Ferrari, L., Bagliani, D., Bardi, A., Battistelli, E., Birkinshaw, M., Colafrancesco, S., Conte, A., DeBernardis, P., DeGregori, S., DePetris, M., De Zotti, G., Donati, A., Franceschini, A., Gatti, F., Gervasi, M., Gonzalez-Nuevo, J., Lamagna, L., Luzzi, G., Maiolino, M., Marchegiani, P., Mariani, A., Masi, S., Massardi, M., Mauskopf, Philip Daniel ![]() |
Official URL: http://dx.doi.org/10.1063/1.3292383
Abstract
We present a concept for the payload SAGACE, the Spectroscopic Active Galaxies And Cluster Explorer, devoted to study the evolution of Universe structures using different observables, all of them in the mm∕submm wavelength. The SAGACE payload is made of a passively cooled 3 m telescope, a cryogenic Fourier Transform Spectrometer (FTS) and detector arrays to be operated at 0.3 K by a 3He fridge. The detectors are Ti∕Au Transition Edge Sensor (TES) bolometers with a NEP<10−17 W/Hz½. A phase‐A study has been recently completed for this experiment, in the framework of the call for small missions of the Italian Space Agency.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | bolometers; galaxies; Fourier transform optics |
Publisher: | American Institute of Physics |
ISBN: | 9780735407510 |
ISSN: | 0094-243X |
Last Modified: | 20 Oct 2022 07:55 |
URI: | https://orca.cardiff.ac.uk/id/eprint/26926 |
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