{"as_of":"2026-08-06T00:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:32411a3d315e904a6f8e871dd8b81793746fc3422500d0893ca6bc81662c6186","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":"2026-07-11T11:50:26.030339Z","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":"2026-06-29T01:22:56.170167Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1701.08040","last_updated":"2017-01-27T12:55:10Z","snapshot_observed_at":"2026-07-06T05:27:49.254573Z","submitted_at":"2017-01-27T12:55:10Z","title":"CO2 infrared emission as a diagnostic of planet-forming regions of disks","version":1},"cited_work":{"arxiv_id":"1701.08040","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.08040","snapshot_observed_at":"2026-06-29T01:22:56.170167Z","title":"CO2 infrared emission as a diagnostic of planet-forming regions of disks","venue":"astro-ph.SR","work_id":"b71563d7-c78a-4fab-ae7a-751785267123","year":2017},"citing_paper":{"arxiv_id":"2606.27477","last_updated":"2026-06-25T18:56:07Z","snapshot_observed_at":"2026-08-04T12:41:17.185796Z","submitted_at":"2026-06-25T18:56:07Z","title":"From Young to Older Disks: JWST/MIRI Evidence for Fading Molecular Emission and Hints for Elevated C/O in Upper Scorpius","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1701.08040","citing_paper":"/paper/2606.27477"},"observation_digest":"sha256:1bbc7b9e1adbe0da7d0c88f25545e76abda700807b2eb67d1ae5fb28c427e1b0","observation_id":"02ebcd74-1f54-4fd7-b701-2b0bc5aa8d92","resolution":{"observed_at":"2026-06-29T01:22:56.171628Z","resolver_source":"local_arxiv","status":"verified_exact"},"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/1701.08040/citation-record","integrity":"/paper/1701.08040/integrity","json":"/paper/1701.08040/citation-record.json","paper":"/paper/1701.08040"},"outbound":[],"paper":{"arxiv_id":"1701.08040","last_updated":"2017-01-27T12:55:10Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T05:27:49.254573Z","submitted_at":"2017-01-27T12:55:10Z","title":"CO2 infrared emission as a diagnostic of planet-forming regions of disks"},"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 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1701.08040."}