Paiella, A., de Bernardis, P., Cacciotti, F., Coppolecchia, A., Masi, S., Barbavara, E., Battistelli, E. S., Carretti, E., Columbro, F., Cruciani, A., D'Alessandro, G., De Petris, M., Govoni, F., Isopi, G., Lamagna, L., Marongiu, P., Mele, L., Molinari, E., Murgia, M., and Navarrini, A.
The MIllimetric Sardinia radio Telescope Receiver based on Array of Lumped elements KIDs, MISTRAL, is a cryogenic W-band (77–103 GH) LEKID camera which will be integrated at the Gregorian focus of the 64 m aperture Sardinia Radio Telescope, in Italy, in Autumn 2022. This instrument, thanks to its high angular resolution ( ∼ 13 arcsec ) and the wide instantaneous field of view ( ∼ 4 arcmin ), will allow continuum surveys of the mm-wave sky with a variety of scientific targets, spanning from extragalactic astrophysics to solar system science. In this contribution, we will describe the design of the MISTRAL camera, with a particular focus on the optimisation and test of a prototype of the focal plane. [ABSTRACT FROM AUTHOR]