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Paper Citation Record · LEDGER

A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.14596.

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

pith.paper-citation-record.v1
2407.14596 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 2026-08-20T06:33:59.587034+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:59:43.051437Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T12:16:16.480190Z

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 84a21e9b-dc4f-4cb2-abe1-bb3598ba6586 · inbound

Polarized Dust Emission in Arp220: Magnetic Fields in the Core of an Ultraluminous Infrared Galaxy cites this paper.

Polarized Dust Emission in Arp220: Magnetic Fields in the Core of an Ultraluminous Infrared Galaxy A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:59:43.512872Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-11T11:59:43.051437Z digest=sha256:d2847958dd6e2f19e8be213c6d80e44528d4b43e0362ec01177f24e47b07d6e0

Observation 4b96dee4-a35f-41ca-9e30-a28d8ad1d1e6 · inbound

Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies cites this paper.

Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6

Reference 33

Resolution
unresolved
no resolver link, observed 2026-07-31T14:25:21.919253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T14:25:21.919253Z digest=sha256:d57ae087288032040e699ba351f5b569da13ab53d5b2c049f776a55f3250321e