The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing

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Autores principales: Farren, Gerrit S., Krolewski, Alex, MacCrann, Niall, Ferraro, Simone, Abril-Cabezas, Irene, An, Rui, Atkins, Zachary, Battaglia, Nicholas, Bond, J. Richard, Calabrese, Erminia, Choi, Steve K., Darwish, Omar, Devlin, Mark J., Duivenvoorden, Adriaan J., Dunkley, Jo, Hill, J. Colin, Hilton, Matt, Huffenberger, Kevin M., Kim, Joshua, Louis, Thibaut, Madhavacheril, Mathew S., Marques, Gabriela A., Moodley, Kavilan, Page, Lyman A., Partridge, Bruce, Qu, Frank J., Schaan, Emmanuel, Sehgal, Neelima, Sherwin, Blake D., Sifón, Cristóbal, Staggs, Suzanne T., Van Engelen, Alexander, Vargas, Cristian, Wenzl, Lukas, White, Martin, Wollack, Edward J.
Formato: Preprint
Publicado: 2023
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author Farren, Gerrit S.
Krolewski, Alex
MacCrann, Niall
Ferraro, Simone
Abril-Cabezas, Irene
An, Rui
Atkins, Zachary
Battaglia, Nicholas
Bond, J. Richard
Calabrese, Erminia
Choi, Steve K.
Darwish, Omar
Devlin, Mark J.
Duivenvoorden, Adriaan J.
Dunkley, Jo
Hill, J. Colin
Hilton, Matt
Huffenberger, Kevin M.
Kim, Joshua
Louis, Thibaut
Madhavacheril, Mathew S.
Marques, Gabriela A.
Moodley, Kavilan
Page, Lyman A.
Partridge, Bruce
Qu, Frank J.
Schaan, Emmanuel
Sehgal, Neelima
Sherwin, Blake D.
Sifón, Cristóbal
Staggs, Suzanne T.
Van Engelen, Alexander
Vargas, Cristian
Wenzl, Lukas
White, Martin
Wollack, Edward J.
author_facet Farren, Gerrit S.
Krolewski, Alex
MacCrann, Niall
Ferraro, Simone
Abril-Cabezas, Irene
An, Rui
Atkins, Zachary
Battaglia, Nicholas
Bond, J. Richard
Calabrese, Erminia
Choi, Steve K.
Darwish, Omar
Devlin, Mark J.
Duivenvoorden, Adriaan J.
Dunkley, Jo
Hill, J. Colin
Hilton, Matt
Huffenberger, Kevin M.
Kim, Joshua
Louis, Thibaut
Madhavacheril, Mathew S.
Marques, Gabriela A.
Moodley, Kavilan
Page, Lyman A.
Partridge, Bruce
Qu, Frank J.
Schaan, Emmanuel
Sehgal, Neelima
Sherwin, Blake D.
Sifón, Cristóbal
Staggs, Suzanne T.
Van Engelen, Alexander
Vargas, Cristian
Wenzl, Lukas
White, Martin
Wollack, Edward J.
contents We present tomographic measurements of structure growth using cross-correlations of Atacama Cosmology Telescope (ACT) DR6 and Planck CMB lensing maps with the unWISE Blue and Green galaxy samples, which span the redshift ranges $0.2 \lesssim z \lesssim 1.1$ and $0.3 \lesssim z \lesssim 1.8$, respectively. We improve on prior unWISE cross-correlations not just by making use of the new, high-precision ACT DR6 lensing maps, but also by including additional spectroscopic data for redshift calibration and by analysing our measurements with a more flexible theoretical model. An extensive suite of systematic and null tests within a blind analysis framework ensures that our results are robust. We determine the amplitude of matter fluctuations at low redshifts ($z\simeq 0.2-1.6$), finding $S_8 \equiv σ_8 (Ω_m / 0.3)^{0.5} = 0.813 \pm 0.021$ using the ACT cross-correlation alone and $S_8 = 0.810 \pm 0.015$ with a combination of Planck and ACT cross-correlations; these measurements are fully consistent with the predictions from primary CMB measurements assuming standard structure growth. The addition of Baryon Acoustic Oscillation data breaks the degeneracy between $σ_8$ and $Ω_m$, allowing us to measure $σ_8 = 0.813 \pm 0.020$ from the cross-correlation of unWISE with ACT and $σ_8 = 0.813\pm 0.015$ from the combination of cross-correlations with ACT and Planck. These results also agree with the expectations from primary CMB extrapolations in $Λ$CDM cosmology; the consistency of $σ_8$ derived from our two redshift samples at $z \sim 0.6$ and $1.1$ provides a further check of our cosmological model. Our results suggest that structure formation on linear scales is well described by $Λ$CDM even down to low redshifts $z\lesssim 1$.
format Preprint
id arxiv_https___arxiv_org_abs_2309_05659
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
Farren, Gerrit S.
Krolewski, Alex
MacCrann, Niall
Ferraro, Simone
Abril-Cabezas, Irene
An, Rui
Atkins, Zachary
Battaglia, Nicholas
Bond, J. Richard
Calabrese, Erminia
Choi, Steve K.
Darwish, Omar
Devlin, Mark J.
Duivenvoorden, Adriaan J.
Dunkley, Jo
Hill, J. Colin
Hilton, Matt
Huffenberger, Kevin M.
Kim, Joshua
Louis, Thibaut
Madhavacheril, Mathew S.
Marques, Gabriela A.
Moodley, Kavilan
Page, Lyman A.
Partridge, Bruce
Qu, Frank J.
Schaan, Emmanuel
Sehgal, Neelima
Sherwin, Blake D.
Sifón, Cristóbal
Staggs, Suzanne T.
Van Engelen, Alexander
Vargas, Cristian
Wenzl, Lukas
White, Martin
Wollack, Edward J.
Cosmology and Nongalactic Astrophysics
We present tomographic measurements of structure growth using cross-correlations of Atacama Cosmology Telescope (ACT) DR6 and Planck CMB lensing maps with the unWISE Blue and Green galaxy samples, which span the redshift ranges $0.2 \lesssim z \lesssim 1.1$ and $0.3 \lesssim z \lesssim 1.8$, respectively. We improve on prior unWISE cross-correlations not just by making use of the new, high-precision ACT DR6 lensing maps, but also by including additional spectroscopic data for redshift calibration and by analysing our measurements with a more flexible theoretical model. An extensive suite of systematic and null tests within a blind analysis framework ensures that our results are robust. We determine the amplitude of matter fluctuations at low redshifts ($z\simeq 0.2-1.6$), finding $S_8 \equiv σ_8 (Ω_m / 0.3)^{0.5} = 0.813 \pm 0.021$ using the ACT cross-correlation alone and $S_8 = 0.810 \pm 0.015$ with a combination of Planck and ACT cross-correlations; these measurements are fully consistent with the predictions from primary CMB measurements assuming standard structure growth. The addition of Baryon Acoustic Oscillation data breaks the degeneracy between $σ_8$ and $Ω_m$, allowing us to measure $σ_8 = 0.813 \pm 0.020$ from the cross-correlation of unWISE with ACT and $σ_8 = 0.813\pm 0.015$ from the combination of cross-correlations with ACT and Planck. These results also agree with the expectations from primary CMB extrapolations in $Λ$CDM cosmology; the consistency of $σ_8$ derived from our two redshift samples at $z \sim 0.6$ and $1.1$ provides a further check of our cosmological model. Our results suggest that structure formation on linear scales is well described by $Λ$CDM even down to low redshifts $z\lesssim 1$.
title The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2309.05659