{"as_of":"2026-08-07T23:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a9651bdeaa8dc4673ea48484fb6d101098163e42e16f2b90897a2bf04be34915","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T19:18:36.269461Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-02T00:06:25.001990Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2301.03625","last_updated":"2023-04-07T14:26:16Z","snapshot_observed_at":"2026-08-05T06:25:05.310427Z","submitted_at":"2023-01-09T19:00:14Z","title":"Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03625","snapshot_observed_at":"2026-08-06T19:18:36.269461Z","title":"Celestial objects as strongly-interacting nonannihilating dark matter detectors,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-07T14:17:55.403871Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.269461Z"},"links":{"cited_paper":"/paper/2301.03625","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:6c461e9d226ef589ac3150b2856f437b306b651e42c23530030a07788cdae044","observation_id":"955a4740-43b4-446f-adc0-f14dc372435c","resolution":{"observed_at":"2026-08-06T19:18:36.269461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03625","last_updated":"2023-04-07T14:26:16Z","snapshot_observed_at":"2026-08-05T06:25:05.310427Z","submitted_at":"2023-01-09T19:00:14Z","title":"Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors","version":2},"cited_work":{"arxiv_id":"2301.03625","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.03625","snapshot_observed_at":"2026-07-02T00:06:25.001990Z","title":"Ray, Celestial objects as strongly-interacting nonannihilating dark matter detectors, Phys","venue":null,"work_id":"5646ac5b-c4ac-4306-b0bd-dfb9dad608c9","year":2023},"citing_paper":{"arxiv_id":"2507.15951","last_updated":"2026-04-23T11:30:08Z","snapshot_observed_at":"2026-07-06T22:00:38.257294Z","submitted_at":"2025-07-21T18:00:07Z","title":"Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-19T03:44:07.472458Z"},"links":{"cited_paper":"/paper/2301.03625","citing_paper":"/paper/2507.15951"},"observation_digest":"sha256:e534a7abeb97c16a708df7bc79b2fefe5a12a5acca299a04ae183b0793273d3e","observation_id":"35df84b0-3971-4735-9377-6cccd9c6d066","resolution":{"observed_at":"2026-05-19T03:47:02.009744Z","resolver_source":"arxiv_id","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":"2301.03625","last_updated":"2023-04-07T14:26:16Z","snapshot_observed_at":"2026-08-05T06:25:05.310427Z","submitted_at":"2023-01-09T19:00:14Z","title":"Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors","version":2},"cited_work":{"arxiv_id":"2301.03625","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.03625","snapshot_observed_at":"2026-07-02T00:06:25.001990Z","title":"Ray, Celestial objects as strongly-interacting nonannihilating dark matter detectors, Phys","venue":null,"work_id":"5646ac5b-c4ac-4306-b0bd-dfb9dad608c9","year":2023},"citing_paper":{"arxiv_id":"2606.02579","last_updated":"2026-06-01T17:59:49Z","snapshot_observed_at":"2026-08-04T20:20:01.350709Z","submitted_at":"2026-06-01T17:59:49Z","title":"New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-06-28T13:34:28.381901Z"},"links":{"cited_paper":"/paper/2301.03625","citing_paper":"/paper/2606.02579"},"observation_digest":"sha256:4648d95571e55b516bde8a203ddbb10d167ea321f5f821368b74d7da25ceda6a","observation_id":"615d675e-6a83-4fb4-8726-30bbe02cfd93","resolution":{"observed_at":"2026-07-02T00:06:25.004177Z","resolver_source":"arxiv_id","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"}}],"links":{"evidence":"/evidence","html":"/paper/2301.03625/citation-record","integrity":"/paper/2301.03625/integrity","json":"/paper/2301.03625/citation-record.json","paper":"/paper/2301.03625"},"outbound":[],"paper":{"arxiv_id":"2301.03625","last_updated":"2023-04-07T14:26:16Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-05T06:25:05.310427Z","submitted_at":"2023-01-09T19:00:14Z","title":"Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors"},"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 3 inbound Pith citation observations for arXiv:2301.03625."}