Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport. I. Stochastic Fragmentation with Optical-depth-dependent Rate and Universal Fragment Mass
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2410.12042.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:24:08.915606Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
3
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 87f4dd46-f87f-44b3-a9e7-e0cc1cb16eaf · inbound
Formation of Giant Planets cites this paper.
Formation of Giant Planets Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport. I. Stochastic Fragmentation with Optical-depth-dependent Rate and Universal Fragment Mass
Reference 161
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:24:08.915606Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e85b07e6-178d-4d9d-9b67-3e75b9c074ac · inbound
VLT/ERIS observations of the V960 Mon system: a dust-embedded substellar object formed by gravitational instability? cites this paper.
VLT/ERIS observations of the V960 Mon system: a dust-embedded substellar object formed by gravitational instability? Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport. I. Stochastic Fragmentation with Optical-depth-dependent Rate and Universal Fragment Mass
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:27:55.828391Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7ddc8a72-94cf-4ffe-b72b-52645c053b26 · inbound
Does magnetic field promote or suppress fragmentation in AGN disks? Results from local shearing box simulations with simple cooling cites this paper.
Does magnetic field promote or suppress fragmentation in AGN disks? Results from local shearing box simulations with simple cooling Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport. I. Stochastic Fragmentation with Optical-depth-dependent Rate and Universal Fragment Mass
Reference 51
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T12:18:55.827853Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 45d0605a-995e-45ba-89f7-36f45b0c60c8 · inbound
Dust growth and planet formation by disc fragmentation cites this paper.
Dust growth and planet formation by disc fragmentation Global Simulations of Gravitational Instability in Protostellar Disks with Full Radiation Transport. I. Stochastic Fragmentation with Optical-depth-dependent Rate and Universal Fragment Mass
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T19:31:04.504347Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.