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Paper Citation Record · LEDGER

Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.00148.

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

pith.paper-citation-record.v1
2410.00148 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T20:03:39.020602Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-08T20:03:39.103171Z

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 d3c2a051-c7e0-4444-8859-2962e2520527 · inbound

Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei cites this paper.

Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars

Reference 33

Resolution
metadata mismatch
local_arxiv, observed 2026-08-08T20:03:39.108956Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-08-08T20:03:39.020602Z digest=sha256:7208cf0e038d337731604ba35f0595e490fad783c43fd954b2a502e36434dee1

Observation 9bdad221-8a54-42d1-b528-33e0eb53d392 · inbound

Something new under the Sun: A magnetically driven CH/CN anti-correlation cites this paper.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.262025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.262025Z digest=sha256:ea7af54b96c2f304fc88fe0caeca7b30abaaac2c4c9dc14d59ca5fdef0333dbb