Paper Citation Record · LEDGER

Sample Variance Cancellation for Future Spectroscopic Surveys

As of 21 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

Coverage vector

measured 45 of 45 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T06:07:09.966305Z

measured 45 of 45 standing notices

One-hop event checks from named stored sources.

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

45 of 45 outbound references displayed

verified exact3
verified fuzzy3
unresolved39
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

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

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T06:07:34.756436Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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

This paper cites Collaboration, A.

Sample Variance Cancellation for Future Spectroscopic Surveys Collaboration, A

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T06:07:34.741972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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

This paper cites Laureijs, J.

Sample Variance Cancellation for Future Spectroscopic Surveys Laureijs, J

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T06:07:34.727981Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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

This paper cites Amendola, S.

Sample Variance Cancellation for Future Spectroscopic Surveys Amendola, S

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.799419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.803353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.807627Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites Besuner, A.

Sample Variance Cancellation for Future Spectroscopic Surveys Besuner, A

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.812359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.815872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.819534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.827778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.831430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.835521Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites Khoraminezhad, S.

Sample Variance Cancellation for Future Spectroscopic Surveys Khoraminezhad, S

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.839740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: verified exact; local_arxiv, observed 2026-08-10T06:07:22.762103Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.847642Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.851887Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.856221Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites Rubiola, S.

Sample Variance Cancellation for Future Spectroscopic Surveys Rubiola, S

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-08-10T06:07:22.696245Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.864369Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.868276Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.871975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites Towards optimal and robust $f_{\rm NL}$ constraints with multi-tracer analyses.

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

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.875939Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.880128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.883943Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites The Galaxy Power Spectrum and Bispectrum in Redshift Space.

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

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.887809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites The clustering of Lyman Alpha Emitting galaxies at z=2-3.

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

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.891673Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f79e0c5-b2ac-4a70-8380-3c92ea8c8410 · outbound

This paper cites High redshift LBGs from deep broadband imaging for future spectroscopic surveys.

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

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.895395Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69d6a7a3-f0f5-4808-9012-492205ce85ed · outbound

This paper cites High-redshift Millennium and Astrid galaxies in effective field theory at the field level.

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

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.898974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e589b41-034f-41ba-addd-cdd1074fcbf4 · outbound

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

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

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.902966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 578949ef-e3eb-44c6-9e30-c56794b20e9e · outbound

This paper cites Measuring the galaxy power spectrum with future redshift surveys.

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

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.906689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b45f1b67-2024-4b40-986c-51d1af25d72f · outbound

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

Resolution: verified exact; local_arxiv, observed 2026-08-10T06:07:10.316706Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 4eb005c7-a0ff-4a92-a1ef-40330f648d16 · outbound

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.914402Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites Estimating the Power Spectrum of the Cosmic Microwave Background.

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

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.918385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.922559Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01d5ec79-5ac4-46e4-bb2d-0211e22d6500 · outbound

This paper cites Towards optimal extraction of cosmological information from nonlinear data.

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

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.926576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.930373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0e708db-8200-4c47-b049-ef8fcedc628e · outbound

This paper cites Cosmology before noon with multiple galaxy populations.

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

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.934329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0d477b52-2fc0-440a-b574-2939e4613350 · outbound

This paper cites The Compressed 3D Lyman-Alpha Forest Bispectrum.

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

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.938135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.941991Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.945862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.949827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.954297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.958358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.962581Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Resolution: unresolved; no resolver link, observed 2026-08-10T06:07:09.966305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

No inbound Pith citation observations are available.