{"as_of":"2026-08-19T03:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6140618b2b14c6d03d328bbf84bde142c1b2723c2921f46daeeb236332638308","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":"2026-08-18T06:34:40.430872+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":"2026-08-16T11:13:14.357346Z","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":"2026-07-03T11:58:06.409405Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2212.05075","last_updated":"2022-12-09T19:00:01Z","snapshot_observed_at":"2026-08-16T16:09:42.125212Z","submitted_at":"2022-12-09T19:00:01Z","title":"Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.05075","snapshot_observed_at":"2026-08-10T19:52:58.518961Z","title":"Present and future constraints on secluded dark matter in the Galactic Halo with TeV Gamma-ray observatories,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.09647","last_updated":"2025-02-17T13:28:31Z","snapshot_observed_at":"2026-08-17T10:54:43.176219Z","submitted_at":"2025-01-16T16:39:19Z","title":"Constraining the Secluded and Catalyzed Annihilation Dark Matter with Fermi-LAT and Planck Data","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T19:52:58.518961Z"},"links":{"cited_paper":"/paper/2212.05075","citing_paper":"/paper/2501.09647"},"observation_digest":"sha256:83e4e73502731082aad32851391334f608962ebe14a2a1cb6cf67e5dfa42c365","observation_id":"b5a6fc5f-9d04-4180-8af8-45e723ff8b6d","resolution":{"observed_at":"2026-08-10T19:52:58.518961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.05075","last_updated":"2022-12-09T19:00:01Z","snapshot_observed_at":"2026-08-16T16:09:42.125212Z","submitted_at":"2022-12-09T19:00:01Z","title":"Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.05075","snapshot_observed_at":"2026-08-16T11:13:14.357346Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.16228","last_updated":"2025-05-08T22:36:23Z","snapshot_observed_at":"2026-08-17T20:26:29.855751Z","submitted_at":"2025-04-22T19:48:02Z","title":"Brazilian Report on Dark Matter 2024","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T11:13:14.357346Z"},"links":{"cited_paper":"/paper/2212.05075","citing_paper":"/paper/2504.16228"},"observation_digest":"sha256:5acea3a10a996370ef0ab0a78d8e2e93860bafc3d3c2a1bbbb5ad69bba3535a0","observation_id":"acd02030-3561-4b4d-890d-00f91c236641","resolution":{"observed_at":"2026-08-16T11:13:14.357346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.05075","last_updated":"2022-12-09T19:00:01Z","snapshot_observed_at":"2026-08-16T16:09:42.125212Z","submitted_at":"2022-12-09T19:00:01Z","title":"Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.05075","snapshot_observed_at":"2026-08-03T21:41:37.480219Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.14635","last_updated":"2026-06-18T19:41:52Z","snapshot_observed_at":"2026-08-18T23:15:14.666537Z","submitted_at":"2025-11-18T16:28:28Z","title":"Probing the Phenomenology of Dark Matter from Decoupled Freeze-Out","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-03T21:41:37.480219Z"},"links":{"cited_paper":"/paper/2212.05075","citing_paper":"/paper/2511.14635"},"observation_digest":"sha256:42f6d7234c946e7e9993739c517aa9a0173cca8f54a9d8e32f954e9c64322ba5","observation_id":"5a6f6715-7e87-4f35-9908-fc22e27ce5ca","resolution":{"observed_at":"2026-08-03T21:41:37.480219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.05075","last_updated":"2022-12-09T19:00:01Z","snapshot_observed_at":"2026-08-16T16:09:42.125212Z","submitted_at":"2022-12-09T19:00:01Z","title":"Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories","version":1},"cited_work":{"arxiv_id":"2212.05075","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.05075","snapshot_observed_at":"2026-07-03T11:58:06.409405Z","title":null,"venue":null,"work_id":"6f3814be-e8a9-400d-ae0b-2cddc11ce1f5","year":2023},"citing_paper":{"arxiv_id":"2604.21976","last_updated":"2026-04-23T18:00:03Z","snapshot_observed_at":"2026-08-11T07:20:17.977553Z","submitted_at":"2026-04-23T18:00:03Z","title":"Cosmic-Ray Signatures of Annihilating and Semi-Annihilating Dark Matter via One-Step Cascades","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-09T20:58:02.150571Z"},"links":{"cited_paper":"/paper/2212.05075","citing_paper":"/paper/2604.21976"},"observation_digest":"sha256:957bd2f6f31c282d12f1e3172c8beee9dd0f04d09adfd7364ed4585746c5a36b","observation_id":"f7097d56-f5ff-49da-a4b3-d0e8397ac56d","resolution":{"observed_at":"2026-05-11T14:51:05.699546Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.05075","last_updated":"2022-12-09T19:00:01Z","snapshot_observed_at":"2026-08-16T16:09:42.125212Z","submitted_at":"2022-12-09T19:00:01Z","title":"Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories","version":1},"cited_work":{"arxiv_id":"2212.05075","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.05075","snapshot_observed_at":"2026-07-03T11:58:06.409405Z","title":null,"venue":null,"work_id":"6f3814be-e8a9-400d-ae0b-2cddc11ce1f5","year":2023},"citing_paper":{"arxiv_id":"2606.11936","last_updated":"2026-06-10T11:08:17Z","snapshot_observed_at":"2026-08-02T03:41:45.576044Z","submitted_at":"2026-06-10T11:08:17Z","title":"Heavy singlet fermionic dark matter with $Z_4$ symmetry","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-27T09:13:48.981590Z"},"links":{"cited_paper":"/paper/2212.05075","citing_paper":"/paper/2606.11936"},"observation_digest":"sha256:7cc14f84a5d4814470f1841a186963402dfe1bd994bc0a52857d0fd28cc87f50","observation_id":"4410a17d-e5ca-4a35-98fc-7a25254a76dc","resolution":{"observed_at":"2026-07-03T11:58:06.410791Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2212.05075/citation-record","integrity":"/paper/2212.05075/integrity","json":"/paper/2212.05075/citation-record.json","paper":"/paper/2212.05075"},"outbound":[],"paper":{"arxiv_id":"2212.05075","last_updated":"2022-12-09T19:00:01Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-16T16:09:42.125212Z","submitted_at":"2022-12-09T19:00:01Z","title":"Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2212.05075."}