{"as_of":"2026-08-05T14:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9faaf35412c0ad545319d080d0cf382ee16869ae04cbbb53fab29c139fdae9ac","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":"2026-08-05T06:32:48.257954+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":"2026-05-25T03:56:11.714959Z","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":"2026-05-25T03:56:36.470571Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1803.04888","last_updated":"2018-03-13T15:38:30Z","snapshot_observed_at":"2026-07-06T06:28:04.898938Z","submitted_at":"2018-03-13T15:38:30Z","title":"A look at possible microwave dust emission via AKARI infrared all-sky surveys","version":1},"cited_work":{"arxiv_id":"1803.04888","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.04888","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"A look at possible microwave dust emission via AKARI infrared all-sky surveys","venue":"astro-ph.GA","work_id":"82eaf839-7353-4359-830d-ab70e25f03e3","year":2018},"citing_paper":{"arxiv_id":"2605.23489","last_updated":"2026-05-22T10:51:03Z","snapshot_observed_at":"2026-08-02T00:51:08.034872Z","submitted_at":"2026-05-22T10:51:03Z","title":"A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-05-25T03:56:11.714959Z"},"links":{"cited_paper":"/paper/1803.04888","citing_paper":"/paper/2605.23489"},"observation_digest":"sha256:a315859de870537cbfd5c1dc57344bb997e61a4a62b7e4d8614d271854bea96c","observation_id":"e0ee8b39-fbb6-4a33-aafe-b33ea3ee57e0","resolution":{"observed_at":"2026-05-25T03:56:36.472133Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1803.04888/citation-record","integrity":"/paper/1803.04888/integrity","json":"/paper/1803.04888/citation-record.json","paper":"/paper/1803.04888"},"outbound":[],"paper":{"arxiv_id":"1803.04888","last_updated":"2018-03-13T15:38:30Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T06:28:04.898938Z","submitted_at":"2018-03-13T15:38:30Z","title":"A look at possible microwave dust emission via AKARI infrared all-sky surveys"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1803.04888."}