{"as_of":"2026-08-11T09:39:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fdf5491712d6cd09476a9ce8f2b3dac251f1a675725c22ccbe3dd0879b4bfdcf","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T21:28:32.196130Z","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":"2026-05-11T06:30:59.796005Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1912.09904","last_updated":"2020-11-04T03:36:33Z","snapshot_observed_at":"2026-08-10T00:53:03.331159Z","submitted_at":"2019-12-20T16:06:41Z","title":"Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.09904","snapshot_observed_at":"2026-08-10T21:28:32.196130Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.07591","last_updated":"2025-01-20T13:06:07Z","snapshot_observed_at":"2026-08-10T21:11:00.824749Z","submitted_at":"2025-01-09T14:30:06Z","title":"Probing Supernova Neutrino Boosted Dark Matter with Collective Excitation","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T21:28:32.196130Z"},"links":{"cited_paper":"/paper/1912.09904","citing_paper":"/paper/2501.07591"},"observation_digest":"sha256:438c7452a89c1cc7b779da979805795f1fadedf2272864f5fee8ef98249456fe","observation_id":"1cca002f-9d69-444e-a62d-c8da8603005f","resolution":{"observed_at":"2026-08-10T21:28:32.196130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.09904","last_updated":"2020-11-04T03:36:33Z","snapshot_observed_at":"2026-08-10T00:53:03.331159Z","submitted_at":"2019-12-20T16:06:41Z","title":"Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.09904","snapshot_observed_at":"2026-08-04T08:57:10.487225Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.18338","last_updated":"2026-06-29T09:20:06Z","snapshot_observed_at":"2026-08-07T10:08:47.110506Z","submitted_at":"2025-10-21T06:44:48Z","title":"Direct Detection of Leptophobic Dark Matter with Electronic Collective Excitations","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-04T08:57:10.487225Z"},"links":{"cited_paper":"/paper/1912.09904","citing_paper":"/paper/2510.18338"},"observation_digest":"sha256:6c5745b000587cbdefef3dcfdacc46b6ffd755417b254ef58fcd7a2c233e65b4","observation_id":"085e26f9-bce6-49ce-af76-85fe6d5bb34c","resolution":{"observed_at":"2026-08-04T08:57:10.487225Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.09904","last_updated":"2020-11-04T03:36:33Z","snapshot_observed_at":"2026-08-10T00:53:03.331159Z","submitted_at":"2019-12-20T16:06:41Z","title":"Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection","version":2},"cited_work":{"arxiv_id":"1912.09904","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.09904","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cosmic ray boosted sub-GeV gravita- tionally interacting dark matter in direct detection","venue":null,"work_id":"8717bc21-5519-4101-91e4-f1d54a71c12a","year":2020},"citing_paper":{"arxiv_id":"2604.06929","last_updated":"2026-04-16T08:22:39Z","snapshot_observed_at":"2026-08-11T09:26:26.680444Z","submitted_at":"2026-04-08T10:41:40Z","title":"Direct-detection constraints on inelastic dark matter with a scalar mediator","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-10T17:36:54.459136Z"},"links":{"cited_paper":"/paper/1912.09904","citing_paper":"/paper/2604.06929"},"observation_digest":"sha256:7f924f104d9aaea0b064418e47c0e9f681eb0f67619a2158b8b2ae7445302c49","observation_id":"c103d339-5e03-4dde-a084-60684a3e1523","resolution":{"observed_at":"2026-05-11T06:30:59.800995Z","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":"1912.09904","last_updated":"2020-11-04T03:36:33Z","snapshot_observed_at":"2026-08-10T00:53:03.331159Z","submitted_at":"2019-12-20T16:06:41Z","title":"Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection","version":2},"cited_work":{"arxiv_id":"1912.09904","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.09904","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cosmic ray boosted sub-GeV gravita- tionally interacting dark matter in direct detection","venue":null,"work_id":"8717bc21-5519-4101-91e4-f1d54a71c12a","year":2020},"citing_paper":{"arxiv_id":"2604.17869","last_updated":"2026-04-20T06:30:15Z","snapshot_observed_at":"2026-07-06T23:04:50.935335Z","submitted_at":"2026-04-20T06:30:15Z","title":"Probing Cosmic-Ray-Boosted and Supernova-Sourced Sub-GeV Dark Matter with Paleo-Detectors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-10T04:51:01.292668Z"},"links":{"cited_paper":"/paper/1912.09904","citing_paper":"/paper/2604.17869"},"observation_digest":"sha256:2ab4370158e207a674b6f82b3c98fe1654caf77519a9dca315e1edd56af64d93","observation_id":"184f26c9-7a90-4a32-8847-9ae9f9ab6d98","resolution":{"observed_at":"2026-05-10T11:30:19.762719Z","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":"1912.09904","last_updated":"2020-11-04T03:36:33Z","snapshot_observed_at":"2026-08-10T00:53:03.331159Z","submitted_at":"2019-12-20T16:06:41Z","title":"Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.09904","snapshot_observed_at":"2026-08-02T00:17:55.075136Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.15098","last_updated":"2026-07-22T07:30:05Z","snapshot_observed_at":"2026-08-09T02:06:10.678309Z","submitted_at":"2026-07-16T15:10:08Z","title":"Inelastic Scattering Effects on Attenuation of Boosted Dark Matter","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-02T00:17:55.075136Z"},"links":{"cited_paper":"/paper/1912.09904","citing_paper":"/paper/2607.15098"},"observation_digest":"sha256:3fa526446bba179fff64ce940278d19a39b2acbf7575837901da967e91e9a041","observation_id":"cf0c0e66-fac6-4b9b-80a1-816956970d41","resolution":{"observed_at":"2026-08-02T00:17:55.075136Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1912.09904/citation-record","integrity":"/paper/1912.09904/integrity","json":"/paper/1912.09904/citation-record.json","paper":"/paper/1912.09904"},"outbound":[],"paper":{"arxiv_id":"1912.09904","last_updated":"2020-11-04T03:36:33Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-10T00:53:03.331159Z","submitted_at":"2019-12-20T16:06:41Z","title":"Cosmic Ray Boosted Sub-GeV Gravitationally Interacting Dark Matter in Direct Detection"},"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 5 inbound Pith citation observations for arXiv:1912.09904."}