{"as_of":"2026-08-12T10:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7483e04676d612613ac51634d0b4d7d4c7f38b53bacebe3b7ab7b9ef6f126bcb","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:15:10.776130Z","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":"2026-08-10T21:10:14.044495Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2111.05864","last_updated":"2021-11-10T19:00:00Z","snapshot_observed_at":"2026-07-06T12:07:19.954510Z","submitted_at":"2021-11-10T19:00:00Z","title":"Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars","version":1},"cited_work":{"arxiv_id":"2111.05864","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.05864","snapshot_observed_at":"2026-08-10T21:10:14.044495Z","title":"Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars","venue":"astro-ph.HE","work_id":"e1ebf4be-7fa3-49fa-8327-26df13910483","year":2021},"citing_paper":{"arxiv_id":"2501.06011","last_updated":"2025-07-01T11:50:03Z","snapshot_observed_at":"2026-08-11T08:54:43.684630Z","submitted_at":"2025-01-10T14:48:22Z","title":"SECRET: Stochasticity Emulator for Cosmic Ray Electrons","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T21:10:13.775531Z"},"links":{"cited_paper":"/paper/2111.05864","citing_paper":"/paper/2501.06011"},"observation_digest":"sha256:018626ed1ec137c573c1f08c36c133bb5f08a4e54f4a5962c6af9af47692ef86","observation_id":"0adf0aec-b5ea-4d50-ba6b-715d8f06f065","resolution":{"observed_at":"2026-08-10T21:10:14.048894Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.05864","last_updated":"2021-11-10T19:00:00Z","snapshot_observed_at":"2026-07-06T12:07:19.954510Z","submitted_at":"2021-11-10T19:00:00Z","title":"Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.05864","snapshot_observed_at":"2026-08-11T19:15:10.776130Z","title":"Cholis and I","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.09336","last_updated":"2026-08-10T09:13:40Z","snapshot_observed_at":"2026-08-12T09:17:49.787493Z","submitted_at":"2026-08-10T09:13:40Z","title":"Astrophysical origins of TeV features in the cosmic-ray lepton spectrum","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T19:15:10.776130Z"},"links":{"cited_paper":"/paper/2111.05864","citing_paper":"/paper/2608.09336"},"observation_digest":"sha256:f4e120c6b9ea0e3d1a949207b03a9db3c56a2e199f471725b7c2bcfd496f889d","observation_id":"5813c0f2-91b3-4f9d-8e7f-9faa84c6ba73","resolution":{"observed_at":"2026-08-11T19:15:10.776130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2111.05864/citation-record","integrity":"/paper/2111.05864/integrity","json":"/paper/2111.05864/citation-record.json","paper":"/paper/2111.05864"},"outbound":[],"paper":{"arxiv_id":"2111.05864","last_updated":"2021-11-10T19:00:00Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T12:07:19.954510Z","submitted_at":"2021-11-10T19:00:00Z","title":"Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.05864."}