{"as_of":"2026-08-08T18:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c9d27205029e0921846dcb407970f36ca2b079f814203212ab5ac8e636991de3","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":"2026-08-08T06:32:00.761636+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":"2026-08-07T12:45:48.260261Z","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":"2026-06-29T03:33:06.478876Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1807.09073","last_updated":"2018-07-24T12:49:52Z","snapshot_observed_at":"2026-07-06T06:51:57.907888Z","submitted_at":"2018-07-24T12:49:52Z","title":"The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.09073","snapshot_observed_at":"2026-08-07T12:45:48.260261Z","title":"Sinha, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.23645","last_updated":"2025-05-29T16:52:25Z","snapshot_observed_at":"2026-08-07T12:38:52.797126Z","submitted_at":"2025-05-29T16:52:25Z","title":"Comprehensive Variability Analysis of Blazars Using Fermi Light Curves Across Multiple Timescales","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T12:45:48.260261Z"},"links":{"cited_paper":"/paper/1807.09073","citing_paper":"/paper/2505.23645"},"observation_digest":"sha256:30bc6c33e8902dc1780840ec531d01f175acef97620caa9e640dc1928e28645a","observation_id":"b2e6e1a4-b8d6-4ca4-87ea-ad4c38665874","resolution":{"observed_at":"2026-08-07T12:45:48.260261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09073","last_updated":"2018-07-24T12:49:52Z","snapshot_observed_at":"2026-07-06T06:51:57.907888Z","submitted_at":"2018-07-24T12:49:52Z","title":"The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration","version":1},"cited_work":{"arxiv_id":"1807.09073","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.09073","snapshot_observed_at":"2026-06-29T03:33:06.478876Z","title":"The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration","venue":"astro-ph.HE","work_id":"b820f166-dfb4-4758-ac16-8342ae61edfc","year":2018},"citing_paper":{"arxiv_id":"2606.28088","last_updated":"2026-06-26T13:50:36Z","snapshot_observed_at":"2026-07-07T00:02:14.441610Z","submitted_at":"2026-06-26T13:50:36Z","title":"A Rare Gamma-ray Flaring episode of the Narrow-Line Seyfert 1 Galaxy 1H 0323+342","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1807.09073","citing_paper":"/paper/2606.28088"},"observation_digest":"sha256:634ccb45cd2790bc5e5502aa388277233d2596fecbb9c2279c7fa1f6fd9c2fee","observation_id":"92a5774c-3aed-4d35-a629-1be88f6c52ad","resolution":{"observed_at":"2026-06-29T03:33:06.480224Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1807.09073/citation-record","integrity":"/paper/1807.09073/integrity","json":"/paper/1807.09073/citation-record.json","paper":"/paper/1807.09073"},"outbound":[],"paper":{"arxiv_id":"1807.09073","last_updated":"2018-07-24T12:49:52Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T06:51:57.907888Z","submitted_at":"2018-07-24T12:49:52Z","title":"The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1807.09073."}