{"as_of":"2026-08-16T01:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f0bb81cc4cea707d8e5cb911323940180790623f74dacfe385479a268386f8ba","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":"2026-08-15T06:32:42.880941+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":"2026-08-14T11:37:46.835659Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-05-23T04:42:34.737101Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1102.2688","last_updated":"2011-02-14T07:37:31Z","snapshot_observed_at":"2026-08-15T13:39:59.688436Z","submitted_at":"2011-02-14T07:37:31Z","title":"Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.2688","snapshot_observed_at":"2026-08-14T11:37:46.835659Z","title":"Honda, T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.08765","last_updated":"2019-11-27T06:22:08Z","snapshot_observed_at":"2026-08-15T15:11:18.014756Z","submitted_at":"2019-08-23T11:40:50Z","title":"Reduction of the Uncertainty in the Atmospheric Neutrino Flux Prediction Below 1 GeV Using Accurately Measured Atmospheric Muon Flux","version":4},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:37:46.835659Z"},"links":{"cited_paper":"/paper/1102.2688","citing_paper":"/paper/1908.08765"},"observation_digest":"sha256:caa3717bf7d5cb492588f74a59ba03845ed408dcbb0b9a18da8ead83747a3eb8","observation_id":"50351751-412c-49bf-919c-66096a3190b3","resolution":{"observed_at":"2026-08-14T11:37:46.835659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.2688","last_updated":"2011-02-14T07:37:31Z","snapshot_observed_at":"2026-08-15T13:39:59.688436Z","submitted_at":"2011-02-14T07:37:31Z","title":"Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.2688","snapshot_observed_at":"2026-08-12T17:44:59.864599Z","title":"Honda, T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.12344","last_updated":"2025-01-27T02:21:30Z","snapshot_observed_at":"2026-08-15T12:09:42.073720Z","submitted_at":"2024-11-19T08:52:35Z","title":"Neutrino Oscillation Tomography of the Earth with the Hyper-Kamiokande Detector","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T17:44:59.864599Z"},"links":{"cited_paper":"/paper/1102.2688","citing_paper":"/paper/2411.12344"},"observation_digest":"sha256:7e75bf3663cb01298aca036ec7ddd722febaa89b83da2f6290e84cdcc76a97f8","observation_id":"7d1aa3aa-4c70-4974-8fa2-3ef4c7bedf18","resolution":{"observed_at":"2026-08-12T17:44:59.864599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.2688","last_updated":"2011-02-14T07:37:31Z","snapshot_observed_at":"2026-08-15T13:39:59.688436Z","submitted_at":"2011-02-14T07:37:31Z","title":"Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.2688","snapshot_observed_at":"2026-08-11T11:20:04.388954Z","title":"Honda, T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.15641","last_updated":"2025-08-02T11:35:09Z","snapshot_observed_at":"2026-08-15T12:56:19.151275Z","submitted_at":"2024-12-20T07:57:48Z","title":"Composite asymmetric dark matter with a dark photon portal: Multimessenger tests","version":2},"reference_index":140,"source":"pdf_text","source_observed_at":"2026-08-11T11:20:04.388954Z"},"links":{"cited_paper":"/paper/1102.2688","citing_paper":"/paper/2412.15641"},"observation_digest":"sha256:afdde4354d8975e7b6b3a2b90fe1519fcfcd0e25f3273d6cd36c9a27e6835634","observation_id":"5d83ca61-b638-493c-8c52-99aa5cdb92c1","resolution":{"observed_at":"2026-08-11T11:20:04.388954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.2688","last_updated":"2011-02-14T07:37:31Z","snapshot_observed_at":"2026-08-15T13:39:59.688436Z","submitted_at":"2011-02-14T07:37:31Z","title":"Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model","version":1},"cited_work":{"arxiv_id":"1102.2688","doi":null,"metadata_source":"pith","pith_arxiv_id":"1102.2688","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model","venue":"astro-ph.HE","work_id":"4ffaf680-0955-4929-b0ba-d852599a54b7","year":2011},"citing_paper":{"arxiv_id":"2501.14864","last_updated":"2026-05-14T04:49:22Z","snapshot_observed_at":"2026-08-15T02:10:50.553723Z","submitted_at":"2025-01-24T19:00:00Z","title":"Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun","version":3},"reference_index":126,"source":"pdf_text","source_observed_at":"2026-05-23T04:38:44.009565Z"},"links":{"cited_paper":"/paper/1102.2688","citing_paper":"/paper/2501.14864"},"observation_digest":"sha256:21ac0cbd49e54bff26599c12e6b7120c6b42e02ed2782f72a8cf3c1202638653","observation_id":"ab53fa6b-306e-4617-b81c-63de6b4dbe73","resolution":{"observed_at":"2026-05-23T04:42:34.739706Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1102.2688/citation-record","integrity":"/paper/1102.2688/integrity","json":"/paper/1102.2688/citation-record.json","paper":"/paper/1102.2688"},"outbound":[],"paper":{"arxiv_id":"1102.2688","last_updated":"2011-02-14T07:37:31Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-15T13:39:59.688436Z","submitted_at":"2011-02-14T07:37:31Z","title":"Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1102.2688."}