BIANCHI, SimoneSimoneBIANCHIMURGIA, MATTEOMATTEOMURGIAMELIS, AndreaAndreaMELISCASASOLA, VIVIANAVIVIANACASASOLAGalametz, MaudMaudGalametzGalliano, FrédéricFrédéricGallianoGOVONI, FEDERICAFEDERICAGOVONIJones, AnthonyAnthonyJonesMadden, SuzanneSuzanneMaddenPaladino, RositaRositaPaladinoXilouris, EmmanuelEmmanuelXilourisYsard, NathalieNathalieYsard2023-01-262023-01-262022978-2-7598-9118-42101-6275http://hdl.handle.net/20.500.12386/33065The mm-to-cm range of the Spectral Energy Distribution of spiral galaxies remains largely unexplored. Its coverage is required to disentangle the contribution of dust emission, free-free and synchrotron radiation and can provide constraints on dust models, star-formation rates and ISM properties. We present the case for a synergy between NIKA2 observations of nearby spirals and those from planned and current instrumentation at the Sardinia Radio Telescope, and report on a pilot K-band program to search for Anomalous Microwave Emission, an elusive emission component which is presumably related to dust.STAMPAenThe mm-to-cm SED of spiral galaxies. Synergies between NIKA2 and SRT instrumentsConference paper10.1051/epjconf/202225700005https://www.epj-conferences.org/articles/epjconf/abs/2022/01/epjconf_mmUniverse2021_00005/epjconf_mmUniverse2021_00005.html2022EPJWC.25700005BFIS/08 - DIDATTICA E STORIA DELLA FISICA