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.
BISOU: A balloon project for spectral observations of the early universe / Maffei, B.; Aghanim, N.; Aumont, J.; Battistelli, E.; Chluba, J.; Coulon, X.; De Bernardis, P.; Douspis, M.; Grain, J.; Hill, J. C.; Kogut, A.; Kuruvilla, J.; Lagache, G.; Macias-Perez, J.; Masi, S.; Matsumura, T.; Mele, L.; Monfardini, A.; O'Sullivan, C.; Pagano, L.; Pisano, G.; Ponthieu, N.; Remazeilles, M.; Ritacco, A.; Rotti, A.; Savini, G.; Sauvage, V.; Shitvov, A.; Stever, S. L.; Tartari, A.; Thiele, L.; Trappe, N.; Aubrun, J. -F.; Laurens, A.; Pheav, D.; Vacher, F.. - 12190:(2022), p. 12. (Intervento presentato al convegno SPIE ASTRONOMICAL TELESCOPES + INSTRUMENTATION tenutosi a Montreal, Canada) [10.1117/12.2630136].
BISOU: A balloon project for spectral observations of the early universe
Battistelli E.;De Bernardis P.;Masi S.;Mele L.;Pisano G.;
2022
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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
