06:34:17.273281+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":"2026-08-02T13:38:45.134746Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":48,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1506.08195","last_updated":"2015-06-26T20:00:19Z","snapshot_observed_at":"2026-07-06T04:22:09.595375Z","submitted_at":"2015-06-26T20:00:19Z","title":"PeV Neutrinos and a 3.5 keV X-Ray Line from a PeV Scale Supersymmetric Neutrino Sector","version":1},"cited_work":{"arxiv_id":"1506.08195","doi":"10.1103/physrevd.92.095018","metadata_source":"pith","pith_arxiv_id":"1506.08195","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"PeV Neutrinos and a 3.5 keV X-Ray Line from a PeV Scale Supersymmetric Neutrino Sector","venue":"hep-ph","work_id":"77a42566-fd04-4dce-97d8-3e4ed7a7633b","year":2015},"citing_paper":{"arxiv_id":"2605.20117","last_updated":"2026-07-22T09:30:05Z","snapshot_observed_at":"2026-08-02T13:38:32.767606Z","submitted_at":"2026-05-19T17:05:28Z","title":"The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1506.08195","citing_paper":"/paper/2605.20117"},"observation_digest":"sha256:d01111c3e9f13ad9d29cbc1ba877c4049b946b66c66da3bc858dd8c38b870692","observation_id":"5f2695fd-f040-4b37-840a-ce0fa963f864","resolution":{"observed_at":"2026-05-20T03:43:01.770240Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.08195","last_updated":"2015-06-26T20:00:19Z","snapshot_observed_at":"2026-07-06T04:22:09.595375Z","submitted_at":"2015-06-26T20:00:19Z","title":"PeV Neutrinos and a 3.5 keV X-Ray Line from a PeV Scale Supersymmetric Neutrino Sector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.08195","snapshot_observed_at":"2026-08-02T13:38:45.134746Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2605.20117","last_updated":"2026-07-22T09:30:05Z","snapshot_observed_at":"2026-08-02T13:38:32.767606Z","submitted_at":"2026-05-19T17:05:28Z","title":"The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-02T13:38:45.134746Z"},"links":{"cited_paper":"/paper/1506.08195","citing_paper":"/paper/2605.20117"},"observation_digest":"sha256:3fe030318ed367323351468a2a3375becb89644f06a1b410023cd1ebb09c9d3b","observation_id":"e2434240-7640-4d02-ab86-f4395e96b329","resolution":{"observed_at":"2026-08-02T13:38:45.134746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1506.08195/citation-record","integrity":"/paper/1506.08195/integrity","json":"/paper/1506.08195/citation-record.json","paper":"/paper/1506.08195"},"outbound":[],"paper":{"arxiv_id":"1506.08195","last_updated":"2015-06-26T20:00:19Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-07-06T04:22:09.595375Z","submitted_at":"2015-06-26T20:00:19Z","title":"PeV Neutrinos and a 3.5 keV X-Ray Line from a PeV Scale Supersymmetric Neutrino Sector"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1506.08195."}