Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2405.13121.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:33:59.559197Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T22:17:40.827256Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 5762ee8c-3f1d-4ebb-a027-896bb509ae7b · inbound
Energy-Dependent Transport of Cosmic Rays in the Multiphase, Dynamic Interstellar Medium cites this paper.
Energy-Dependent Transport of Cosmic Rays in the Multiphase, Dynamic Interstellar Medium Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:32:50.458557Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c2032a22-8d1e-40f8-8101-b4f234d9b799 · inbound
Modeling Cosmic Ray Electron Spectra and Synchrotron Emission in the Multiphase ISM cites this paper.
Modeling Cosmic Ray Electron Spectra and Synchrotron Emission in the Multiphase ISM Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
Reference 102
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:33:59.559197Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 35a15761-8092-48c2-9a6b-b395c93af54c · inbound
Dynamically Controlled Transport of GeV Cosmic Rays in Diverse Galactic Environments cites this paper.
Dynamically Controlled Transport of GeV Cosmic Rays in Diverse Galactic Environments Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T10:58:01.766607Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb01299b-4a0b-4d73-838f-cdd40b95a7b2 · inbound
CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra cites this paper.
CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
Reference 238
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T22:17:40.841948Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation f7440442-0d52-432e-9c06-51e9587cd0ad · inbound
CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.
CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
Reference 175
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:26:50.805003Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a6e4e2ff-1c7e-48e7-a035-3620a178b395 · inbound
Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies cites this paper.
Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
Reference 145
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T14:25:22.203819Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.