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Paper Citation Record · LEDGER

Launching cosmic-ray-driven outflows from the magnetized interstellar medium

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1509.07247.

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

pith.paper-citation-record.v1
1509.07247 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T22:21:53.091949Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T22:17:40.024110Z

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 a98d918c-40a1-4da7-9c23-4808781d3678 · inbound

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Reference 162

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T08:11:16.391586Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:47a980c5e0d5c72554963818c0e91ad49bad0c4eaaa6ea4e31e2c50a0aa38f4b

Observation 2ddf873f-330f-45be-be89-4405c5491c30 · inbound

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds cites this paper.

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Reference 293

Resolution
unresolved
no resolver link, observed 2026-07-11T06:21:15.541076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:21:15.541076Z digest=sha256:270a773f56ac4bb917b889b510af580446b5b40d64d17a7fa001f67f14656cd5

Observation f4d6672c-437b-4ae3-a8d0-2d1f5b044ee2 · 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 Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Reference 175

Resolution
verified exact
local_arxiv, observed 2026-07-10T22:17:40.043789Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ac9962aa773d8d0b9034787661654fb28a4721aa7f9fd2f00fec5ab7ddcf455a

Observation 5d1deb0e-3e11-4871-aeb7-61b36ef0c50d · inbound

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Reference 1

Resolution
unresolved
no resolver link, observed 2026-07-13T06:20:04.707661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:20:04.707661Z digest=sha256:a99f039cf7e05e1836b1fb526d9fdb3fe038f95e3cdda8b061e856f990614e1d

Observation ab01d8fa-8d6b-4a6a-bd73-208b3a9734f6 · inbound

A cosmic-ray loaded nascent outflow driven by a massive star cluster cites this paper.

A cosmic-ray loaded nascent outflow driven by a massive star cluster Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-01T22:21:53.091949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T22:21:53.091949Z digest=sha256:b471901e9935757986f404c559e87e8a36b2c6370875acb1efed2f56e8a2e22c