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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics

As of 12 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 2 inbound Pith citation observations for arXiv:2502.02246.

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pith.paper-citation-record.v1
2502.02246 v3

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measured 40 of 40 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Source: arxiv_reference, observed 2026-05-23T04:32:31.999451Z

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40 of 40 outbound references displayed

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Outbound references

Observation 5f748d72-543a-475f-bbb6-70977938b8f2 · outbound

This paper cites an unresolved cited work.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

Reference 1

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Observation 736eb0ed-c002-47e2-8ef1-33c5ddd778f5 · outbound

This paper cites One simple solution for low redshift galaxy distributions is to use the same specification as for sources.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics One simple solution for low redshift galaxy distributions is to use the same specification as for sources

Reference 2

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This paper cites The binning is opti- mized for different values of the photometric redshift uncer- taintyσz.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The binning is opti- mized for different values of the photometric redshift uncer- taintyσz

Reference 3

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Observation fc4ad3cd-67c4-4c90-81b0-7c2537f49cac · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 4

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This paper cites (A2) For simplicity, we will drop the tilde in the main text.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics (A2) For simplicity, we will drop the tilde in the main text

Reference 5

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

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Observation d0f574d5-0961-492b-a37a-a3c4b09e930d · outbound

This paper cites This procedure is purely geometri- cal and thus scale-independent and independent of the power spectrum or matter density contrast.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics This procedure is purely geometri- cal and thus scale-independent and independent of the power spectrum or matter density contrast

Reference 8

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This paper cites Specifically, we require ˆwa(z) ⩽ 0.1× max( ˆwa(z))≈ 0.02 for z ⩽ z ˆw(a), where we take 0.2 as an approximated common maximum value across all nulled lensing kernels.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Specifically, we require ˆwa(z) ⩽ 0.1× max( ˆwa(z))≈ 0.02 for z ⩽ z ˆw(a), where we take 0.2 as an approximated common maximum value across all nulled lensing kernels

Reference 9

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This paper cites Specifically, we require na−3(z ˆw(a)) ⩽ 0.1× n(z), to ensure that the overlap between na−3(z) and ˆwa(z) con- tributes negligibly to the signal.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Specifically, we require na−3(z ˆw(a)) ⩽ 0.1× n(z), to ensure that the overlap between na−3(z) and ˆwa(z) con- tributes negligibly to the signal

Reference 10

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

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Observation c191010f-4f88-419f-acea-40ce699ffd17 · outbound

This paper cites The Kilo-Degree Survey.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The Kilo-Degree Survey

Reference 12

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This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 13

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This paper cites The Dark Energy Survey.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The Dark Energy Survey

Reference 14

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics pre-factor unity approximation

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This paper cites Large Synoptic Survey Telescope: Dark Energy Science Collaboration.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Large Synoptic Survey Telescope: Dark Energy Science Collaboration

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This paper cites Mellier et al.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Mellier et al

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This paper cites Power Spectrum Tomography with Weak Lensing.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Power Spectrum Tomography with Weak Lensing

Reference 18

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This paper cites Cosmic shear full nulling: sorting out dynamics, geometry and systematics.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cosmic shear full nulling: sorting out dynamics, geometry and systematics

Reference 19

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This paper cites x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics x-cut Cosmic Shear: Optimally Removing Sensitivity to Baryonic and Nonlinear Physics with an Application to the Dark Energy Survey Year 1 Shear Data

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This paper cites Observing Baryonic Acoustic Oscillations in tomographic cosmic shear surveys.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Observing Baryonic Acoustic Oscillations in tomographic cosmic shear surveys

Reference 21

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Observation a6fb5e18-fc5d-4968-b905-a1eecd3df173 · outbound

This paper cites Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence

Reference 22

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This paper cites A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing

Reference 23

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This paper cites Controlling intrinsic alignments in weak lensing statistics: The nulling and boosting techniques.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Controlling intrinsic alignments in weak lensing statistics: The nulling and boosting techniques

Reference 24

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This paper cites Cosmological lensing ratios with DES Y1, SPT and Planck.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cosmological lensing ratios with DES Y1, SPT and Planck

Reference 25

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This paper cites Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios

Reference 26

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This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

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This paper cites Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Kaiser, Weak gravitational lensing of distant galaxies, As- trophys

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This paper cites Revising the Halofit Model for the Nonlinear Matter Power Spectrum.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Revising the Halofit Model for the Nonlinear Matter Power Spectrum

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Stable clustering, the halo model and nonlinear cosmological power spectra

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This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Planck 2018 results. I. Overview and the cosmological legacy of Planck

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Euclid preparation: VII. Forecast validation for Euclid cosmological probes

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments

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This paper cites Determination of Inflationary Observables by Cosmic Microwave Background Anisotropy Experiments.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Determination of Inflationary Observables by Cosmic Microwave Background Anisotropy Experiments

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This paper cites The Limits of Cosmic Shear.

Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics The Limits of Cosmic Shear

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Precision calculations of the cosmic shear power spectrum projection

Reference 37

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Unresolved cited work

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics A Fitting Formula for the Non-Linear Evolution of the Bispectrum

Reference 39

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Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 40

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Observation e14bc32a-5c18-4498-9c4c-186245e6d632 · inbound

Mitigating Nonlinear Systematics in Weak Lensing Surveys: The Bernardeau-Nishimichi-Taruya Approach cites this paper.

Mitigating Nonlinear Systematics in Weak Lensing Surveys: The Bernardeau-Nishimichi-Taruya Approach Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics

Reference 27

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Novel geometrical test of cosmological expansion from photometric data cites this paper.

Novel geometrical test of cosmological expansion from photometric data Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics

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