BISOU: a balloon project for spectral observations of the early universe

B. Maffei, N. Aghanim, J. Aumont, E. Battistelli, J. Chluba, X. Coulon, P. de Bernardis, M. Douspis, J. Grain, J. C. Hill, A. Kogut, Joseph Kuruvilla, G. Lagache, Juan Macis-Perez, S. Masi, T. Matsumura, L. Mele, A. Monfardini, C. O'sullivan, L. Pagano, G. Pisano, N. Ponthieu, M. Remazeilles, A. Ritacco, A. Rotti, G. Savini, V. Sauvage, A. Shitvov, S. Stever, A. Tartari, L. Thiele, N. Trappe, Jean-François Aubrun, A. Laurens, D. Pheav, F. Vacher
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Abstract

The BISOU (Balloon Interferometer for Spectral Observations of the Universe) project studies the viability and prospects of a balloon-borne spectrometer, pathfinder of a future space mission dedicated to the measurements of the CMB spectral distortions, while consolidating the instrumental concept and improving the readiness of some of its key sub-systems. A balloon concept based on a Fourier Transform Spectrometer, covering a spectral range from about 90 GHz to 2 THz, adapted from previous mission proposals such as PIXIE and FOSSIL, is being studied and modelled. Taking into account the requirements and conditions of balloon flights (i.e. residual atmosphere, observation strategy for instance), we present here the instrument concept together with the results of the CNES phase 0 study, evaluating the sensitivity to some of its potential observables. For instance, we forecast a detection of the CMB Compton y-distortion monopole with a signal-to-noise ratio of at least 5.
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BISOU:早期宇宙光谱观测的气球项目
BISOU(宇宙光谱观测气球干涉仪)项目研究了气球载光谱仪的可行性和前景,这是未来太空任务的探路者,致力于测量宇宙微波背景辐射的光谱畸变,同时巩固了仪器概念,提高了一些关键子系统的准备程度。一个基于傅里叶变换光谱仪的气球概念,覆盖了大约90千兆赫到2太赫兹的光谱范围,改编自先前的任务提案,如PIXIE和FOSSIL,正在研究和建模。考虑到气球飞行的要求和条件(例如残余大气,观测策略),我们在这里提出了仪器概念以及CNES第0阶段研究的结果,评估了对一些潜在观测值的敏感性。例如,我们预测CMB康普顿失真单极子的信噪比至少为5。
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