{"as_of":"2026-08-08T01:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fa069830a9ce1b7ce1d71ea954d9512f0ffe57b7e42a6e65fece3b42ecc645c7","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":"2026-08-07T06:34:17.273281+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":"2026-08-03T23:49:13.884871Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-11T06:10:58.685828Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1711.08327","last_updated":"2017-12-01T14:43:16Z","snapshot_observed_at":"2026-08-03T18:52:00.870248Z","submitted_at":"2017-11-22T15:18:18Z","title":"Tomography of cool giant and supergiant star atmospheres. I. Validation of the method","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.08327","snapshot_observed_at":"2026-08-03T23:49:13.884871Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.04254","last_updated":"2026-05-28T09:50:04Z","snapshot_observed_at":"2026-08-03T23:48:30.974746Z","submitted_at":"2025-11-06T10:42:14Z","title":"3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae","version":2},"reference_index":274,"source":"arxiv_source","source_observed_at":"2026-08-03T23:49:13.884871Z"},"links":{"cited_paper":"/paper/1711.08327","citing_paper":"/paper/2511.04254"},"observation_digest":"sha256:9da20b7283d45b5f1859e5f46da1b50519ea581761399c799479c377d476a7cf","observation_id":"3028b762-078b-463c-ac22-057727b60d19","resolution":{"observed_at":"2026-08-03T23:49:13.884871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.08327","last_updated":"2017-12-01T14:43:16Z","snapshot_observed_at":"2026-08-03T18:52:00.870248Z","submitted_at":"2017-11-22T15:18:18Z","title":"Tomography of cool giant and supergiant star atmospheres. I. Validation of the method","version":2},"cited_work":{"arxiv_id":"1711.08327","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1711.08327","snapshot_observed_at":"2026-07-04T22:33:49.965779Z","title":null,"venue":null,"work_id":"e038240b-6420-4ee0-ad88-aeebf3fc2499","year":2018},"citing_paper":{"arxiv_id":"2604.09205","last_updated":"2026-04-10T10:45:40Z","snapshot_observed_at":"2026-08-01T18:25:50.554931Z","submitted_at":"2026-04-10T10:45:40Z","title":"Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-10T17:47:10.739575Z"},"links":{"cited_paper":"/paper/1711.08327","citing_paper":"/paper/2604.09205"},"observation_digest":"sha256:436544a33e297b3e1fd84d2563b78b21badda14770a4bb63c5f1c6748030c974","observation_id":"bb426b3a-5515-40c7-966a-4673937cc236","resolution":{"observed_at":"2026-07-04T22:33:49.965779Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1711.08327/citation-record","integrity":"/paper/1711.08327/integrity","json":"/paper/1711.08327/citation-record.json","paper":"/paper/1711.08327"},"outbound":[],"paper":{"arxiv_id":"1711.08327","last_updated":"2017-12-01T14:43:16Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-03T18:52:00.870248Z","submitted_at":"2017-11-22T15:18:18Z","title":"Tomography of cool giant and supergiant star atmospheres. I. Validation of the method"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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:1711.08327."}