Presentation
5 October 2023 PHOENIX: a probe-class mission for cosmology
Author Affiliations +
Abstract
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.
Conference Presentation
© (2023) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alan J. Kogut, Dale J. Fixsen, Nabilah Aghanim, Brandon Hensley, Jacques Delabrouille, Bruno Maffei, Edward J. Wollack, and 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
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KEYWORDS
Cosmology

Equipment

Signal detection

Spectrometers

Modulation

Optical calibration

Simulations

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