Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
As of 20 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1701.07028.
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 2026-07-19T06:30:13.599613+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T22:17:39.411055Z
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 4297da6e-bab0-46f4-aaa4-78a5acfd3cba · inbound
Magnetised CGM Gas at z~1 revealed by SPICE-RACS cites this paper.
Magnetised CGM Gas at z~1 revealed by SPICE-RACS Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
Reference 123
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T20:57:46.333131Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.
Observation 70116fed-aeed-40e7-9fed-7b7c495f4bea · 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 formation in the Milky Way-like disk galaxies of the Auriga project
Reference 273
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T14:02:16.608939Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.
Observation ed63cdc8-3ed6-4ac9-9e92-82e947de3aab · inbound
Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures cites this paper.
Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
Reference 69
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T15:21:00.473177Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.
Observation a6f902a0-3e0e-44bc-aaad-85e59dac7191 · inbound
Introducing AuriGLOBES: the effect of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters cites this paper.
Introducing AuriGLOBES: the effect of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
Reference 79
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T01:45:14.331066Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.
Observation d13f18dd-a760-4b7a-82e4-dbbb00121fff · 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 Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
Reference 87
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T22:17:39.432277Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.