Paper Citation Record · LEDGER

Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 25 inbound Pith citation observations for arXiv:1910.02914.

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pith.paper-citation-record.v1
1910.02914 v3

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measured 25 of 25 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 25 of 25 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:21:13.995774Z

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

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Pith citing papers

Observation 683b1608-78ef-494d-9dbf-29fb54721287 · inbound

The impact of braiding covariance and in-survey covariance on next-generation galaxy surveys cites this paper.

The impact of braiding covariance and in-survey covariance on next-generation galaxy surveys Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-14T05:43:51.116662Z

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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

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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

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Observation 4488c6ea-7c4a-4820-9d09-7cd967fc21d0 · inbound

Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis cites this paper.

Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-12T18:05:04.965758Z

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Observation 038fdfca-d1af-4d90-ac66-5186f2ab38e2 · inbound

Super sample covariance and the volume scaling of galaxy survey covariance matrices cites this paper.

Super sample covariance and the volume scaling of galaxy survey covariance matrices Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-12T12:45:52.955723Z

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Observation 9ada14fe-f227-4a4b-abba-79ec7d704848 · inbound

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure cites this paper.

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T22:24:26.883813Z

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Observation d3c597f3-fe5b-4078-8083-8a21f43afc6e · inbound

Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum cites this paper.

Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-11T19:40:39.094113Z

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Observation 618470ad-2e86-4b71-accd-6a21990ceea5 · inbound

Lyman Alpha Forest - Halo Cross-Correlations in Effective Field Theory cites this paper.

Lyman Alpha Forest - Halo Cross-Correlations in Effective Field Theory Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T21:32:52.473131Z

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Observation a5a43142-db51-4dce-85c1-2abfd1632102 · inbound

Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions cites this paper.

Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-09T22:58:54.755515Z

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Observation 3bca7ed6-9ff2-4299-b8f6-63160aaaa7b2 · inbound

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation cites this paper.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 152

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.995774Z

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Observation 7eddf521-29ff-4d9c-8f40-3b2233dc859f · inbound

Perturbative Likelihoods for Large-Scale Structure of the Universe cites this paper.

Perturbative Likelihoods for Large-Scale Structure of the Universe Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:15.923016Z

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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

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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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+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 2026-08-20T06:33:59.587034+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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+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 2026-08-20T06:33:59.587034+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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+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

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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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