Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog

Fuente: arXiv
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Auteurs principaux: Huang, Yu-Hsiu, Krause, Elisabeth, Xu, Jiachuan, Eifler, Tim, S., Pranjal R., Huff, Eric
Format: Preprint
Publié: 2024
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author Huang, Yu-Hsiu
Krause, Elisabeth
Xu, Jiachuan
Eifler, Tim
S., Pranjal R.
Huff, Eric
author_facet Huang, Yu-Hsiu
Krause, Elisabeth
Xu, Jiachuan
Eifler, Tim
S., Pranjal R.
Huff, Eric
contents Kinematic lensing (KL) is a new weak lensing technique that reduces shape noise for disk galaxies by including spectroscopically measured galaxy kinematics in addition to photometrically measured galaxy shapes. Since KL utilizes the Tully-Fisher relation, any correlation of this relation with the local environment may bias the cosmological interpretation. For the first time, we explore such a Tully-Fisher environmental dependence (TED) effect as a potential astrophysical systematic for KL. Our derivation of the TED systematic can be described in a similar analytical form as intrinsic alignment for traditional weak lensing. We demonstrate analytically that TED only impacts KL if intrinsic aligment for disk galaxies is non-zero. We further use IllustrisTNG simulations to quantify the TED effect. Our two-point correlation measurements do not yield any additional coherent signals that would indicate a systematic bias on KL, within the uncertainties set by the simulation volume.
format Preprint
id arxiv_https___arxiv_org_abs_2404_00197
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
Huang, Yu-Hsiu
Krause, Elisabeth
Xu, Jiachuan
Eifler, Tim
S., Pranjal R.
Huff, Eric
Cosmology and Nongalactic Astrophysics
Kinematic lensing (KL) is a new weak lensing technique that reduces shape noise for disk galaxies by including spectroscopically measured galaxy kinematics in addition to photometrically measured galaxy shapes. Since KL utilizes the Tully-Fisher relation, any correlation of this relation with the local environment may bias the cosmological interpretation. For the first time, we explore such a Tully-Fisher environmental dependence (TED) effect as a potential astrophysical systematic for KL. Our derivation of the TED systematic can be described in a similar analytical form as intrinsic alignment for traditional weak lensing. We demonstrate analytically that TED only impacts KL if intrinsic aligment for disk galaxies is non-zero. We further use IllustrisTNG simulations to quantify the TED effect. Our two-point correlation measurements do not yield any additional coherent signals that would indicate a systematic bias on KL, within the uncertainties set by the simulation volume.
title Astrophysical systematics in Kinematic Lensing: quantifying an Intrinsic Alignment analog
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2404.00197