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Paper Citation Record · LEDGER

ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2406.14519.

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

pith.paper-citation-record.v1
2406.14519 v1

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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T23:51:27.632793Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T09:39:46.369341Z

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 26f9fb9f-6bb4-4980-b272-971b89dc5de3 · inbound

Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements cites this paper.

Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-15T23:51:27.632793Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T23:51:27.632793Z digest=sha256:39498524539deb035647567e0da3fb703ec0a477bb1fdf2454b58f0f97d3feae

Observation f27ce377-49b7-4775-824e-741a2d562eec · 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 ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network

Reference 10

Resolution
malformed identifier
arxiv_id, observed 2026-07-04T09:39:46.370726Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-26T09:46:24.839336Z digest=sha256:92093ad59a0744fce58ae1a78537f3b45541e56132dda97748bee720906cb954