Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1201.4263.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T12:59:58.251850Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T14:02:16.870748Z
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 c3c5e782-478f-454c-87b0-a848e63e7ae1 · inbound
Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A cites this paper.
Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
Reference 99
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-23T05:55:27.482917Z
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.
Observation c4ce1632-52a1-42c0-85a1-1adc7e01483f · 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 Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
Reference 192
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T14:02:16.873016Z
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.
Observation c5c04c99-17b3-4b36-be76-4e2ef27dfe45 · inbound
Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps cites this paper.
Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T07:49:08.568355Z
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.
Observation 857ba2fc-e234-4543-a52a-b517c266cddf · inbound
ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 cites this paper.
ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
Reference 114
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T12:59:58.251850Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.