{"as_of":"2026-08-23T17:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:87bc123e2f32c93251b5a56d1742192bd3ad3f2659490223605d87957e974a8c","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T18:47:19.760602Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-14T14:17:59.250081Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03479","last_updated":"2019-12-18T10:05:05Z","snapshot_observed_at":"2026-08-16T23:54:52.416120Z","submitted_at":"2019-08-09T14:43:25Z","title":"First direct detection constraint on mirror dark matter kinetic mixing using LUX 2013 data","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T14:17:59.250081Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/1908.03479"},"observation_digest":"sha256:5e5d03b31a28bdb9a1410dc66d83c7c502a02864fb87814e84184c6941db647b","observation_id":"65854f18-f565-45e3-ab77-9a0ca5e7b95d","resolution":{"observed_at":"2026-08-14T14:17:59.250081Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-14T10:51:09.694645Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.10369","last_updated":"2020-03-03T19:17:40Z","snapshot_observed_at":"2026-08-15T10:41:56.295777Z","submitted_at":"2019-08-27T18:00:01Z","title":"Constraining Nonthermal Dark Matter's Impact on the Matter Power Spectrum","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T10:51:09.694645Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/1908.10369"},"observation_digest":"sha256:9f003cc75af34d3774da5ee88d45c15b44e8f47ec6d832ca2c6bf934f906d4de","observation_id":"d2e05e89-318b-4382-a5b3-d1dc08f29a49","resolution":{"observed_at":"2026-08-14T10:51:09.694645Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-14T10:38:40.628414Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.10881","last_updated":"2020-02-03T09:14:30Z","snapshot_observed_at":"2026-08-14T23:47:50.343446Z","submitted_at":"2019-08-28T18:00:11Z","title":"On the relation between Migdal effect and dark matter-electron scattering in isolated atoms and semiconductors","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T10:38:40.628414Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/1908.10881"},"observation_digest":"sha256:a75f76d5ad7d35d04aac60c10f913001bb87d36549d91b0a7b9412b5d3d1d153","observation_id":"cd637bf7-433e-4522-a155-de3d55e40c90","resolution":{"observed_at":"2026-08-14T10:38:40.628414Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-12T05:53:38.321562Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.19836","last_updated":"2025-03-19T19:09:40Z","snapshot_observed_at":"2026-08-18T11:19:59.415809Z","submitted_at":"2024-11-29T16:47:02Z","title":"Searching for MeV-mass neutrinophilic Dark Matter with Large Scale Dark Matter Detectors","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T05:53:38.321562Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2411.19836"},"observation_digest":"sha256:470163db866d90150727e2abc2121c60a4ece4d90479e64c89ab10689a289bee","observation_id":"c176bd9f-d922-44be-a9b6-6d15e8b98271","resolution":{"observed_at":"2026-08-12T05:53:38.321562Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-11T10:50:17.680635Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.16283","last_updated":"2024-12-20T19:00:00Z","snapshot_observed_at":"2026-08-17T11:54:25.175273Z","submitted_at":"2024-12-20T19:00:00Z","title":"Dark Matter-Electron Detectors for Dark Matter-Nucleon Interactions","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T10:50:17.680635Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2412.16283"},"observation_digest":"sha256:13237e52676314b33802e94adbb6384ed20191d5fd39b05e2aa596d1c0e5577f","observation_id":"919aea08-dcd7-4751-9b43-4eb97e2b3803","resolution":{"observed_at":"2026-08-11T10:50:17.680635Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-15T18:47:19.760602Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.18982","last_updated":"2026-07-01T15:46:40Z","snapshot_observed_at":"2026-08-20T00:51:51.558741Z","submitted_at":"2025-06-23T18:00:03Z","title":"First direct search for light dark matter interactions in a transition-edge sensor","version":4},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-15T18:47:19.760602Z"},"links":{"cited_paper":"/paper/1811.11241","citing_paper":"/paper/2506.18982"},"observation_digest":"sha256:4ba8c36f444678b3a838ff9149ded5995aa40ed3ccdbf8b101fbf41141bfdd89","observation_id":"dc132802-7d4c-425d-a7f4-99ab77a051d2","resolution":{"observed_at":"2026-08-15T18:47:19.760602Z","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-17T09:51:36.511349Z","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:ef49904389b97ef27bc86c9d7d482234c01b3e275575c73eaa050c4f2d1ca24b","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":"2026-08-15T11:16:44.013323Z","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:b7091ab65521eec98c1c3478593d1b691cefe012fd40c1dc3305f03103d36dd7","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 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.11241","last_updated":"2019-10-16T20:22:07Z","snapshot_observed_at":"2026-08-15T11:16:44.013323Z","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":"2026-08-16T10:04:42.032561Z","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":"sha256:45aa6df2f14d782ed767a96a61e07ff21f04f0cc451f54b662e35dafc0c48746","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-16T10:04:42.032561Z","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:c1e362a3bba75f7d3713d21927212a29dddf1b17ad9ac322e737b6e7d5e5c82d","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":"2026-08-15T11:16:44.013323Z","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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1811.11241."}