Measurements of the Thermal Sunyaev-Zel'dovich Effect with ACT and DESI Luminous Red Galaxies

Fuente: arXiv
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Autori principali: Liu, R. Henry, Ferraro, Simone, Schaan, Emmanuel, Zhou, Rongpu, Aguilar, Jessica Nicole, Ahlen, Steven, Battaglia, Nicholas, Bianchi, Davide, Brooks, David, Claybaugh, Todd, Cole, Shaun, Coulton, William R., de la Macorra, Axel, Dey, Arjun, Fanning, Kevin, Forero-Romero, Jaime E., Gaztañaga, Enrique, Gong, Yulin, Gontcho, Satya Gontcho A, Gruen, Daniel, Gutierrez, Gaston, Hadzhiyska, Boryana, Honscheid, Klaus, Howlett, Cullan, Kehoe, Robert, Kisner, Theodore, Kremin, Anthony, Kusiak, Aleksandra, Lambert, Andrew, Landriau, Martin, Guillou, Laurent Le, Levi, Michael, Lokken, Martine, Manera, Marc, Martini, Paul, Meisner, Aaron, Miquel, Ramon, Moodley, Kavilan, Newman, Jeffrey A., Niz, Gustavo, Palanque-Delabrouille, Nathalie, Percival, Will, Prada, Francisco, Pérez-Ràfols, Ignasi, Guachalla, Bernardita Ried, Rossi, Graziano, Sanchez, Eusebio, Schlegel, David, Schubnell, Michael, Seo, Hee-Jong, Sifón, Cristóbal, Sprayberry, David, Tarlé, Gregory, Vavagiakis, Eve M., Weaver, Benjamin Alan, Wollack, Edward J., Zou, Hu
Natura: Preprint
Pubblicazione: 2025
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author Liu, R. Henry
Ferraro, Simone
Schaan, Emmanuel
Zhou, Rongpu
Aguilar, Jessica Nicole
Ahlen, Steven
Battaglia, Nicholas
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cole, Shaun
Coulton, William R.
de la Macorra, Axel
Dey, Arjun
Fanning, Kevin
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gong, Yulin
Gontcho, Satya Gontcho A
Gruen, Daniel
Gutierrez, Gaston
Hadzhiyska, Boryana
Honscheid, Klaus
Howlett, Cullan
Kehoe, Robert
Kisner, Theodore
Kremin, Anthony
Kusiak, Aleksandra
Lambert, Andrew
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Lokken, Martine
Manera, Marc
Martini, Paul
Meisner, Aaron
Miquel, Ramon
Moodley, Kavilan
Newman, Jeffrey A.
Niz, Gustavo
Palanque-Delabrouille, Nathalie
Percival, Will
Prada, Francisco
Pérez-Ràfols, Ignasi
Guachalla, Bernardita Ried
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Seo, Hee-Jong
Sifón, Cristóbal
Sprayberry, David
Tarlé, Gregory
Vavagiakis, Eve M.
Weaver, Benjamin Alan
Wollack, Edward J.
Zou, Hu
author_facet Liu, R. Henry
Ferraro, Simone
Schaan, Emmanuel
Zhou, Rongpu
Aguilar, Jessica Nicole
Ahlen, Steven
Battaglia, Nicholas
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cole, Shaun
Coulton, William R.
de la Macorra, Axel
Dey, Arjun
Fanning, Kevin
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gong, Yulin
Gontcho, Satya Gontcho A
Gruen, Daniel
Gutierrez, Gaston
Hadzhiyska, Boryana
Honscheid, Klaus
Howlett, Cullan
Kehoe, Robert
Kisner, Theodore
Kremin, Anthony
Kusiak, Aleksandra
Lambert, Andrew
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Lokken, Martine
Manera, Marc
Martini, Paul
Meisner, Aaron
Miquel, Ramon
Moodley, Kavilan
Newman, Jeffrey A.
Niz, Gustavo
Palanque-Delabrouille, Nathalie
Percival, Will
Prada, Francisco
Pérez-Ràfols, Ignasi
Guachalla, Bernardita Ried
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Seo, Hee-Jong
Sifón, Cristóbal
Sprayberry, David
Tarlé, Gregory
Vavagiakis, Eve M.
Weaver, Benjamin Alan
Wollack, Edward J.
Zou, Hu
contents Cosmic Microwave Background (CMB) photons scatter off the free-electron gas in galaxies and clusters, allowing us to use the CMB as a backlight to probe the gas in and around low-redshift galaxies. The thermal Sunyaev-Zel'dovich effect, sourced by hot electrons in high-density environments, measures the thermal pressure of the target objects, shedding light on halo thermodynamics and galaxy formation and providing a path toward understanding the baryon distribution around cosmic structures. We use a combination of high-resolution CMB maps from the Atacama Cosmology Telescope (ACT) and photometric luminous red galaxy (LRG) catalogues from the Dark Energy Spectroscopic Instrument (DESI) to measure the thermal Sunyaev-Zel'dovich signal in four redshift bins from $z=0.4$ to $z=1.2$, with a combined detection significance of 19$σ$ when stacking on the fiducial CMB Compton-$y$ map. We discuss possible sources of contamination, finding that residual dust emission associated with the target galaxies is important and limits current analyses. We discuss several mitigation strategies and quantify the residual modelling uncertainty. This work complements closely related measurements of the kinematic Sunyaev-Zel'dovich and weak lensing of the same galaxies.
format Preprint
id arxiv_https___arxiv_org_abs_2502_08850
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Measurements of the Thermal Sunyaev-Zel'dovich Effect with ACT and DESI Luminous Red Galaxies
Liu, R. Henry
Ferraro, Simone
Schaan, Emmanuel
Zhou, Rongpu
Aguilar, Jessica Nicole
Ahlen, Steven
Battaglia, Nicholas
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cole, Shaun
Coulton, William R.
de la Macorra, Axel
Dey, Arjun
Fanning, Kevin
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gong, Yulin
Gontcho, Satya Gontcho A
Gruen, Daniel
Gutierrez, Gaston
Hadzhiyska, Boryana
Honscheid, Klaus
Howlett, Cullan
Kehoe, Robert
Kisner, Theodore
Kremin, Anthony
Kusiak, Aleksandra
Lambert, Andrew
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Lokken, Martine
Manera, Marc
Martini, Paul
Meisner, Aaron
Miquel, Ramon
Moodley, Kavilan
Newman, Jeffrey A.
Niz, Gustavo
Palanque-Delabrouille, Nathalie
Percival, Will
Prada, Francisco
Pérez-Ràfols, Ignasi
Guachalla, Bernardita Ried
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Seo, Hee-Jong
Sifón, Cristóbal
Sprayberry, David
Tarlé, Gregory
Vavagiakis, Eve M.
Weaver, Benjamin Alan
Wollack, Edward J.
Zou, Hu
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Cosmic Microwave Background (CMB) photons scatter off the free-electron gas in galaxies and clusters, allowing us to use the CMB as a backlight to probe the gas in and around low-redshift galaxies. The thermal Sunyaev-Zel'dovich effect, sourced by hot electrons in high-density environments, measures the thermal pressure of the target objects, shedding light on halo thermodynamics and galaxy formation and providing a path toward understanding the baryon distribution around cosmic structures. We use a combination of high-resolution CMB maps from the Atacama Cosmology Telescope (ACT) and photometric luminous red galaxy (LRG) catalogues from the Dark Energy Spectroscopic Instrument (DESI) to measure the thermal Sunyaev-Zel'dovich signal in four redshift bins from $z=0.4$ to $z=1.2$, with a combined detection significance of 19$σ$ when stacking on the fiducial CMB Compton-$y$ map. We discuss possible sources of contamination, finding that residual dust emission associated with the target galaxies is important and limits current analyses. We discuss several mitigation strategies and quantify the residual modelling uncertainty. This work complements closely related measurements of the kinematic Sunyaev-Zel'dovich and weak lensing of the same galaxies.
title Measurements of the Thermal Sunyaev-Zel'dovich Effect with ACT and DESI Luminous Red Galaxies
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2502.08850