{"as_of":"2026-08-05T04:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5730e9aa098a5437f737121cc08202dff73aa8551b7fa9df5c2f48c4b7579e1a","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":"2026-08-04T06:34:03.388597+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":"2026-08-02T07:35:32.209021Z","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":"2026-07-10T18:17:33.230288Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1702.02904","last_updated":"2017-02-09T17:19:50Z","snapshot_observed_at":"2026-07-06T05:29:26.748965Z","submitted_at":"2017-02-09T17:19:50Z","title":"Searching for chemical signatures of brown dwarf formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02904","snapshot_observed_at":"2026-07-12T07:45:39.933353Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.02682","last_updated":"2026-07-09T13:08:58Z","snapshot_observed_at":"2026-08-03T17:31:23.520740Z","submitted_at":"2026-07-02T18:23:47Z","title":"On the Eccentricity Distribution and Tidal Evolution of Transiting Brown Dwarfs","version":2},"reference_index":136,"source":"arxiv_source","source_observed_at":"2026-07-12T07:45:39.933353Z"},"links":{"cited_paper":"/paper/1702.02904","citing_paper":"/paper/2607.02682"},"observation_digest":"sha256:775ce0630f42bbba8d4d4c92fd4ecc7c20004d5343971dc6f077248f8d013afb","observation_id":"c5f458ff-6126-4c5d-85bb-a0fbf2706256","resolution":{"observed_at":"2026-07-12T07:45:39.933353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02904","last_updated":"2017-02-09T17:19:50Z","snapshot_observed_at":"2026-07-06T05:29:26.748965Z","submitted_at":"2017-02-09T17:19:50Z","title":"Searching for chemical signatures of brown dwarf formation","version":1},"cited_work":{"arxiv_id":"1702.02904","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.02904","snapshot_observed_at":"2026-07-10T18:17:33.230288Z","title":"Searching for chemical signatures of brown dwarf formation","venue":"astro-ph.SR","work_id":"eed756e6-53af-4473-bcce-100cd338758e","year":2017},"citing_paper":{"arxiv_id":"2607.07787","last_updated":"2026-07-08T18:00:00Z","snapshot_observed_at":"2026-08-01T19:41:50.334203Z","submitted_at":"2026-07-08T18:00:00Z","title":"Probing the origins. III. Exoplanet demographics across Galactic birth radii","version":1},"reference_index":112,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.02904","citing_paper":"/paper/2607.07787"},"observation_digest":"sha256:abf1cb755e918ae1ee513e943fd4f63e0684dbc7fca9b88a7c193139b64f29fb","observation_id":"4ec513ff-1d98-462d-af7e-634d0edda674","resolution":{"observed_at":"2026-07-10T18:17:33.231780Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02904","last_updated":"2017-02-09T17:19:50Z","snapshot_observed_at":"2026-07-06T05:29:26.748965Z","submitted_at":"2017-02-09T17:19:50Z","title":"Searching for chemical signatures of brown dwarf formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02904","snapshot_observed_at":"2026-07-14T15:03:55.648723Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09851","last_updated":"2026-07-14T18:49:23Z","snapshot_observed_at":"2026-08-02T07:35:18.884396Z","submitted_at":"2026-07-10T18:00:00Z","title":"Benchmark Brown Dwarf Systems I: Chemical Abundance Analysis of FGK Stars with Wide-Separation Brown Dwarf Companions Using PEPSI","version":1},"reference_index":289,"source":"arxiv_source","source_observed_at":"2026-07-14T15:03:55.648723Z"},"links":{"cited_paper":"/paper/1702.02904","citing_paper":"/paper/2607.09851"},"observation_digest":"sha256:66fb658dcb347ba488bccc0834ee74414bc5ff068619fd8d4fd2cd8cbb620dcf","observation_id":"6399d8b6-42a5-4efd-a5db-733e55b00060","resolution":{"observed_at":"2026-07-14T15:03:55.648723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02904","last_updated":"2017-02-09T17:19:50Z","snapshot_observed_at":"2026-07-06T05:29:26.748965Z","submitted_at":"2017-02-09T17:19:50Z","title":"Searching for chemical signatures of brown dwarf formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02904","snapshot_observed_at":"2026-08-02T07:35:32.209021Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09851","last_updated":"2026-07-14T18:49:23Z","snapshot_observed_at":"2026-08-02T07:35:18.884396Z","submitted_at":"2026-07-10T18:00:00Z","title":"Benchmark Brown Dwarf Systems I: Chemical Abundance Analysis of FGK Stars with Wide-Separation Brown Dwarf Companions Using PEPSI","version":2},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-02T07:35:32.209021Z"},"links":{"cited_paper":"/paper/1702.02904","citing_paper":"/paper/2607.09851"},"observation_digest":"sha256:93e61ce4ca189fae6cf27254f21d1a7f2e4ea83a3701bdce5fa2abec1e6e015e","observation_id":"3e325816-9a9d-4953-9299-1ea487d378ec","resolution":{"observed_at":"2026-08-02T07:35:32.209021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1702.02904/citation-record","integrity":"/paper/1702.02904/integrity","json":"/paper/1702.02904/citation-record.json","paper":"/paper/1702.02904"},"outbound":[],"paper":{"arxiv_id":"1702.02904","last_updated":"2017-02-09T17:19:50Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T05:29:26.748965Z","submitted_at":"2017-02-09T17:19:50Z","title":"Searching for chemical signatures of brown dwarf formation"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1702.02904."}