{"as_of":"2026-08-10T06:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ba4b1b261082c75a0d81cee5ff19e38f0fd5e19abab83b635316d2295d8be357","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T19:51:26.342186Z","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":"2026-07-04T11:39:46.736220Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":"2405.12004","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-07-04T11:39:46.736220Z","title":null,"venue":null,"work_id":"09a30f80-cc38-4ed0-8b0c-b8d42cba7b23","year":2025},"citing_paper":{"arxiv_id":"2405.17409","last_updated":"2026-05-09T09:22:47Z","snapshot_observed_at":"2026-08-02T20:53:14.388644Z","submitted_at":"2024-05-27T17:56:51Z","title":"Ultraheavy Ultrahigh-Energy Cosmic Rays","version":3},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-05-24T00:42:49.655371Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2405.17409"},"observation_digest":"sha256:49e7098312aed12a01460572be9fdb8de4bcc63d57cefaf4d540af83a69840f5","observation_id":"bdf2b9a6-0051-48bb-ae2e-e5e9c831257c","resolution":{"observed_at":"2026-05-24T00:43:40.261577Z","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":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-08-06T19:51:26.342186Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.04588","last_updated":"2025-07-07T00:45:57Z","snapshot_observed_at":"2026-08-08T16:59:19.390379Z","submitted_at":"2025-07-07T00:45:57Z","title":"The Global Cosmic Ray Observatory -- Challenging next-generation multi-messenger astronomy with interdisciplinary research","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T19:51:26.342186Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2507.04588"},"observation_digest":"sha256:4645d5ac2e676db176c805e095fabf35fffd536cc2bb137b21be353909c0a535","observation_id":"daaf95dd-ac8a-4247-a655-4c2eff09c000","resolution":{"observed_at":"2026-08-06T19:51:26.342186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":"2405.12004","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-07-04T11:39:46.736220Z","title":null,"venue":null,"work_id":"09a30f80-cc38-4ed0-8b0c-b8d42cba7b23","year":2025},"citing_paper":{"arxiv_id":"2511.08153","last_updated":"2026-04-27T19:21:05Z","snapshot_observed_at":"2026-08-03T04:09:34.415981Z","submitted_at":"2025-11-11T12:05:29Z","title":"Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-17T23:53:01.784343Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2511.08153"},"observation_digest":"sha256:69b6359bbfc6463cf758feb684a13bf457b175c191e975b6f1903abe200f92e5","observation_id":"685808a0-6f39-4659-a38a-10a087fe0d7d","resolution":{"observed_at":"2026-05-17T23:55:31.191149Z","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":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":"2405.12004","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-07-04T11:39:46.736220Z","title":null,"venue":null,"work_id":"09a30f80-cc38-4ed0-8b0c-b8d42cba7b23","year":2025},"citing_paper":{"arxiv_id":"2606.11299","last_updated":"2026-06-09T18:00:02Z","snapshot_observed_at":"2026-08-05T19:03:12.115770Z","submitted_at":"2026-06-09T18:00:02Z","title":"A magnetar formation in binary neutron star merger","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:c7a4fe4b792b686e6fd8e923269d50fc2e5ec944115b99952f23b2582b42a8ac","observation_id":"d75ccc90-b0f3-4cd2-af70-5c8480d45314","resolution":{"observed_at":"2026-07-03T07:37:45.132135Z","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":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":"2405.12004","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-07-04T11:39:46.736220Z","title":null,"venue":null,"work_id":"09a30f80-cc38-4ed0-8b0c-b8d42cba7b23","year":2025},"citing_paper":{"arxiv_id":"2606.23812","last_updated":"2026-06-22T18:01:01Z","snapshot_observed_at":"2026-08-07T14:00:53.935104Z","submitted_at":"2026-06-22T18:01:01Z","title":"Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-26T07:51:26.064246Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2606.23812"},"observation_digest":"sha256:e655d66ded8c9455f256c4a8b79ae9102b7b9b1d76abbc3c5f943eac6f79321f","observation_id":"b5b0684c-1379-4f15-a27d-9597e9347050","resolution":{"observed_at":"2026-07-04T11:39:46.737765Z","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":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-08-01T07:48:49.867444Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.21385","last_updated":"2026-07-23T14:47:21Z","snapshot_observed_at":"2026-08-09T00:40:45.205954Z","submitted_at":"2026-07-23T14:47:21Z","title":"Ultra-High-Energy Particle Production in Binary Mergers Endowed with Magnetic Fields","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-01T07:48:49.867444Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2607.21385"},"observation_digest":"sha256:1cf6acc7fac7594410f61114a7ad81d74304b77b8a47fcc995001ba1eb133fa1","observation_id":"4ee005d9-d533-47ee-8a33-a886b8a71de6","resolution":{"observed_at":"2026-08-01T07:48:49.867444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12004","last_updated":"2025-02-13T18:44:27Z","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12004","snapshot_observed_at":"2026-08-01T05:12:26.591580Z","title":"Binary Neutron Star Mergers as the Source of the Highest Energy Cosmic Rays,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.22323","last_updated":"2026-07-24T14:03:07Z","snapshot_observed_at":"2026-08-06T12:43:08.037493Z","submitted_at":"2026-07-24T14:03:07Z","title":"Proton-air interaction properties at $\\sqrt{s} \\simeq 100$ TeV from shower-depth measurements with the Pierre Auger Observatory and their connection to the Muon Puzzle","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-01T05:12:26.591580Z"},"links":{"cited_paper":"/paper/2405.12004","citing_paper":"/paper/2607.22323"},"observation_digest":"sha256:ffac8f2894fcfc7a6b43fa3b0c8e1399049159b6bd232a4d28772979b14ba887","observation_id":"e85b41a1-8ff2-48c0-ae49-bd95fd313dbc","resolution":{"observed_at":"2026-08-01T05:12:26.591580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2405.12004/citation-record","integrity":"/paper/2405.12004/integrity","json":"/paper/2405.12004/citation-record.json","paper":"/paper/2405.12004"},"outbound":[],"paper":{"arxiv_id":"2405.12004","last_updated":"2025-02-13T18:44:27Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T18:16:42.428308Z","submitted_at":"2024-05-20T13:22:13Z","title":"Binary neutron star mergers as the source of the highest energy cosmic rays"},"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 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2405.12004."}