{"as_of":"2026-08-10T20:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:381aea492f2ac13792f0b60bc318d66987fe8ff64d1291c2c5c762fa5b824b6c","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-13T02:52:48.075479Z","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":"2026-07-13T02:59:21.427248Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1601.01698","last_updated":"2016-01-07T21:06:46Z","snapshot_observed_at":"2026-07-06T04:42:11.317805Z","submitted_at":"2016-01-07T21:06:46Z","title":"A New Star-Formation Rate Calibration from Polycyclic Aromatic Hydrocarbon Emission Features and Application to High Redshift Galaxies","version":1},"cited_work":{"arxiv_id":"1601.01698","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.01698","snapshot_observed_at":"2026-07-13T02:59:21.427248Z","title":"A New Star-Formation Rate Calibration from Polycyclic Aromatic Hydrocarbon Emission Features and Application to High Redshift Galaxies","venue":"astro-ph.GA","work_id":"9fef8dd5-9d85-4991-801f-3fbfe2535f55","year":2016},"citing_paper":{"arxiv_id":"2607.09460","last_updated":"2026-07-10T14:32:43Z","snapshot_observed_at":"2026-08-07T04:18:36.572626Z","submitted_at":"2026-07-10T14:32:43Z","title":"Project Hephaistos -- IV. James Webb Space Telescope Observations of Two Dyson Sphere Candidates","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-13T02:52:48.075479Z"},"links":{"cited_paper":"/paper/1601.01698","citing_paper":"/paper/2607.09460"},"observation_digest":"sha256:471bc6a09443cf0c126b6072e5c119f78ddba9bbd6d8c955b71e4804089c60ca","observation_id":"9ef7cfdb-d14d-47ca-a663-7a35813ff328","resolution":{"observed_at":"2026-07-13T02:59:21.430206Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1601.01698/citation-record","integrity":"/paper/1601.01698/integrity","json":"/paper/1601.01698/citation-record.json","paper":"/paper/1601.01698"},"outbound":[],"paper":{"arxiv_id":"1601.01698","last_updated":"2016-01-07T21:06:46Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T04:42:11.317805Z","submitted_at":"2016-01-07T21:06:46Z","title":"A New Star-Formation Rate Calibration from Polycyclic Aromatic Hydrocarbon Emission Features and Application to High Redshift Galaxies"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1601.01698."}