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English: From the paper:

"CLASS Angular Power Spectra and Map-component Analysis for 40 GHz Observations through 2022,"

The Astrophysical Journal The American Astronomical Society, find out more.

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The following article isOpen access CLASS Angular Power Spectra and Map-component Analysis for 40 GHz Observations through 2022

Joseph R. Eimer, Yunyang Li (李云炀), Michael K. Brewer, Rui Shi (时瑞), Aamir Ali, John W. Appel, Charles L. Bennett, Sarah Marie Bruno, Ricardo Bustos, David T. Chuss, Joseph Cleary, Sumit Dahal, Rahul Datta, Jullianna Denes Couto, Kevin L. Denis, Rolando Dünner, Thomas Essinger-Hileman, Pedro Fluxá, Johannes Hubmayer, Kathleen Harrington, Jeffrey Iuliano, John Karakla, Tobias A. Marriage, Carolina Núñez, Lucas Parker, Matthew A. Petroff, Rodrigo A. Reeves, Karwan Rostem, Deniz A. N. Valle, Duncan J. Watts, Janet L. Weiland, Edward J. Wollack, Zhilei Xu (徐智磊), and Lingzhen Zeng

Published 2024 March 4 © 2024. The Author(s). Published by the American Astronomical Society. The Astrophysical Journal, Volume 963, Number 2 Citation Joseph R. Eimer et al 2024 ApJ 963 92

DOI 10.3847/1538-4357/ad1abf
Date
Source Own work
Author Tom.essinger.hileman

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Captions

Maps of microwave brightness temperature in Q and U linearly polarized Stokes parameters and V circularly polarized Stokes parameter in the 40 GHz band of the Cosmology Large Angular Scale Surveyor (CLASS).

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