{"as_of":"2026-08-11T17:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:73dbb49cfebec48fadf4d86b2833dec2327f4ac35caf684cacdd5d951a15c70d","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":"2026-08-11T06:34:44.6726+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":"2026-08-06T17:43:12.318276Z","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":"2026-07-02T14:57:04.846522Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1504.05397","last_updated":"2015-11-24T16:21:19Z","snapshot_observed_at":"2026-07-30T17:36:14.492893Z","submitted_at":"2015-04-21T12:03:27Z","title":"An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05397","snapshot_observed_at":"2026-08-06T17:43:12.318276Z","title":"Aab et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.10214","last_updated":"2025-07-24T11:20:15Z","snapshot_observed_at":"2026-08-11T14:28:34.629966Z","submitted_at":"2025-07-14T12:31:42Z","title":"Search for Ultra-High-Energy Neutrinos at the Pierre Auger Observatory: New Triggers, Methods, and Constraints","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T17:43:12.318276Z"},"links":{"cited_paper":"/paper/1504.05397","citing_paper":"/paper/2507.10214"},"observation_digest":"sha256:c54d29a55c36adba1b6e87fc850b257a6a0180cccac03237be68879a01e6f8f4","observation_id":"548e7b25-6686-4fba-ba6c-2fd7e692443b","resolution":{"observed_at":"2026-08-06T17:43:12.318276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05397","last_updated":"2015-11-24T16:21:19Z","snapshot_observed_at":"2026-07-30T17:36:14.492893Z","submitted_at":"2015-04-21T12:03:27Z","title":"An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05397","snapshot_observed_at":"2026-08-03T10:36:36.559985Z","title":"Aabet al.(Pierre Auger), Phys","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2601.09790","last_updated":"2026-06-09T22:42:56Z","snapshot_observed_at":"2026-08-07T12:38:27.225346Z","submitted_at":"2026-01-14T19:00:23Z","title":"The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T10:36:36.559985Z"},"links":{"cited_paper":"/paper/1504.05397","citing_paper":"/paper/2601.09790"},"observation_digest":"sha256:1e72f4feb71babb0c3beeedf9b7dd88cd3f8c5262a750947c5d3c7cf6dc27a6b","observation_id":"46ac7710-4f3c-4d3c-9e2c-014b504ef99b","resolution":{"observed_at":"2026-08-03T10:36:36.559985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05397","last_updated":"2015-11-24T16:21:19Z","snapshot_observed_at":"2026-07-30T17:36:14.492893Z","submitted_at":"2015-04-21T12:03:27Z","title":"An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":"1504.05397","doi":null,"metadata_source":"pith","pith_arxiv_id":"1504.05397","snapshot_observed_at":"2026-07-02T14:57:04.846522Z","title":"An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory","venue":"astro-ph.HE","work_id":"a6432fd2-1496-495e-bd44-7b0d979a0524","year":2015},"citing_paper":{"arxiv_id":"2606.06773","last_updated":"2026-06-04T23:34:44Z","snapshot_observed_at":"2026-08-04T00:00:17.590114Z","submitted_at":"2026-06-04T23:34:44Z","title":"Lepton interactions from GeV to EeV","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-28T00:06:38.765589Z"},"links":{"cited_paper":"/paper/1504.05397","citing_paper":"/paper/2606.06773"},"observation_digest":"sha256:64b3eea8a56ee3a5dc82ace4b36cc13feced9cf41bfd08af021ffca3f43eb2e3","observation_id":"0e620bed-82c0-4dc9-b94c-5e267d927e97","resolution":{"observed_at":"2026-07-02T14:57:04.847867Z","resolver_source":"local_arxiv","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":"1504.05397","last_updated":"2015-11-24T16:21:19Z","snapshot_observed_at":"2026-07-30T17:36:14.492893Z","submitted_at":"2015-04-21T12:03:27Z","title":"An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05397","snapshot_observed_at":"2026-08-06T00:17:57.476098Z","title":"Aabet al.(Pierre Auger), Phys","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.01496","last_updated":"2026-08-02T20:57:54Z","snapshot_observed_at":"2026-08-08T22:50:02.081071Z","submitted_at":"2026-08-02T20:57:54Z","title":"Search for active-sterile neutrino transitions using Pierre Auger Observatory data","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T00:17:57.476098Z"},"links":{"cited_paper":"/paper/1504.05397","citing_paper":"/paper/2608.01496"},"observation_digest":"sha256:e77480d32761d2cd346caf31207b1c64a209665e0ae51e15f17f4254f2cd391c","observation_id":"3ae8aac3-026f-43ed-b8a8-b8fe78c88d36","resolution":{"observed_at":"2026-08-06T00:17:57.476098Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1504.05397/citation-record","integrity":"/paper/1504.05397/integrity","json":"/paper/1504.05397/citation-record.json","paper":"/paper/1504.05397"},"outbound":[],"paper":{"arxiv_id":"1504.05397","last_updated":"2015-11-24T16:21:19Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-30T17:36:14.492893Z","submitted_at":"2015-04-21T12:03:27Z","title":"An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory"},"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 4 inbound Pith citation observations for arXiv:1504.05397."}