1NASA Goddard Space Flight Ctr. (United States) 2Univ. of Maryland, College Park (United States) 3Institut d'Astrophysique Spatiale (France) 4Princeton Univ. (United States) 5CNRS-UCB International Research Lab. (United States) 6Univ. of California, Los Angeles (United States)
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Spectral distortions in the cosmic microwave background open a new window to the structure, content, and evolution of the universe. Detecting the expected signals at the few part-per-billion level requires background-limited sensitivity with careful control of instrumental signatures. PHOENIX is a Probe-class mission to map the CMB and diffuse astrophysical foregrounds at microwave through far-IR wavelengths. I describe the scientific goals and instrument design for the PHOENIX mission and use detailed time-ordered simulations to evaluate the projected instrument performance.
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Alan J. Kogut, Dale J. Fixsen, Nabilah Aghanim, Brandon Hensley, Jacques Delabrouille, Bruno Maffei, Edward J. Wollack, Ioana Zelko, "PHOENIX: a probe-class mission for cosmology," Proc. SPIE 12676, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts XI, 126760D (5 October 2023); https://doi.org/10.1117/12.2676491