Pith. sign in

Paper Citation Record · LEDGER

Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1405.0872.

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

pith.paper-citation-record.v1
1405.0872 v3

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 2026-08-04T06:34:03.388597+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T10:56:39.708614Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T08:05:16.230513Z

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 2f068e7c-d912-48d9-99e2-568da6202631 · inbound

Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions cites this paper.

Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-06-28T05:41:41.031105Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d5fef4e1434c0bbdcb0016776bc1c67b8b8fa636b6addb05ead0392e0042cfb8

Observation d569e072-319f-4140-a50e-94c9d0062c8b · 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 Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence

Reference 9

Resolution
verified exact
local_arxiv, observed 2026-06-27T06:50:39.949429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c4e7f511a2786014ea56870843f83738f9b1e025a2c2ec8800240e179134f54b

Observation 4750000d-bff1-4fe6-8792-432ce6afb4fc · inbound

Galactic Science with the LiteBIRD satellite: Spectral characterization of diffuse Galactic polarized emission at the angular power spectrum level cites this paper.

Galactic Science with the LiteBIRD satellite: Spectral characterization of diffuse Galactic polarized emission at the angular power spectrum level Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-01T10:56:39.708614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T10:56:39.708614Z digest=sha256:228e2c946f5317704a721c172ce9a370ecc7114ce46aeec479aa0cf1e7fc0703