{"as_of":"2026-08-09T14:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9aaf86e91def987b2b65335a1bc829e4e13cca6d1c710b1320a450ca045dcf68","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T11:42:10.541573Z","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":"2026-05-15T01:48:28.383796Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1811.11241","last_updated":"2019-10-16T20:22:07Z","snapshot_observed_at":"2026-08-04T15:59:28.652221Z","submitted_at":"2018-11-27T20:26:11Z","title":"Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.11241","snapshot_observed_at":"2026-08-05T11:42:10.541573Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02325","last_updated":"2025-09-02T13:51:14Z","snapshot_observed_at":"2026-08-09T03:07:09.723512Z","submitted_at":"2025-09-02T13:51:14Z","title":"Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-05T11:42:10.541573Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2509.02325"},"observation_digest":"sha256:d12bb1dbff487ea6ed93d0968e4733bd518d810681c304295d2cad340f47cb24","observation_id":"2ed877f7-dab5-4f73-8209-b744115164c9","resolution":{"observed_at":"2026-08-05T11:42:10.541573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.11241","last_updated":"2019-10-16T20:22:07Z","snapshot_observed_at":"2026-08-04T15:59:28.652221Z","submitted_at":"2018-11-27T20:26:11Z","title":"Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data","version":3},"cited_work":{"arxiv_id":"1811.11241","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1811.11241","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"cd4b7b17-0510-464e-95c5-eda2f5a5cb54","year":2019},"citing_paper":{"arxiv_id":"2605.14447","last_updated":"2026-05-14T06:41:34Z","snapshot_observed_at":"2026-07-06T23:25:54.070869Z","submitted_at":"2026-05-14T06:41:34Z","title":"Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-05-15T01:47:28.438537Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2605.14447"},"observation_digest":"sha256:ccd75688dbdebf6594adfaeeedec4cf74fbf9f9480d30634fa6607f743af78b6","observation_id":"093dbb55-233f-4eb7-bbf0-45f2f8b84a33","resolution":{"observed_at":"2026-05-15T01:48:28.385455Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.11241","last_updated":"2019-10-16T20:22:07Z","snapshot_observed_at":"2026-08-04T15:59:28.652221Z","submitted_at":"2018-11-27T20:26:11Z","title":"Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.11241","snapshot_observed_at":"2026-07-14T09:47:34.937735Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10716","last_updated":"2026-07-27T03:25:36Z","snapshot_observed_at":"2026-08-06T08:31:12.447959Z","submitted_at":"2026-07-12T11:16:41Z","title":"Migdal Ionization as a Probe of Light Dark Matter from Nuclear Transition","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-14T09:47:34.937735Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2607.10716"},"observation_digest":"sha256:365cad0aea34f12a7bf0cbc1c8f095a7e056aaec7f88a3b6efeac951fbac730d","observation_id":"6be6e1c6-9c78-43e9-b07c-dfbdf118f52d","resolution":{"observed_at":"2026-07-14T09:47:34.937735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.11241","last_updated":"2019-10-16T20:22:07Z","snapshot_observed_at":"2026-08-04T15:59:28.652221Z","submitted_at":"2018-11-27T20:26:11Z","title":"Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.11241","snapshot_observed_at":"2026-08-02T07:18:12.834975Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10716","last_updated":"2026-07-27T03:25:36Z","snapshot_observed_at":"2026-08-06T08:31:12.447959Z","submitted_at":"2026-07-12T11:16:41Z","title":"Migdal Ionization as a Probe of Light Dark Matter from Nuclear Transition","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-02T07:18:12.834975Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2607.10716"},"observation_digest":"sha256:15a899607af67f20f3c5daaacd5f22713af899d522a1de7d5c601ba7eee0bae3","observation_id":"3dc9b40e-eb4a-475a-9a52-fac1e7a5656b","resolution":{"observed_at":"2026-08-02T07:18:12.834975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1811.11241/citation-record","integrity":"/paper/1811.11241/integrity","json":"/paper/1811.11241/citation-record.json","paper":"/paper/1811.11241"},"outbound":[],"paper":{"arxiv_id":"1811.11241","last_updated":"2019-10-16T20:22:07Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T15:59:28.652221Z","submitted_at":"2018-11-27T20:26:11Z","title":"Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1811.11241."}