机译:The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M-* plane up to z similar to 2
Max Planck Inst Extraterr Phys, D-85741 Garching, Germany;
Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy;
Univ Calif Irvine, Ctr Cosmol, Dept Phys & Astron, Irvine, CA 92697 USAUniv Valparaiso, Inst Fis & Astron, Valparaiso, ChileUniv Bonn, Argelander Inst Astron, D-53121 Bonn, GermanyDSM CNRS Univ Paris Diderot, CEA Saclay, Lab AIM, IRFU,Serv Astrophys,CEA, F-91191 Gif Sur Yvette, FranceTel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Sch Phys & Astron, IL-69978 Tel Aviv, IsraelUniv Sussex, Dept Phys & Astron, Ctr Astron, Brighton BN1 9QH, E Sussex, EnglandUniv Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, EnglandUniv Oxford, Dept Phys, Oxford OX1 3RH, EnglandNASA Ames, Moffett Field, CA 94035 USAUniv Padua, Dipartimento Astron, I-35122 Padua, ItalyUniv Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, ScotlandESAC, Herschel Sci Ctr, Madrid 28691, SpainVirginia Tech, Dept Phys, Blacksburg, VA 24061 USACALTECH, Pasadena, CA 91125 USA;
galaxies: evolution; galaxies: formation; galaxies: starburst; galaxies: high-redshift; infrared: galaxies;