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Paper Citation Record · LEDGER

CMB Power Asymmetry from Non-Gaussian Modulation

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1210.2965.

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

pith.paper-citation-record.v1
1210.2965 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 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:09:03.264750Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

70
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation fd8c21f8-8d5f-4a7a-bad7-bb88dae87e27 · inbound

Probing dipolar power asymmetry with galaxy clustering and intrinsic alignments cites this paper.

Probing dipolar power asymmetry with galaxy clustering and intrinsic alignments CMB Power Asymmetry from Non-Gaussian Modulation

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-07T14:09:03.264750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:09:03.264750Z digest=sha256:c13e3752472a75ca1d5375ce2870d82161fed686160f19ef2422ba2a1aec948f

Observation 44e27ec7-7daf-408f-993a-bfcfdbdb7061 · inbound

Constraining Scale-Dependent Growth in $f(R)$ Gravity with Future 21 cm Surveys cites this paper.

Constraining Scale-Dependent Growth in $f(R)$ Gravity with Future 21 cm Surveys CMB Power Asymmetry from Non-Gaussian Modulation

Reference 96

Resolution
verified exact
local_arxiv, observed 2026-06-28T08:41:48.604469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:25e5362640c33b4bc0849a02be90373eed4b5c7c715c8f17fa88c94831a74251

Observation c61f670e-c47a-46d3-9208-acfecccc7a3f · inbound

Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum cites this paper.

Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum CMB Power Asymmetry from Non-Gaussian Modulation

Reference 107

Resolution
verified exact
local_arxiv, observed 2026-07-01T17:55:52.352174Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-29T02:50:45.187677Z digest=sha256:32194de6f4c4ac3d9c1cf8479bf634e1ffab126cfa140d78cbab85c53d0e91cc