{"as_of":"2026-08-12T18:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a8476b804f775b6eb02ec79f8f2643ae7fa0304b5129b874cbcfbef19f0c5ac3","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":"2026-08-12T06:34:41.77262+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":"2026-08-11T23:13:10.690200Z","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":"2026-08-11T23:13:11.357547Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1208.4685","last_updated":"2012-08-23T08:11:15Z","snapshot_observed_at":"2026-07-06T02:54:13.777135Z","submitted_at":"2012-08-23T08:11:15Z","title":"NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity","version":1},"cited_work":{"arxiv_id":"1208.4685","doi":null,"metadata_source":"pith","pith_arxiv_id":"1208.4685","snapshot_observed_at":"2026-08-11T23:13:11.357547Z","title":"NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity","venue":"astro-ph.EP","work_id":"099a0553-2ddd-48bf-8d5c-358caab42ae3","year":2012},"citing_paper":{"arxiv_id":"2412.02785","last_updated":"2024-12-03T19:26:19Z","snapshot_observed_at":"2026-08-12T18:06:29.077474Z","submitted_at":"2024-12-03T19:26:19Z","title":"Accretion of Uranus and Neptune: confronting different giant impact scenarios","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T23:13:10.690200Z"},"links":{"cited_paper":"/paper/1208.4685","citing_paper":"/paper/2412.02785"},"observation_digest":"sha256:3339c6d5438204ee7e8825ada4db0402d454c8f6f2c56a60e05c5a91326e703c","observation_id":"f3c5eaf1-bcc7-42ee-873d-e0d61270724a","resolution":{"observed_at":"2026-08-11T23:13:11.362056Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.4685","last_updated":"2012-08-23T08:11:15Z","snapshot_observed_at":"2026-07-06T02:54:13.777135Z","submitted_at":"2012-08-23T08:11:15Z","title":"NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.4685","snapshot_observed_at":"2026-08-01T13:29:15.372796Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.19118","last_updated":"2026-07-21T14:04:46Z","snapshot_observed_at":"2026-08-07T07:38:37.470320Z","submitted_at":"2026-07-21T14:04:46Z","title":"Dynamical formation of long-period exoplanets systems in evolving binary stars","version":1},"reference_index":129,"source":"arxiv_source","source_observed_at":"2026-08-01T13:29:15.372796Z"},"links":{"cited_paper":"/paper/1208.4685","citing_paper":"/paper/2607.19118"},"observation_digest":"sha256:ac0620a0433afb1e449a2b062e066c25a3a520743b078c784042ebc32f7e444c","observation_id":"8d89c949-0f97-4a2b-a977-6a25a64d9af5","resolution":{"observed_at":"2026-08-01T13:29:15.372796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1208.4685/citation-record","integrity":"/paper/1208.4685/integrity","json":"/paper/1208.4685/citation-record.json","paper":"/paper/1208.4685"},"outbound":[],"paper":{"arxiv_id":"1208.4685","last_updated":"2012-08-23T08:11:15Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-07-06T02:54:13.777135Z","submitted_at":"2012-08-23T08:11:15Z","title":"NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1208.4685."}