Spin bias: theory and observations

I summarize here my contribution to the 62a Meeting of the Argentinian Astronomical Society. My presentation addressed the halo-galaxy connection and, in particular, the effect catted secondary halo bias, which refers to the secondary dependencies of halo clustering at fixed halo mass. In this paper...

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Autor principal: Montero Dorta, A. D.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2021
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/171019
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spelling I19-R120-10915-1710192024-10-02T20:04:34Z http://sedici.unlp.edu.ar/handle/10915/171019 Spin bias: theory and observations Montero Dorta, A. D. 2021 2024-10-02T13:47:02Z en Ciencias Astronómicas cosmology: theory dark matter large-scale structure of universe galaxies: halos I summarize here my contribution to the 62a Meeting of the Argentinian Astronomical Society. My presentation addressed the halo-galaxy connection and, in particular, the effect catted secondary halo bias, which refers to the secondary dependencies of halo clustering at fixed halo mass. In this paper, I focused on one of these secondary dependencies, the so-called halo spin bias, which corresponds to the contribution from halo spin. I show here a high signal-to-noise measurement of the effect, discuss some of the physical mechanisms associated with it, and propose a method to probe it with future observations based on the Sunyaev-Zel’dovich effect. Resumo aquí mi contribución a la 62a Reunión de la Asociación Argentina de Astronomía. Mi presentación se centró en la conexión halo-galaxia y, en particular, en el fenómeno conocido como secondary halo bias. Este término engloba todas las dependencias secundarias (a masa de halo fija) de la distribución espacial de los halos. El presente artículo aborda una de estas dependencias, el llamado halo spin bias, que corresponde a la contribución del spin al agrupamiento o clustering de los halos. Muestro aquí una medida precisa del efecto, discuto algunos de los mecanismos físicos asociados con el mismo y propongo un posible método de observación basado en el efecto Sunyaev-Zel’dovich. Asociación Argentina de Astronomía Articulo Articulo http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 159-164
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
cosmology: theory
dark matter
large-scale structure of universe
galaxies: halos
spellingShingle Ciencias Astronómicas
cosmology: theory
dark matter
large-scale structure of universe
galaxies: halos
Montero Dorta, A. D.
Spin bias: theory and observations
topic_facet Ciencias Astronómicas
cosmology: theory
dark matter
large-scale structure of universe
galaxies: halos
description I summarize here my contribution to the 62a Meeting of the Argentinian Astronomical Society. My presentation addressed the halo-galaxy connection and, in particular, the effect catted secondary halo bias, which refers to the secondary dependencies of halo clustering at fixed halo mass. In this paper, I focused on one of these secondary dependencies, the so-called halo spin bias, which corresponds to the contribution from halo spin. I show here a high signal-to-noise measurement of the effect, discuss some of the physical mechanisms associated with it, and propose a method to probe it with future observations based on the Sunyaev-Zel’dovich effect.
format Articulo
Articulo
author Montero Dorta, A. D.
author_facet Montero Dorta, A. D.
author_sort Montero Dorta, A. D.
title Spin bias: theory and observations
title_short Spin bias: theory and observations
title_full Spin bias: theory and observations
title_fullStr Spin bias: theory and observations
title_full_unstemmed Spin bias: theory and observations
title_sort spin bias: theory and observations
publishDate 2021
url http://sedici.unlp.edu.ar/handle/10915/171019
work_keys_str_mv AT monterodortaad spinbiastheoryandobservations
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