The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies

Fuente: arXiv
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Autori principali: Kim, Joshua, Sailer, Noah, Madhavacheril, Mathew S., Ferraro, Simone, Abril-Cabezas, Irene, Aguilar, Jessica Nicole, Ahlen, Steven, Bond, J. Richard, Brooks, David, Burtin, Etienne, Calabrese, Erminia, Chen, Shi-Fan, Choi, Steve K., Claybaugh, Todd, Darwish, Omar, de la Macorra, Axel, DeRose, Joseph, Devlin, Mark, Dey, Arjun, Doel, Peter, Dunkley, Jo, Embil-Villagra, Carmen, Farren, Gerrit S., Font-Ribera, Andreu, Forero-Romero, Jaime E., Gaztañaga, Enrique, Gluscevic, Vera, Gontcho, Satya Gontcho A, Guy, Julien, Honscheid, Klaus, Howlett, Cullan, Kirkby, David, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Guillou, Laurent Le, Levi, Michael E., MacCrann, Niall, Manera, Marc, Marques, Gabriela A., Meisner, Aaron, Miquel, Ramon, Moodley, Kavilan, Moustakas, John, Newburgh, Laura B., Newman, Jeffrey A., Niz, Gustavo, Orlowski-Scherer, John, Palanque-Delabrouille, Nathalie, Percival, Will J., Prada, Francisco, Qu, Frank J., Rossi, Graziano, Sanchez, Eusebio, Schaan, Emmanuel, Schlafly, Edward F., Schlegel, David, Schubnell, Michael, Sehgal, Neelima, Seo, Hee-Jung, Shaikh, Shabbir, Sherwin, Blake D., Sifón, Cristóbal, Sprayberry, David, Staggs, Suzanne T., Tarlé, Gregory, van Engelen, Alexander, Weaver, Benjamin Alan, Wenzl, Lukas, White, Martin, Wollack, Edward J., Yèche, Christophe, Zou, Hu
Natura: Preprint
Pubblicazione: 2024
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author Kim, Joshua
Sailer, Noah
Madhavacheril, Mathew S.
Ferraro, Simone
Abril-Cabezas, Irene
Aguilar, Jessica Nicole
Ahlen, Steven
Bond, J. Richard
Brooks, David
Burtin, Etienne
Calabrese, Erminia
Chen, Shi-Fan
Choi, Steve K.
Claybaugh, Todd
Darwish, Omar
de la Macorra, Axel
DeRose, Joseph
Devlin, Mark
Dey, Arjun
Doel, Peter
Dunkley, Jo
Embil-Villagra, Carmen
Farren, Gerrit S.
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gluscevic, Vera
Gontcho, Satya Gontcho A
Guy, Julien
Honscheid, Klaus
Howlett, Cullan
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Landriau, Martin
Guillou, Laurent Le
Levi, Michael E.
MacCrann, Niall
Manera, Marc
Marques, Gabriela A.
Meisner, Aaron
Miquel, Ramon
Moodley, Kavilan
Moustakas, John
Newburgh, Laura B.
Newman, Jeffrey A.
Niz, Gustavo
Orlowski-Scherer, John
Palanque-Delabrouille, Nathalie
Percival, Will J.
Prada, Francisco
Qu, Frank J.
Rossi, Graziano
Sanchez, Eusebio
Schaan, Emmanuel
Schlafly, Edward F.
Schlegel, David
Schubnell, Michael
Sehgal, Neelima
Seo, Hee-Jung
Shaikh, Shabbir
Sherwin, Blake D.
Sifón, Cristóbal
Sprayberry, David
Staggs, Suzanne T.
Tarlé, Gregory
van Engelen, Alexander
Weaver, Benjamin Alan
Wenzl, Lukas
White, Martin
Wollack, Edward J.
Yèche, Christophe
Zou, Hu
author_facet Kim, Joshua
Sailer, Noah
Madhavacheril, Mathew S.
Ferraro, Simone
Abril-Cabezas, Irene
Aguilar, Jessica Nicole
Ahlen, Steven
Bond, J. Richard
Brooks, David
Burtin, Etienne
Calabrese, Erminia
Chen, Shi-Fan
Choi, Steve K.
Claybaugh, Todd
Darwish, Omar
de la Macorra, Axel
DeRose, Joseph
Devlin, Mark
Dey, Arjun
Doel, Peter
Dunkley, Jo
Embil-Villagra, Carmen
Farren, Gerrit S.
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gluscevic, Vera
Gontcho, Satya Gontcho A
Guy, Julien
Honscheid, Klaus
Howlett, Cullan
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Landriau, Martin
Guillou, Laurent Le
Levi, Michael E.
MacCrann, Niall
Manera, Marc
Marques, Gabriela A.
Meisner, Aaron
Miquel, Ramon
Moodley, Kavilan
Moustakas, John
Newburgh, Laura B.
Newman, Jeffrey A.
Niz, Gustavo
Orlowski-Scherer, John
Palanque-Delabrouille, Nathalie
Percival, Will J.
Prada, Francisco
Qu, Frank J.
Rossi, Graziano
Sanchez, Eusebio
Schaan, Emmanuel
Schlafly, Edward F.
Schlegel, David
Schubnell, Michael
Sehgal, Neelima
Seo, Hee-Jung
Shaikh, Shabbir
Sherwin, Blake D.
Sifón, Cristóbal
Sprayberry, David
Staggs, Suzanne T.
Tarlé, Gregory
van Engelen, Alexander
Weaver, Benjamin Alan
Wenzl, Lukas
White, Martin
Wollack, Edward J.
Yèche, Christophe
Zou, Hu
contents We present a high-significance cross-correlation of CMB lensing maps from the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) with spectroscopically calibrated luminous red galaxies (LRGs) from the Dark Energy Spectroscopic Instrument (DESI). We detect this cross-correlation at a significance of 38$σ$; combining our measurement with the Planck Public Release 4 (PR4) lensing map, we detect the cross-correlation at 50$σ$. Fitting this jointly with the galaxy auto-correlation power spectrum to break the galaxy bias degeneracy with $σ_8$, we perform a tomographic analysis in four LRG redshift bins spanning $0.4 \le z \le 1.0$ to constrain the amplitude of matter density fluctuations through the parameter combination $S_8^\times = σ_8 \left(Ω_m / 0.3\right)^{0.4}$. Prior to unblinding, we confirm with extragalactic simulations that foreground biases are negligible and carry out a comprehensive suite of null and consistency tests. Using a hybrid effective field theory (HEFT) model that allows scales as small as $k_{\rm max}=0.6$ $h/{\rm Mpc}$, we obtain a 3.3% constraint on $S_8^\times = σ_8 \left(Ω_m / 0.3\right)^{0.4} = 0.792^{+0.024}_{-0.028}$ from ACT data, as well as constraints on $S_8^\times(z)$ that probe structure formation over cosmic time. Our result is consistent with the early-universe extrapolation from primary CMB anisotropies measured by Planck PR4 within 1.2$σ$. Jointly fitting ACT and Planck lensing cross-correlations we obtain a 2.7% constraint of $S_8^\times = 0.776^{+0.019}_{-0.021}$, which is consistent with the Planck early-universe extrapolation within 2.1$σ$, with the lowest redshift bin showing the largest difference in mean. The latter may motivate further CMB lensing tomography analyses at $z<0.6$ to assess the impact of potential systematics or the consistency of the $Λ$CDM model over cosmic time.
format Preprint
id arxiv_https___arxiv_org_abs_2407_04606
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
Kim, Joshua
Sailer, Noah
Madhavacheril, Mathew S.
Ferraro, Simone
Abril-Cabezas, Irene
Aguilar, Jessica Nicole
Ahlen, Steven
Bond, J. Richard
Brooks, David
Burtin, Etienne
Calabrese, Erminia
Chen, Shi-Fan
Choi, Steve K.
Claybaugh, Todd
Darwish, Omar
de la Macorra, Axel
DeRose, Joseph
Devlin, Mark
Dey, Arjun
Doel, Peter
Dunkley, Jo
Embil-Villagra, Carmen
Farren, Gerrit S.
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gluscevic, Vera
Gontcho, Satya Gontcho A
Guy, Julien
Honscheid, Klaus
Howlett, Cullan
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Landriau, Martin
Guillou, Laurent Le
Levi, Michael E.
MacCrann, Niall
Manera, Marc
Marques, Gabriela A.
Meisner, Aaron
Miquel, Ramon
Moodley, Kavilan
Moustakas, John
Newburgh, Laura B.
Newman, Jeffrey A.
Niz, Gustavo
Orlowski-Scherer, John
Palanque-Delabrouille, Nathalie
Percival, Will J.
Prada, Francisco
Qu, Frank J.
Rossi, Graziano
Sanchez, Eusebio
Schaan, Emmanuel
Schlafly, Edward F.
Schlegel, David
Schubnell, Michael
Sehgal, Neelima
Seo, Hee-Jung
Shaikh, Shabbir
Sherwin, Blake D.
Sifón, Cristóbal
Sprayberry, David
Staggs, Suzanne T.
Tarlé, Gregory
van Engelen, Alexander
Weaver, Benjamin Alan
Wenzl, Lukas
White, Martin
Wollack, Edward J.
Yèche, Christophe
Zou, Hu
Cosmology and Nongalactic Astrophysics
We present a high-significance cross-correlation of CMB lensing maps from the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) with spectroscopically calibrated luminous red galaxies (LRGs) from the Dark Energy Spectroscopic Instrument (DESI). We detect this cross-correlation at a significance of 38$σ$; combining our measurement with the Planck Public Release 4 (PR4) lensing map, we detect the cross-correlation at 50$σ$. Fitting this jointly with the galaxy auto-correlation power spectrum to break the galaxy bias degeneracy with $σ_8$, we perform a tomographic analysis in four LRG redshift bins spanning $0.4 \le z \le 1.0$ to constrain the amplitude of matter density fluctuations through the parameter combination $S_8^\times = σ_8 \left(Ω_m / 0.3\right)^{0.4}$. Prior to unblinding, we confirm with extragalactic simulations that foreground biases are negligible and carry out a comprehensive suite of null and consistency tests. Using a hybrid effective field theory (HEFT) model that allows scales as small as $k_{\rm max}=0.6$ $h/{\rm Mpc}$, we obtain a 3.3% constraint on $S_8^\times = σ_8 \left(Ω_m / 0.3\right)^{0.4} = 0.792^{+0.024}_{-0.028}$ from ACT data, as well as constraints on $S_8^\times(z)$ that probe structure formation over cosmic time. Our result is consistent with the early-universe extrapolation from primary CMB anisotropies measured by Planck PR4 within 1.2$σ$. Jointly fitting ACT and Planck lensing cross-correlations we obtain a 2.7% constraint of $S_8^\times = 0.776^{+0.019}_{-0.021}$, which is consistent with the Planck early-universe extrapolation within 2.1$σ$, with the lowest redshift bin showing the largest difference in mean. The latter may motivate further CMB lensing tomography analyses at $z<0.6$ to assess the impact of potential systematics or the consistency of the $Λ$CDM model over cosmic time.
title The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2407.04606