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Paper Citation Record · LEDGER

Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1608.02601.

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

pith.paper-citation-record.v1
1608.02601 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 2026-08-06T06:34:29.942622+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T16:43:10.179035Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T01:20:20.630779Z

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 ac4f3285-2575-4e86-a364-1f492c1b76ac · inbound

The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky cites this paper.

The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field

Reference 261

Resolution
metadata mismatch
local_arxiv, observed 2026-05-19T21:03:18.624062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b8ad1ab70a39826aef3ec6e748202ac06789e179660e5ab972c3be53b989c7c0

Observation 0c837554-37d7-4120-ad4f-35ffe8dbc541 · inbound

The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky cites this paper.

The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field

Reference 261

Resolution
metadata mismatch
local_arxiv, observed 2026-05-21T09:14:05.169526Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8e4384b5d0ca38fb67522cbeab50851d0bd715570454a923237387a61f0fd449

Observation f93488bb-7f01-4502-8b8b-4fafef4aae14 · inbound

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds cites this paper.

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field

Reference 233

Resolution
verified exact
local_arxiv, observed 2026-06-27T01:20:20.632116Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:21d50867525575bc24ba425bacd904fc7acd390ff02882dc378b6e7f91a1a28c

Observation 747b2842-ad45-4991-b7df-6c73fca8bbd7 · inbound

Exploring the Galactic plasma with pulsars in the SKA Era cites this paper.

Exploring the Galactic plasma with pulsars in the SKA Era Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field

Reference 81

Resolution
unresolved
no resolver link, observed 2026-07-12T08:30:18.472851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T08:30:18.472851Z digest=sha256:de20371f6a2a3e3ce0aaf9ce1ae1d7ac09fce1c4000cc604fd71b523a76d0a01

Observation 2cb6a841-7dbd-4788-90fb-a80131abc907 · inbound

Exploring the Galactic plasma with pulsars in the SKA Era cites this paper.

Exploring the Galactic plasma with pulsars in the SKA Era Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field

Reference 81

Resolution
unresolved
no resolver link, observed 2026-07-14T16:43:10.179035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T16:43:10.179035Z digest=sha256:2108f3315160d78428fe7bcedf7dbdf762d09dca5087dff661dab16a4d855272