Paper Citation Record · LEDGER

How to measure CMB power spectra without losing information

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/9611174.

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

pith.paper-citation-record.v1
astro-ph/9611174 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T14:47:48.499887Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T18:21:55.730648Z

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Outbound references

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Pith citing papers

Observation 84d61203-8286-499e-929d-5c693c52c231 · inbound

Window convolution of the galaxy clustering bispectrum cites this paper.

Window convolution of the galaxy clustering bispectrum How to measure CMB power spectra without losing information

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-12T14:47:48.499887Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 19f29736-9c7d-48df-8928-a4a2b2b4cb45 · inbound

DeepWiener: Neural Networks for CMB polarization maps and power spectrum computation cites this paper.

DeepWiener: Neural Networks for CMB polarization maps and power spectrum computation How to measure CMB power spectra without losing information

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T15:57:41.012365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9f411da-aa9e-43be-9fd5-d8732934a980 · inbound

The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey cites this paper.

The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey How to measure CMB power spectra without losing information

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-09T17:15:38.765235Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f82e703-07f1-4fe6-b246-78bf4147bc24 · inbound

Constraints on primordial non-Gaussianity from Quaia cites this paper.

Constraints on primordial non-Gaussianity from Quaia How to measure CMB power spectra without losing information

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-05-22T18:21:55.732776Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation c75a1f1c-b1b2-487d-8bc5-0c40a77485df · inbound

A unified harmonic framework for dark siren cosmology cites this paper.

A unified harmonic framework for dark siren cosmology How to measure CMB power spectra without losing information

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-05-15T11:30:31.180394Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation d9764d1d-a5ff-42ec-809c-6c1d38c5f3e9 · inbound

Searching for Population III stars with line intensity mapping cross-correlations cites this paper.

Searching for Population III stars with line intensity mapping cross-correlations How to measure CMB power spectra without losing information

Reference 133

Resolution: unresolved; no resolver link, observed 2026-08-03T00:21:45.621206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.