The Atacama Cosmology Telescope: map-based noise simulations for DR6

Atkins, Zachary, Duivenvoorden, Adriaan J., Coulton, William R., Qu, Frank J., Aiola, Simone, Calabrese, Erminia ORCID: https://orcid.org/0000-0003-0837-0068, Chesmore, Grace E., Choi, Steve K., Devlin, Mark J., Dunkley, Jo, Hervías-Caimapo, Carlos, Guan, Yilun, Posta, Adrien La, Li, Zack, Louis, Thibaut, Madhavacheril, Mathew S., Moodley, Kavilan, Naess, Sigurd, Nati, Federico, Niemack, Michael D., Page, Lyman, Puddu, Roberto, Salatino, Maria, Sifón, Cristóbal, Staggs, Suzanne T., Vargas, Cristian, Vavagiakis, Eve M. and Wollack, Edward J. 2023. The Atacama Cosmology Telescope: map-based noise simulations for DR6. Journal of Cosmology and Astroparticle Physics 2023 , 073. 10.1088/1475-7516/2023/11/073

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Abstract

The increasing statistical power of cosmic microwave background (CMB) datasets requires a commensurate effort in understanding their noise properties. The noise in maps from ground-based instruments is dominated by large-scale correlations, which poses a modeling challenge. This paper develops novel models of the complex noise covariance structure in the Atacama Cosmology Telescope Data Release 6 (ACT DR6) maps. We first enumerate the noise properties that arise from the combination of the atmosphere and the ACT scan strategy. We then prescribe a class of Gaussian, map-based noise models, including a new wavelet-based approach that uses directional wavelet kernels for modeling correlated instrumental noise. The models are empirical, whose only inputs are a small number of independent realizations of the same region of sky. We evaluate the performance of these models against the ACT DR6 data by drawing ensembles of noise realizations. Applying these simulations to the ACT DR6 power spectrum pipeline reveals a ∼ 20% excess in the covariance matrix diagonal when compared to an analytic expression that assumes noise properties are uniquely described by their power spectrum. Along with our public code, mnms, this work establishes a necessary element in the science pipelines of both ACT DR6 and future ground-based CMB experiments such as the Simons Observatory (SO).

Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Advanced Research Computing @ Cardiff (ARCCA) Physics and Astronomy
Additional Information:	License information from Publisher: LICENSE 1: URL: http://creativecommons.org/licenses/by/4.0/, Type: cc-by
Publisher:	IOP Publishing
Date of First Compliant Deposit:	16 November 2023
Date of Acceptance:	15 August 2023
Last Modified:	11 Jun 2024 10:18
URI:	https://orca.cardiff.ac.uk/id/eprint/163946

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