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Paper Citation Record · LEDGER

Sample Variance Cancellation for Future Spectroscopic Surveys

As of 10 August 2026, this Paper Citation Record lists 45 of 45 outbound references and 0 inbound Pith citation observations for arXiv:2608.07339.

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

pith.paper-citation-record.v1
2608.07339 v1

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measured 45 of 45 reference resolution

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Outbound references

Observation b5a7d0df-7e05-485d-b66e-7d80642736bb · outbound

This paper cites Collaboration, A.

Sample Variance Cancellation for Future Spectroscopic Surveys Collaboration, A

Reference 1

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Observation e67a3ba7-8314-4c8f-8b3e-3fc413cbb753 · outbound

This paper cites Collaboration, A.

Sample Variance Cancellation for Future Spectroscopic Surveys Collaboration, A

Reference 2

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Observation acd3585a-a060-4494-97d5-691b9e1bdac6 · outbound

This paper cites Laureijs, J.

Sample Variance Cancellation for Future Spectroscopic Surveys Laureijs, J

Reference 3

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Observation 5139c42a-d091-44f1-97a7-13b800ca7cbc · outbound

This paper cites Amendola, S.

Sample Variance Cancellation for Future Spectroscopic Surveys Amendola, S

Reference 4

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Observation 993b2c8b-1571-46ae-801b-4e8fc79ad74e · outbound

This paper cites Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS).

Sample Variance Cancellation for Future Spectroscopic Surveys Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)

Reference 5

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Observation fa95b809-9488-4cee-adec-048f2d136676 · outbound

This paper cites WST -- Widefield Spectroscopic Telescope: Motivation, science drivers and top-level requirements for a new dedicated facility.

Sample Variance Cancellation for Future Spectroscopic Surveys WST -- Widefield Spectroscopic Telescope: Motivation, science drivers and top-level requirements for a new dedicated facility

Reference 6

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Observation 796624b6-9151-40ed-8231-0f182e9e0613 · outbound

This paper cites Besuner, A.

Sample Variance Cancellation for Future Spectroscopic Surveys Besuner, A

Reference 7

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Observation b401e5fa-eeae-4acf-8a9d-1433e09a5d96 · outbound

This paper cites Kaiser,Clustering in real space and in redshift space, MNRAS227(1987) 1.

Sample Variance Cancellation for Future Spectroscopic Surveys Kaiser,Clustering in real space and in redshift space, MNRAS227(1987) 1

Reference 8

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Observation 7689cc76-e08e-457d-b926-af6094e92f5e · outbound

This paper cites Radiative Transfer Modeling of Lyman Alpha Emitters. II. New Effects in Galaxy Clustering.

Sample Variance Cancellation for Future Spectroscopic Surveys Radiative Transfer Modeling of Lyman Alpha Emitters. II. New Effects in Galaxy Clustering

Reference 9

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Observation 2d4285e3-5918-4a77-9a6f-b44ff678e8f0 · outbound

This paper cites The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation.

Sample Variance Cancellation for Future Spectroscopic Surveys The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation

Reference 11

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Observation 6a5f0def-1ce6-4434-bd02-f26cbe99f6c2 · outbound

This paper cites Ly{\alpha} emitters in a cosmological volume I: the impact of radiative transfer.

Sample Variance Cancellation for Future Spectroscopic Surveys Ly{\alpha} emitters in a cosmological volume I: the impact of radiative transfer

Reference 12

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Observation 2863076a-0276-449f-af1e-156dbc111c53 · outbound

This paper cites Catch Me if You Can: Biased Distribution of Ly$\alpha$-emitting Galaxies according to the Viewing Direction.

Sample Variance Cancellation for Future Spectroscopic Surveys Catch Me if You Can: Biased Distribution of Ly$\alpha$-emitting Galaxies according to the Viewing Direction

Reference 13

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Observation 64a6cb0e-4a14-4156-8fdd-163139bd1365 · outbound

This paper cites Khoraminezhad, S.

Sample Variance Cancellation for Future Spectroscopic Surveys Khoraminezhad, S

Reference 14

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Observation 3f95c14c-78d8-44b1-a254-f2bd18ffc090 · outbound

This paper cites Lyman-alpha emitters in a cosmological volume II: the impact of the intergalactic medium.

Sample Variance Cancellation for Future Spectroscopic Surveys Lyman-alpha emitters in a cosmological volume II: the impact of the intergalactic medium

Reference 15

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Observation 15512f9b-5ac0-4bb9-80cc-8e1dbe7c5033 · outbound

This paper cites Measuring primordial non-gaussianity without cosmic variance.

Sample Variance Cancellation for Future Spectroscopic Surveys Measuring primordial non-gaussianity without cosmic variance

Reference 16

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Observation 66c4d992-9e18-4e58-8c99-8e706c67c006 · outbound

This paper cites How to measure redshift-space distortions without sample variance.

Sample Variance Cancellation for Future Spectroscopic Surveys How to measure redshift-space distortions without sample variance

Reference 17

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Observation ef0bcf35-e8f1-4d3d-bba0-e273fddb0a81 · outbound

This paper cites Fourier analysis of multi-tracer cosmological surveys.

Sample Variance Cancellation for Future Spectroscopic Surveys Fourier analysis of multi-tracer cosmological surveys

Reference 18

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Observation 21c0d1eb-ab50-4d55-a200-f4430818be28 · outbound

This paper cites Rubiola, S.

Sample Variance Cancellation for Future Spectroscopic Surveys Rubiola, S

Reference 19

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Observation 0a352802-50af-4235-b4a6-a265859e26db · outbound

This paper cites The Effective Field Theory of Large-Scale Structure and Multi-tracer.

Sample Variance Cancellation for Future Spectroscopic Surveys The Effective Field Theory of Large-Scale Structure and Multi-tracer

Reference 20

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Observation 7ff50a3f-4343-4365-b6bf-ad6ff347ca23 · outbound

This paper cites Rubira and F.

Sample Variance Cancellation for Future Spectroscopic Surveys Rubira and F

Reference 21

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Observation ced8cb65-5316-440f-b81d-e5fc0674a513 · outbound

This paper cites Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias.

Sample Variance Cancellation for Future Spectroscopic Surveys Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias

Reference 22

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Observation b3983851-f17e-40d8-becc-9ddd0c3291f2 · outbound

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Sample Variance Cancellation for Future Spectroscopic Surveys Towards optimal and robust $f_{\rm NL}$ constraints with multi-tracer analyses

Reference 23

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Observation cffa7e5d-7d00-4cbe-a72f-af6442ababa4 · outbound

This paper cites Taming assembly bias for primordial non-Gaussianity.

Sample Variance Cancellation for Future Spectroscopic Surveys Taming assembly bias for primordial non-Gaussianity

Reference 24

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Observation 0dfd9fcc-5319-40a9-bd37-9b4d12ba95f7 · outbound

This paper cites Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation.

Sample Variance Cancellation for Future Spectroscopic Surveys Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation

Reference 25

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Observation ccfcc67d-5b7b-44d3-ac0d-41a41f1ff7f1 · outbound

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Sample Variance Cancellation for Future Spectroscopic Surveys The Galaxy Power Spectrum and Bispectrum in Redshift Space

Reference 26

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Observation 9f31ab48-8f13-4b86-8ae0-97fa7588f8b4 · outbound

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Sample Variance Cancellation for Future Spectroscopic Surveys The clustering of Lyman Alpha Emitting galaxies at z=2-3

Reference 27

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Sample Variance Cancellation for Future Spectroscopic Surveys High redshift LBGs from deep broadband imaging for future spectroscopic surveys

Reference 28

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Sample Variance Cancellation for Future Spectroscopic Surveys High-redshift Millennium and Astrid galaxies in effective field theory at the field level

Reference 29

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This paper cites Planck 2015 results. XIII. Cosmological parameters.

Sample Variance Cancellation for Future Spectroscopic Surveys Planck 2015 results. XIII. Cosmological parameters

Reference 30

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Sample Variance Cancellation for Future Spectroscopic Surveys Measuring the galaxy power spectrum with future redshift surveys

Reference 31

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This paper cites Towards Optimal Measurement of Power Spectra I: Minimum Variance Pair Weighting and the Fisher Matrix.

Sample Variance Cancellation for Future Spectroscopic Surveys Towards Optimal Measurement of Power Spectra I: Minimum Variance Pair Weighting and the Fisher Matrix

Reference 32

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This paper cites Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?.

Sample Variance Cancellation for Future Spectroscopic Surveys Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?

Reference 33

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Observation d8206415-6dcc-4101-aa78-921d8b1d93a4 · outbound

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Sample Variance Cancellation for Future Spectroscopic Surveys Estimating the Power Spectrum of the Cosmic Microwave Background

Reference 34

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Observation 481539e7-d1d8-493d-b027-48b7a316b170 · outbound

This paper cites Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum.

Sample Variance Cancellation for Future Spectroscopic Surveys Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum

Reference 35

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Sample Variance Cancellation for Future Spectroscopic Surveys Towards optimal extraction of cosmological information from nonlinear data

Reference 36

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Observation 586f8f66-c11b-45b6-8893-77d86caf4864 · outbound

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

Sample Variance Cancellation for Future Spectroscopic Surveys The 3D clustering of Lyman Alpha Emitters measured with DESI

Reference 37

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Sample Variance Cancellation for Future Spectroscopic Surveys Cosmology before noon with multiple galaxy populations

Reference 38

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Sample Variance Cancellation for Future Spectroscopic Surveys The Compressed 3D Lyman-Alpha Forest Bispectrum

Reference 39

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Observation ecfa1792-c12d-44cc-888f-55f33d13af13 · outbound

This paper cites Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level.

Sample Variance Cancellation for Future Spectroscopic Surveys Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level

Reference 40

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Observation e344b24c-9e58-4bbf-a76d-d0fb97024288 · outbound

This paper cites Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory.

Sample Variance Cancellation for Future Spectroscopic Surveys Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory

Reference 41

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Observation c498a78a-a3f4-47f0-9341-aae6c02ba7de · outbound

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

Sample Variance Cancellation for Future Spectroscopic Surveys Lyman Alpha Forest - Halo Cross-Correlations in Effective Field Theory

Reference 42

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Observation 5af87966-f4a9-4dfe-af04-094ce3f3afef · outbound

This paper cites The Ly$\alpha$ forest flux correlation function: a perturbation theory perspective.

Sample Variance Cancellation for Future Spectroscopic Surveys The Ly$\alpha$ forest flux correlation function: a perturbation theory perspective

Reference 43

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Observation 8b1fabbf-3d19-480e-b0de-ec19ccda5e32 · outbound

This paper cites Toward a Measurement of the Cosmological Geometry at z~2: Predicting Lyman-alpha Forest Correlation in Three Dimensions, and the Potential of Future Data Sets.

Sample Variance Cancellation for Future Spectroscopic Surveys Toward a Measurement of the Cosmological Geometry at z~2: Predicting Lyman-alpha Forest Correlation in Three Dimensions, and the Potential of Future Data Sets

Reference 44

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Observation e7cd04d3-7c70-4c34-9862-c0d4e684e11e · outbound

This paper cites Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest.

Sample Variance Cancellation for Future Spectroscopic Surveys Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest

Reference 45

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Observation 9a8f04b5-3e9f-47a6-9560-df3760004b05 · outbound

This paper cites Halo Stochasticity from Exclusion and non-linear Clustering.

Sample Variance Cancellation for Future Spectroscopic Surveys Halo Stochasticity from Exclusion and non-linear Clustering

Reference 46

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