Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The maximum accretion rate of a protoplanet: how fast can runaway be?
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2305.01684.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T10:51:27.490103Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T13:55:05.277451Z
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 6cbe8958-4a62-4252-ac61-661b63411a1e · inbound
Correlation between planet formation rate and gas surface density: an analog of Kennicutt Schmidt law for planet formation cites this paper.
Correlation between planet formation rate and gas surface density: an analog of Kennicutt Schmidt law for planet formation The maximum accretion rate of a protoplanet: how fast can runaway be?
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T10:51:27.490103Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 14dd309f-52aa-40c4-88b8-5967066772ba · inbound
Effects of Thermodynamics on the Concurrent Accretion and Migration of Gas Giants in Protoplanetary Disks cites this paper.
Effects of Thermodynamics on the Concurrent Accretion and Migration of Gas Giants in Protoplanetary Disks The maximum accretion rate of a protoplanet: how fast can runaway be?
Reference 34
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T13:55:05.282202Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.