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Paper Citation Record · LEDGER

Radiative hydrodynamics simulations of red supergiant stars. IV gray versus non-gray opacities

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1109.3619.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1109.3619 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:00:24.060663Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-12T17:12:21.729017Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b6a9e19f-644f-45f0-a54b-9f2d15eba4c2 · inbound

Numerical Simulations of Cosmic-Ray Acceleration at Core-Collapse Supernovae cites this paper.

Numerical Simulations of Cosmic-Ray Acceleration at Core-Collapse Supernovae Radiative hydrodynamics simulations of red supergiant stars. IV gray versus non-gray opacities

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-14T15:00:24.060663Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T15:00:24.060663Z digest=sha256:60def89f9a5dc60399f0e6c13c95f00f0d5a65161a56b46ba1b50d71f75f40a5

Observation b7ac6dbf-3858-44c0-993d-29f77baf761b · inbound

Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter cites this paper.

Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter Radiative hydrodynamics simulations of red supergiant stars. IV gray versus non-gray opacities

Reference 5

Resolution
verified exact
local_arxiv, observed 2026-08-12T17:12:21.732862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-12T17:12:21.128325Z digest=sha256:8357897e4c0b5cdbdee0be58927b6e1b922178220d4102950625a394d7faccaf

Observation 23c8a5ef-6e5c-43c4-89b9-d26847cfd725 · inbound

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae cites this paper.

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae Radiative hydrodynamics simulations of red supergiant stars. IV gray versus non-gray opacities

Reference 120

Resolution
unresolved
no resolver link, observed 2026-08-03T23:48:58.181657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:48:58.181657Z digest=sha256:b1a155b73639eea5a271c337a2377b53e88e025ae795d820a53827fa09049a0c