Pith. sign in

Paper Citation Record · LEDGER

Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2505.03737.

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

pith.paper-citation-record.v1
2505.03737 v2

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 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:18:11.286997Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T09:39:46.286336Z

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 96416992-4e3f-4661-b44c-c528840cc810 · inbound

The Atacama Cosmology Telescope: High-redshift measurement of structure growth from the cross-correlation of Quaia quasars and CMB lensing from ACT DR6 and $\textit{Planck}$ PR4 cites this paper.

The Atacama Cosmology Telescope: High-redshift measurement of structure growth from the cross-correlation of Quaia quasars and CMB lensing from ACT DR6 and $\textit{Planck}$ PR4 Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-06T18:18:11.286997Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:18:11.286997Z digest=sha256:c93fb1865d084d9e10744dd8e2737236c7d6a212abaac1e5eec387e5ccc20455

Observation 5021ee52-372e-4513-868a-729aa58e8f3d · inbound

Non-Gaussianity in SMICA cites this paper.

Non-Gaussianity in SMICA Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements

Reference 24

Resolution
verified exact
arxiv_id, observed 2026-05-21T18:50:29.416539Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-21T18:49:55.245811Z digest=sha256:65da3fb1dd830c0fce0bab5092490526f776372e0ba7ed7127614f0da6771fc4

Observation 0023c135-f830-4d5d-82c8-e1a3c55e7f98 · inbound

Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales cites this paper.

Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements

Reference 11

Resolution
verified exact
arxiv_id, observed 2026-07-04T09:39:46.287658Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-26T09:46:24.839336Z digest=sha256:199d338667e0b133437d7bfe1ee5693bde6e186d11e693794e6418d5fecc1e66