{"as_of":"2026-08-22T19:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ff3e137205e13e6992de02f7f20acd5b11a1cd5aea786048ded51f96141ada2c","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T06:05:07.719948Z","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":"2026-05-22T09:11:20.059275Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1603.00463","last_updated":"2016-03-30T09:05:47Z","snapshot_observed_at":"2026-08-14T22:07:59.187895Z","submitted_at":"2016-03-01T21:00:01Z","title":"Ultra-diffuse galaxies: the high-spin tail of the abundant dwarf galaxy population","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.00463","snapshot_observed_at":"2026-08-04T06:05:07.719948Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2602.14747","last_updated":"2026-08-03T08:54:52Z","snapshot_observed_at":"2026-08-11T01:45:09.772607Z","submitted_at":"2026-02-16T13:43:08Z","title":"Exploring Non-minimal coupling using ultra-diffuse galaxies","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-04T06:05:07.719948Z"},"links":{"cited_paper":"/paper/1603.00463","citing_paper":"/paper/2602.14747"},"observation_digest":"sha256:6107d9ad21136981b202c5db15c7abc2f3b7bd9e275625b46e601de33c55bd4b","observation_id":"2109f426-6319-4785-a4c7-0b9ffe54a077","resolution":{"observed_at":"2026-08-04T06:05:07.719948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00463","last_updated":"2016-03-30T09:05:47Z","snapshot_observed_at":"2026-08-14T22:07:59.187895Z","submitted_at":"2016-03-01T21:00:01Z","title":"Ultra-diffuse galaxies: the high-spin tail of the abundant dwarf galaxy population","version":2},"cited_work":{"arxiv_id":"1603.00463","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.00463","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ultra-diffuse galaxies: the high-spin tail of the abundant dwarf galaxy population","venue":"astro-ph.GA","work_id":"07cf3024-f937-44e9-a685-98ccdde62267","year":2016},"citing_paper":{"arxiv_id":"2605.13842","last_updated":"2026-05-13T17:58:55Z","snapshot_observed_at":"2026-07-18T23:18:11.723165Z","submitted_at":"2026-05-13T17:58:55Z","title":"From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies","version":1},"reference_index":203,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.00463","citing_paper":"/paper/2605.13842"},"observation_digest":"sha256:dc722982ebf8c47df4d92324d445e3be1c9ede4ab6708ebfb4fd0a3b1361fc36","observation_id":"1a186860-9fcb-4b88-bf7c-d4f1b457af40","resolution":{"observed_at":"2026-05-14T17:47:31.149379Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00463","last_updated":"2016-03-30T09:05:47Z","snapshot_observed_at":"2026-08-14T22:07:59.187895Z","submitted_at":"2016-03-01T21:00:01Z","title":"Ultra-diffuse galaxies: the high-spin tail of the abundant dwarf galaxy population","version":2},"cited_work":{"arxiv_id":"1603.00463","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.00463","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ultra-diffuse galaxies: the high-spin tail of the abundant dwarf galaxy population","venue":"astro-ph.GA","work_id":"07cf3024-f937-44e9-a685-98ccdde62267","year":2016},"citing_paper":{"arxiv_id":"2605.21598","last_updated":"2026-05-20T18:01:04Z","snapshot_observed_at":"2026-08-12T14:43:42.309267Z","submitted_at":"2026-05-20T18:01:04Z","title":"Advancing the detection of low surface brightness galaxies. I. ATTILA: multi-tAsking deTecTIon tool for Lsb gAlaxies","version":1},"reference_index":187,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.00463","citing_paper":"/paper/2605.21598"},"observation_digest":"sha256:8b637c3e185d953276b26050c3546da551f387130efa4b14e922226a57e9bb55","observation_id":"b523fc63-3924-44b7-9e62-53075c6eb3d9","resolution":{"observed_at":"2026-05-22T09:11:20.061751Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1603.00463/citation-record","integrity":"/paper/1603.00463/integrity","json":"/paper/1603.00463/citation-record.json","paper":"/paper/1603.00463"},"outbound":[],"paper":{"arxiv_id":"1603.00463","last_updated":"2016-03-30T09:05:47Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T22:07:59.187895Z","submitted_at":"2016-03-01T21:00:01Z","title":"Ultra-diffuse galaxies: the high-spin tail of the abundant dwarf galaxy population"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1603.00463."}