{"as_of":"2026-08-15T21:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e6d6ba70ed39738aa774853086b4b9e8eea883559dba344e7a2bc5bd2ea6f42f","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":"2026-08-15T06:32:42.880941+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":"2026-08-11T19:34:24.311013Z","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":"2026-07-03T18:48:49.150489Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1705.06090","last_updated":"2017-05-17T11:08:08Z","snapshot_observed_at":"2026-08-14T21:00:07.679299Z","submitted_at":"2017-05-17T11:08:08Z","title":"Observational evidence for two distinct giant planet populations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.06090","snapshot_observed_at":"2026-08-11T19:34:24.311013Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06594","last_updated":"2024-12-09T15:46:38Z","snapshot_observed_at":"2026-08-15T07:00:22.892385Z","submitted_at":"2024-12-09T15:46:38Z","title":"On the formation of super-Jupiters: Core Accretion or Gravitational Instability?","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-11T19:34:24.311013Z"},"links":{"cited_paper":"/paper/1705.06090","citing_paper":"/paper/2412.06594"},"observation_digest":"sha256:f7dbcab8ef8274b7d029018719f5687f86963683d7f5fb2fcbca12376a266796","observation_id":"3c57ccdb-9f7a-4014-a242-742c4acbf295","resolution":{"observed_at":"2026-08-11T19:34:24.311013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.06090","last_updated":"2017-05-17T11:08:08Z","snapshot_observed_at":"2026-08-14T21:00:07.679299Z","submitted_at":"2017-05-17T11:08:08Z","title":"Observational evidence for two distinct giant planet populations","version":1},"cited_work":{"arxiv_id":"1705.06090","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.06090","snapshot_observed_at":"2026-07-03T18:48:49.150489Z","title":"Observational evidence for two distinct giant planet populations","venue":"astro-ph.EP","work_id":"22636ef0-a895-4a2a-b1b2-9213266e3ab9","year":2017},"citing_paper":{"arxiv_id":"2607.01315","last_updated":"2026-07-01T18:00:00Z","snapshot_observed_at":"2026-08-12T16:55:31.008925Z","submitted_at":"2026-07-01T18:00:00Z","title":"Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss","version":1},"reference_index":209,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1705.06090","citing_paper":"/paper/2607.01315"},"observation_digest":"sha256:2a81639893860735869295d76113301c53e38f03b7be86ad00ba4115b0539556","observation_id":"36765f21-0f68-4bce-9763-b79b351e5a85","resolution":{"observed_at":"2026-07-03T18:48:49.151718Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1705.06090/citation-record","integrity":"/paper/1705.06090/integrity","json":"/paper/1705.06090/citation-record.json","paper":"/paper/1705.06090"},"outbound":[],"paper":{"arxiv_id":"1705.06090","last_updated":"2017-05-17T11:08:08Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-14T21:00:07.679299Z","submitted_at":"2017-05-17T11:08:08Z","title":"Observational evidence for two distinct giant planet populations"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1705.06090."}