VALENTE, GiuseppeGiuseppeVALENTEMARONGIU, PasqualinoPasqualinoMARONGIU0000-0003-0314-7801NAVARRINI, AlessandroAlessandroNAVARRINI0000-0002-6191-6958SABA, AndreaAndreaSABA0000-0002-1607-5010Montisci, G.G.MontisciLADU, AdelaideAdelaideLADU0000-0003-1920-9560PISANU, ToninoToninoPISANU0000-0003-2510-7501PILI, MauroMauroPILI0000-0003-3715-1091Dessi, S.S.DessiUccheddu, A.A.UcchedduIacolina, N.N.IacolinaPERRODIN, DELPHINEDELPHINEPERRODIN0000-0002-1806-2483BUTTU, MarcoMarcoBUTTU0000-0003-4559-049XEGRON, ELISE MARIE JEANNEELISE MARIE JEANNEEGRON0000-0002-1532-4142MELIS, AndreaAndreaMELIS0000-0002-6558-1315Tiburzi, C.C.TiburziVACCA, VALENTINAVALENTINAVACCA0000-0003-1997-07712020-05-262020-05-26201697815106020760277-786Xhttp://hdl.handle.net/20.500.12386/25199Existing radio receivers have a very low noise temperature. To further increase the observation speed, the new generation of radio receivers use a multi-beam focal plane array (FPA) together with wide bandwidth. In this article, we present the front-end and cryogenic design of the 7-beam FPA double linear polarization receiver for the 64-m primary focus of the Sardinia Radio Telescope. At the end of this article, we show the simulated performances of the front-end receiver and the measurements of the down-conversion section.STAMPAenThe 7-beam S-band cryogenic receiver for the SRT primary focus: project statusConference paper10.1117/12.22326252-s2.0-85015045106000385793800050https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9914/1/The-7-beam-S-band-cryogenic-receiver-for-the-SRT/10.1117/12.2232625.short?SSO=12016SPIE.9914E..22VFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation