Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2311.04365.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T17:11:32.115794Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T17:11:32.417036Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 8c5a030b-76bf-4a27-a7cd-9fda73e1cebe · inbound
Why Wide Jupiter-Mass Binary-Objects Cannot Form cites this paper.
Why Wide Jupiter-Mass Binary-Objects Cannot Form Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux
Reference 11
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-06T17:11:32.422082Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.