{"as_of":"2026-08-07T19:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3c7ff542a8a94e679a2cad75d8229427ebd7e582caeba31986c3d7aed2edcf94","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":"2026-08-07T06:34:17.273281+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":"2026-08-06T11:45:35.529151Z","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":"2026-07-03T02:57:35.302035Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1711.11432","last_updated":"2017-11-30T14:40:38Z","snapshot_observed_at":"2026-07-06T06:12:05.411952Z","submitted_at":"2017-11-30T14:40:38Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.11432","snapshot_observed_at":"2026-08-06T11:45:35.529151Z","title":"Dembinski, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.22463","last_updated":"2025-09-05T09:29:13Z","snapshot_observed_at":"2026-08-06T20:30:01.234110Z","submitted_at":"2025-07-30T08:10:02Z","title":"A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors","version":3},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-06T11:45:35.529151Z"},"links":{"cited_paper":"/paper/1711.11432","citing_paper":"/paper/2507.22463"},"observation_digest":"sha256:d1d77e1a1ea5c1dac9a141c8f026aa677c886f57500ab4d266b89c27d21d2e39","observation_id":"2ba05099-f955-47f3-ae02-3daee5f85a6e","resolution":{"observed_at":"2026-08-06T11:45:35.529151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.11432","last_updated":"2017-11-30T14:40:38Z","snapshot_observed_at":"2026-07-06T06:12:05.411952Z","submitted_at":"2017-11-30T14:40:38Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.11432","snapshot_observed_at":"2026-08-03T17:08:36.111670Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2512.10744","last_updated":"2026-05-26T23:48:16Z","snapshot_observed_at":"2026-08-03T23:20:30.720746Z","submitted_at":"2025-12-11T15:32:01Z","title":"Exploring New Propagation Scales With Galactic Neutrinos","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-03T17:08:36.111670Z"},"links":{"cited_paper":"/paper/1711.11432","citing_paper":"/paper/2512.10744"},"observation_digest":"sha256:1193adc0a1795921d56d7a29c31fcb6323d151178c5ccb5727655c8170cb55f7","observation_id":"37ba7773-5720-4355-bde5-af8a9f5cbc12","resolution":{"observed_at":"2026-08-03T17:08:36.111670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.11432","last_updated":"2017-11-30T14:40:38Z","snapshot_observed_at":"2026-07-06T06:12:05.411952Z","submitted_at":"2017-11-30T14:40:38Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV","version":1},"cited_work":{"arxiv_id":"1711.11432","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.11432","snapshot_observed_at":"2026-07-03T02:57:35.302035Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV","venue":"astro-ph.HE","work_id":"feadb6b4-6ccd-44ea-870a-e45f4f9b682c","year":2017},"citing_paper":{"arxiv_id":"2606.06029","last_updated":"2026-06-04T11:22:14Z","snapshot_observed_at":"2026-08-02T08:31:16.406160Z","submitted_at":"2026-06-04T11:22:14Z","title":"Mountain Muography for China Jinping Underground Laboratory","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-27T23:03:40.799637Z"},"links":{"cited_paper":"/paper/1711.11432","citing_paper":"/paper/2606.06029"},"observation_digest":"sha256:78581b856ac2aac9ada3fc1b00e431ee0d40c137ca24a60400153d01b7701fd5","observation_id":"880a28e9-1895-45a7-9ba1-f385944e7d11","resolution":{"observed_at":"2026-07-02T16:07:08.599109Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.11432","last_updated":"2017-11-30T14:40:38Z","snapshot_observed_at":"2026-07-06T06:12:05.411952Z","submitted_at":"2017-11-30T14:40:38Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV","version":1},"cited_work":{"arxiv_id":"1711.11432","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.11432","snapshot_observed_at":"2026-07-03T02:57:35.302035Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV","venue":"astro-ph.HE","work_id":"feadb6b4-6ccd-44ea-870a-e45f4f9b682c","year":2017},"citing_paper":{"arxiv_id":"2606.09604","last_updated":"2026-06-08T15:13:49Z","snapshot_observed_at":"2026-08-01T21:00:39.820232Z","submitted_at":"2026-06-08T15:13:49Z","title":"Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-06-27T15:39:48.644607Z"},"links":{"cited_paper":"/paper/1711.11432","citing_paper":"/paper/2606.09604"},"observation_digest":"sha256:c2dec0167b61fe46817d0352f26f97d08702317de43407d7ecf6d870935a141b","observation_id":"69dbf327-6fe8-40de-9d29-5fcb9d16c465","resolution":{"observed_at":"2026-07-03T02:57:35.303761Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1711.11432/citation-record","integrity":"/paper/1711.11432/integrity","json":"/paper/1711.11432/citation-record.json","paper":"/paper/1711.11432"},"outbound":[],"paper":{"arxiv_id":"1711.11432","last_updated":"2017-11-30T14:40:38Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T06:12:05.411952Z","submitted_at":"2017-11-30T14:40:38Z","title":"Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1711.11432."}