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Paper Citation Record · LEDGER

Magnetic Field Strengths and Grain Alignment Variations in the Local Bubble Wall

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1901.07692.

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

pith.paper-citation-record.v1
1901.07692 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 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:30:21.778193Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T14:02:16.592898Z

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 2b37b749-80ee-4aaa-af44-38469c0a0b02 · inbound

Analyzing Stellar and Interstellar Contributions to Polarization: Modeling Approaches for Hot Stars cites this paper.

Analyzing Stellar and Interstellar Contributions to Polarization: Modeling Approaches for Hot Stars Magnetic Field Strengths and Grain Alignment Variations in the Local Bubble Wall

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-07T15:30:21.778193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T15:30:21.778193Z digest=sha256:69ffa30dd53da66fb252fbcc6f3cc2bdbf943fb75280f4ea69a444eae3656a2f

Observation 98ced87f-85dd-48ef-b190-72aead8dcadc · inbound

The magnetic field of the Milky Way: an observational perspective cites this paper.

The magnetic field of the Milky Way: an observational perspective Magnetic Field Strengths and Grain Alignment Variations in the Local Bubble Wall

Reference 235

Resolution
verified exact
local_arxiv, observed 2026-06-28T14:02:16.595866Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8016ffcaf9953f605175741b2fe2397c8d4ed166b4d9896a36f7355d1fa354c9

Observation 19a406d8-e606-442c-908e-48d2a422c726 · inbound

Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra cites this paper.

Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra Magnetic Field Strengths and Grain Alignment Variations in the Local Bubble Wall

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-06-27T06:50:39.882692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:88aa079c22503d04ed231427dc3ba67f4a2f10cedf0a3b9f8ae290a83ec7a333