Paper Citation Record · LEDGER

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis

As of 9 August 2026, this Paper Citation Record lists 22 of 22 outbound references and 0 inbound Pith citation observations for arXiv:2608.05504.

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

pith.paper-citation-record.v1
2608.05504 v1

Coverage vector

measured 22 of 22 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-08T12:03:04.970386Z

measured 22 of 22 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

22 of 22 outbound references displayed

verified exact3
verified fuzzy0
unresolved19
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 60e33bc4-feb8-4d9c-ab05-b31989e677bc · outbound

This paper cites Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.892202Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2888517b-86c5-4ff2-ad4b-90659f332a34 · outbound

This paper cites How to optimally combine pre-reconstruction full shape and post-reconstruction BAO signals.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis How to optimally combine pre-reconstruction full shape and post-reconstruction BAO signals

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.898750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 033e91b2-2763-4f2a-9d70-53d2e3db7d23 · outbound

This paper cites An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.904119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3df938d-6edd-4d1f-add0-79eab3efdb34 · outbound

This paper cites Extracting high-order cosmological information in galaxy surveys with power spectra.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Extracting high-order cosmological information in galaxy surveys with power spectra

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.908261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 147912ad-e2ba-4819-a2dd-9be7812a1e81 · outbound

This paper cites an unresolved cited work.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Unresolved cited work

Reference 5

Resolution: verified exact; raw_fallback, observed 2026-08-08T12:03:35.282594Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e45c28de-398e-4f80-a23d-02aed9f5bdcd · outbound

This paper cites Covariance of the redshift-space matter power spectrum after reconstruction.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Covariance of the redshift-space matter power spectrum after reconstruction

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-08-08T12:03:20.199590Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation a71f5281-9adc-42a1-86f4-c5654768424e · outbound

This paper cites Modelling the covariance matrix for the power spectra before and after the BAO reconstruction.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Modelling the covariance matrix for the power spectra before and after the BAO reconstruction

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.920331Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50025886-6f41-4a7a-928d-6576f57e9f62 · outbound

This paper cites Forecasting Cosmological Constraints from Redshift Surveys.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Forecasting Cosmological Constraints from Redshift Surveys

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.923913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09e6cd82-a22b-4423-b94a-79cea74ad125 · outbound

This paper cites Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.927608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2635497c-a768-4c17-99cf-3c3ebf3ed493 · outbound

This paper cites Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.931209Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 30e7218b-1cc4-4f66-928c-9d8e7234346d · outbound

This paper cites Chen et al.,Extensive analysis of reconstruction algorithms for DESI 2024 baryon acoustic oscillations,JCAP05(2026) 001 [2411.19738].

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Chen et al.,Extensive analysis of reconstruction algorithms for DESI 2024 baryon acoustic oscillations,JCAP05(2026) 001 [2411.19738]

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.934372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9ccba31b-9368-4c74-bb3e-b210635e28d0 · outbound

This paper cites Developing a Theoretical Model for the Resummation of Infrared Effects in the Post-Reconstruction Power Spectrum (an explanatory video is available in the comments section).

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Developing a Theoretical Model for the Resummation of Infrared Effects in the Post-Reconstruction Power Spectrum (an explanatory video is available in the comments section)

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.937003Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 328bb442-cf9b-4491-9faa-9ae9defdeddb · outbound

This paper cites Angular power spectrum of galaxies in the 2MASS Redshift Survey.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Angular power spectrum of galaxies in the 2MASS Redshift Survey

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.939842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d1ea5c3c-75e9-4243-90d6-7c6c3e1d0080 · outbound

This paper cites Emulating power spectra for pre- and post-reconstructed galaxy samples.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Emulating power spectra for pre- and post-reconstructed galaxy samples

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.942547Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 595a3e53-4991-4bb2-85d2-5b7b09fd7f09 · outbound

This paper cites Dark matter statistics for large galaxy catalogs: power spectra and covariance matrices.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Dark matter statistics for large galaxy catalogs: power spectra and covariance matrices

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.945609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 289fdb04-f1e0-46b8-9851-fe8b2222abb2 · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modeling of the luminosity and colour dependence in the Data Release 10.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modeling of the luminosity and colour dependence in the Data Release 10

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-08-08T12:03:05.064975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 4f13c3f6-7d66-48d6-a6e1-39f4dd6f53f7 · outbound

This paper cites The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Including covariance matrix errors.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Including covariance matrix errors

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.952656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c24b79ea-55d5-4b36-87b9-27e1654b7ef6 · outbound

This paper cites Power Spectrum Correlations Induced by Non-Linear Clustering.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Power Spectrum Correlations Induced by Non-Linear Clustering

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.956163Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c187461d-55e4-4208-876e-924266fa350b · outbound

This paper cites Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.959634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbe20ebd-fafb-47e0-a99d-fc40c148aa9c · outbound

This paper cites Sample Variance Considerations for Cluster Surveys.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Sample Variance Considerations for Cluster Surveys

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.963245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 329f5f22-eb6b-4708-934d-aac95e619bcf · outbound

This paper cites Power Spectrum Super-Sample Covariance.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Power Spectrum Super-Sample Covariance

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.966809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 662177b8-acc7-486c-8b98-b40b5699eb88 · outbound

This paper cites Disconnected Covariance of 2-point Functions in Large-Scale Structure.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Disconnected Covariance of 2-point Functions in Large-Scale Structure

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-08T12:03:04.970386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

No inbound Pith citation observations are available.