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We investigate the potential of CO rotational lines at redshifts $z\sim 0-6$ being an appreciable source of extragalactic foreground anisotropies in the cosmic microwave background.
1904
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J. Kamenetzky, N. Rangwala, J. Glenn, P. R. Maloney, and A. Conley, “L CO
2016
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T. Y. Li, R. H. Wechsler, K. Devaraj, and S. E. Church, “CONNECTING CO INTENSITY MAPPING TO MOLECULAR GAS AND STAR FORMATION IN THE EPOCH OF GALAXY ASSEMBLY,” The Astrophysical Journal
2016
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“ NIST Digital Library of Mathematical Functions · 2024
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