Paper Citation Record · LEDGER

Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:1910.02914.

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

pith.paper-citation-record.v1
1910.02914 v3

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measured 0 of 0 reference resolution

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measured 16 of 16 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:55:49.481592Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T18:10:01.426141Z

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Outbound references

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Pith citing papers

Observation 21ef25a8-ce81-464c-a59a-50bb0d74757a · inbound

DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars cites this paper.

DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 135

Resolution: verified exact; arxiv_id, observed 2026-05-17T06:34:54.726593Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 7994513d-7b1b-48bf-99cc-36e50ad7b60d · inbound

DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars cites this paper.

DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 163

Resolution: verified exact; arxiv_id, observed 2026-05-17T06:00:50.000671Z

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No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 6abadf9a-93dd-4e47-b15a-f3b076b84a7b · inbound

Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation cites this paper.

Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-07T05:55:49.481592Z

Source-reported events for the cited work

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Observation 19fa704c-16eb-447b-80e8-ed3d6e9ee1dc · inbound

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys cites this paper.

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 122

Resolution: unresolved; no resolver link, observed 2026-08-07T04:21:40.113892Z

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Observation f34d0ed0-346a-4352-899d-599c0c120040 · inbound

Equivalence of the field-level inference and conventional analyses on large scales cites this paper.

Equivalence of the field-level inference and conventional analyses on large scales Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T19:34:09.536018Z

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Observation 4a4b3aae-454a-4e79-ac7a-4f977a7277ec · inbound

Fiducial-Cosmology-dependent systematics for the DESI 2024 Full-Shape Analysis cites this paper.

Fiducial-Cosmology-dependent systematics for the DESI 2024 Full-Shape Analysis Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-04T21:28:55.555202Z

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Observation 1c2ef50f-1390-4005-9caf-dfe4f4d6bb0a · inbound

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum cites this paper.

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 111

Resolution: unresolved; no resolver link, observed 2026-08-03T22:43:50.493651Z

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Observation 1e6ef5b1-f2db-4b0c-b620-06b15ea3f7c5 · inbound

The Linear Point Standard Ruler with DESI DR1 and DR2 Data cites this paper.

The Linear Point Standard Ruler with DESI DR1 and DR2 Data Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-04T06:27:26.358991Z

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Observation 3fb7f0fc-5d9c-4a99-93e8-14cd4d997984 · inbound

Large-scale Modeling of the Observed Power Spectrum Multipoles cites this paper.

Large-scale Modeling of the Observed Power Spectrum Multipoles Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-04T06:23:26.444533Z

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Observation bf5d9977-8cab-4253-931f-813b57491940 · inbound

Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope cites this paper.

Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-05-10T10:49:57.076131Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation d64b4cd2-3f12-4888-a22c-588f694c98b4 · inbound

If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics cites this paper.

If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 7

Resolution: verified exact; arxiv_id, observed 2026-05-11T12:31:06.871653Z

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No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation bf128e07-a6ba-412b-9aa6-ddf08c41322a · inbound

Fewer simulations, sharper covariances: Reducing mock covariance noise with Zeldovich approximation control variates cites this paper.

Fewer simulations, sharper covariances: Reducing mock covariance noise with Zeldovich approximation control variates Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-06-29T13:33:28.711081Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 990e3bb2-08d2-4f03-92e8-79fdd8c303e0 · inbound

The 3D clustering of Lyman Alpha Emitters measured with DESI cites this paper.

The 3D clustering of Lyman Alpha Emitters measured with DESI Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 82

Resolution: verified exact; arxiv_id, observed 2026-07-04T18:10:01.427687Z

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No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 2f1ca262-0248-4311-96ab-d77d27c31705 · inbound

How I stop worrying about non-universality and $b_\phi$: Constraining local $f_{\rm NL}$ with $b_\phi$ priors from HOD posteriors cites this paper.

How I stop worrying about non-universality and $b_\phi$: Constraining local $f_{\rm NL}$ with $b_\phi$ priors from HOD posteriors Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-07-03T18:58:50.543231Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation f12540f0-e8eb-4614-bc34-288291078c13 · inbound

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 207

Resolution: unresolved; no resolver link, observed 2026-07-14T14:25:37.540627Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15c2b8b3-db05-4e23-a018-875ec3eaf6cb · inbound

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 213

Resolution: unresolved; no resolver link, observed 2026-08-02T07:33:01.287829Z

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Unavailable: canonical work link unavailable.