{"as_of":"2026-08-08T14:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d2d6abdd1834994161df1ce0f321fc8949c062bd98c5a6a724715e4003c9fed4","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":"2026-08-08T06:32:00.761636+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":"2026-08-06T00:40:22.841715Z","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":"2026-07-01T02:05:14.116526Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1702.02571","last_updated":"2017-03-30T09:41:13Z","snapshot_observed_at":"2026-07-06T05:29:20.465955Z","submitted_at":"2017-02-08T19:00:01Z","title":"The Fermi blazar sequence","version":2},"cited_work":{"arxiv_id":"1702.02571","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.02571","snapshot_observed_at":"2026-07-01T02:05:14.116526Z","title":"The Fermi blazar sequence","venue":"astro-ph.HE","work_id":"c51cd176-2de9-40f7-bfcb-46e40995d09f","year":2017},"citing_paper":{"arxiv_id":"2605.15867","last_updated":"2026-05-15T11:34:48Z","snapshot_observed_at":"2026-08-04T10:30:44.557237Z","submitted_at":"2026-05-15T11:34:48Z","title":"Spectral-Regime Overlap and Transition-like Behavior in the Blazar Population from Multi-Instrument X-ray and TeV Observations","version":1},"reference_index":299,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.02571","citing_paper":"/paper/2605.15867"},"observation_digest":"sha256:d8b68ee7329ba7cab0492fd6ffe4964e43f75505a44011a93eba042fc3381aa1","observation_id":"18714ea2-e425-4e4a-8c3f-50fca4aa9251","resolution":{"observed_at":"2026-05-20T18:58:53.566529Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02571","last_updated":"2017-03-30T09:41:13Z","snapshot_observed_at":"2026-07-06T05:29:20.465955Z","submitted_at":"2017-02-08T19:00:01Z","title":"The Fermi blazar sequence","version":2},"cited_work":{"arxiv_id":"1702.02571","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.02571","snapshot_observed_at":"2026-07-01T02:05:14.116526Z","title":"The Fermi blazar sequence","venue":"astro-ph.HE","work_id":"c51cd176-2de9-40f7-bfcb-46e40995d09f","year":2017},"citing_paper":{"arxiv_id":"2606.30764","last_updated":"2026-07-12T21:55:27Z","snapshot_observed_at":"2026-08-02T08:18:53.119406Z","submitted_at":"2026-06-29T18:01:35Z","title":"Active Galactic Nuclei as high-energy neutrino sources","version":1},"reference_index":241,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.02571","citing_paper":"/paper/2606.30764"},"observation_digest":"sha256:f1a6b9f53539621c9bfbc195567cb54953f25228c27d1bb26a4f04a9963fe1cc","observation_id":"6fbb66c9-9462-4b2a-b707-2797e4bb98e0","resolution":{"observed_at":"2026-07-01T02:05:14.117896Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02571","last_updated":"2017-03-30T09:41:13Z","snapshot_observed_at":"2026-07-06T05:29:20.465955Z","submitted_at":"2017-02-08T19:00:01Z","title":"The Fermi blazar sequence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02571","snapshot_observed_at":"2026-07-14T16:57:50.370612Z","title":"469(1):255--266","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2606.30764","last_updated":"2026-07-12T21:55:27Z","snapshot_observed_at":"2026-08-02T08:18:53.119406Z","submitted_at":"2026-06-29T18:01:35Z","title":"Active Galactic Nuclei as high-energy neutrino sources","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-14T16:57:50.370612Z"},"links":{"cited_paper":"/paper/1702.02571","citing_paper":"/paper/2606.30764"},"observation_digest":"sha256:11efe55029f0fc4a5a480c511a8bbf1e762c0b23e42ebe911c5dfcf3823bb03a","observation_id":"acf23dd2-79a4-4dbf-99d2-ed07d99bc1f7","resolution":{"observed_at":"2026-07-14T16:57:50.370612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02571","last_updated":"2017-03-30T09:41:13Z","snapshot_observed_at":"2026-07-06T05:29:20.465955Z","submitted_at":"2017-02-08T19:00:01Z","title":"The Fermi blazar sequence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02571","snapshot_observed_at":"2026-08-06T00:40:22.841715Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.00996","last_updated":"2026-08-02T04:46:19Z","snapshot_observed_at":"2026-08-06T23:25:17.286849Z","submitted_at":"2026-08-02T04:46:19Z","title":"Radio-Gamma-Ray Properties and High-Energy Implications for Fermi Blazars","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-06T00:40:22.841715Z"},"links":{"cited_paper":"/paper/1702.02571","citing_paper":"/paper/2608.00996"},"observation_digest":"sha256:b18c3163d07aef99c08d83bbca23983a1dab9cbfdde4aa59547c37e3211939bd","observation_id":"398c6c59-2cc0-40f9-94ef-dc51e26fcae0","resolution":{"observed_at":"2026-08-06T00:40:22.841715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1702.02571/citation-record","integrity":"/paper/1702.02571/integrity","json":"/paper/1702.02571/citation-record.json","paper":"/paper/1702.02571"},"outbound":[],"paper":{"arxiv_id":"1702.02571","last_updated":"2017-03-30T09:41:13Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T05:29:20.465955Z","submitted_at":"2017-02-08T19:00:01Z","title":"The Fermi blazar sequence"},"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 4 inbound Pith citation observations for arXiv:1702.02571."}