{"as_of":"2026-08-06T02:36:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7f7dfe1229c16445691adcf6cef1a617d53262ee1c94c37221c98bb650b9ee34","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":"2026-08-05T06:32:48.257954+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":"2026-08-04T19:31:00.890372Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1706.00417","last_updated":"2017-11-09T17:51:21Z","snapshot_observed_at":"2026-07-06T05:45:13.627570Z","submitted_at":"2017-06-01T17:58:23Z","title":"Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.00417","snapshot_observed_at":"2026-08-04T19:31:00.890372Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.09305","last_updated":"2025-09-11T09:45:48Z","snapshot_observed_at":"2026-08-04T19:30:52.721017Z","submitted_at":"2025-09-11T09:45:48Z","title":"Dust growth and planet formation by disc fragmentation","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-04T19:31:00.890372Z"},"links":{"cited_paper":"/paper/1706.00417","citing_paper":"/paper/2509.09305"},"observation_digest":"sha256:b2daba6bd5da0cd475fffd2d394f1bde3c4e69aa75188603991305f812af8966","observation_id":"95e71546-ebd6-4f24-aded-44be798b4db9","resolution":{"observed_at":"2026-08-04T19:31:00.890372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.00417","last_updated":"2017-11-09T17:51:21Z","snapshot_observed_at":"2026-07-06T05:45:13.627570Z","submitted_at":"2017-06-01T17:58:23Z","title":"Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.00417","snapshot_observed_at":"2026-08-02T01:02:18.453993Z","title":"ApJ , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14828","last_updated":"2026-07-16T10:46:59Z","snapshot_observed_at":"2026-08-05T08:24:16.854317Z","submitted_at":"2026-07-16T10:46:59Z","title":"SPH methods in the modelling of compact objects","version":1},"reference_index":134,"source":"arxiv_source","source_observed_at":"2026-08-02T01:02:18.453993Z"},"links":{"cited_paper":"/paper/1706.00417","citing_paper":"/paper/2607.14828"},"observation_digest":"sha256:4c50f6869382532e0ef7f173a34096f206517e0bafd9312418ea26992e8c4155","observation_id":"2e969633-6fb6-4bca-9832-cf97a216e3c6","resolution":{"observed_at":"2026-08-02T01:02:18.453993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1706.00417/citation-record","integrity":"/paper/1706.00417/integrity","json":"/paper/1706.00417/citation-record.json","paper":"/paper/1706.00417"},"outbound":[],"paper":{"arxiv_id":"1706.00417","last_updated":"2017-11-09T17:51:21Z","latest_version":2,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-07-06T05:45:13.627570Z","submitted_at":"2017-06-01T17:58:23Z","title":"Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1706.00417."}