{"as_of":"2026-08-11T07:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e7262d99694152cb1c8263b9f39df7d7343e112e7bd1a3383a0dd3863b298ded","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":"2026-08-11T06:34:44.6726+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":"2026-07-13T05:17:12.889672Z","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":"2026-05-22T22:47:13.431678Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1902.00929","last_updated":"2019-10-10T04:50:43Z","snapshot_observed_at":"2026-07-06T07:30:50.190635Z","submitted_at":"2019-02-03T17:09:19Z","title":"GW170817 constraints on the properties of a neutron star in the presence of WIMP dark matter","version":2},"cited_work":{"arxiv_id":"1902.00929","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.00929","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Quddus, G","venue":null,"work_id":"e5f7e25c-a924-445c-b0dc-ae9b4ac3eebc","year":2020},"citing_paper":{"arxiv_id":"2503.19691","last_updated":"2026-03-04T15:53:07Z","snapshot_observed_at":"2026-07-06T20:58:27.929311Z","submitted_at":"2025-03-25T14:18:06Z","title":"Strongly Interacting Dark Matter admixed Neutron Stars","version":4},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-22T22:45:48.648963Z"},"links":{"cited_paper":"/paper/1902.00929","citing_paper":"/paper/2503.19691"},"observation_digest":"sha256:59a00d3bc507012bea5a7f69a901886cff8eed2c98023a64e913bb153a3b83f7","observation_id":"9f35da39-0cf8-44bd-b78e-f29edd0d1474","resolution":{"observed_at":"2026-05-22T22:47:13.434579Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.00929","last_updated":"2019-10-10T04:50:43Z","snapshot_observed_at":"2026-07-06T07:30:50.190635Z","submitted_at":"2019-02-03T17:09:19Z","title":"GW170817 constraints on the properties of a neutron star in the presence of WIMP dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.00929","snapshot_observed_at":"2026-07-13T05:17:12.889672Z","title":"Quddus, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.09119","last_updated":"2026-07-10T06:16:49Z","snapshot_observed_at":"2026-08-08T02:18:59.676855Z","submitted_at":"2026-07-10T06:16:49Z","title":"Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-13T05:17:12.889672Z"},"links":{"cited_paper":"/paper/1902.00929","citing_paper":"/paper/2607.09119"},"observation_digest":"sha256:c2a36aed361c36336e8d4a98a11b655afe2a83b7beac86160722afa96c5d71dd","observation_id":"3cb86441-aa85-4a19-9bb7-ccaf18aed213","resolution":{"observed_at":"2026-07-13T05:17:12.889672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1902.00929/citation-record","integrity":"/paper/1902.00929/integrity","json":"/paper/1902.00929/citation-record.json","paper":"/paper/1902.00929"},"outbound":[],"paper":{"arxiv_id":"1902.00929","last_updated":"2019-10-10T04:50:43Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T07:30:50.190635Z","submitted_at":"2019-02-03T17:09:19Z","title":"GW170817 constraints on the properties of a neutron star in the presence of WIMP dark matter"},"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 2 inbound Pith citation observations for arXiv:1902.00929."}