The infrared-radio correlation of star-forming galaxies is strongly M*-dependent but nearly redshift-invariant since z ~ 4

Author(s):
Delvecchio, I.; Daddi, E.; Sargent, M.T.; Jarvis, M.J.; Elbaz, D.; Jin, S.; Liu, D.; Whittam, I.H.; Algera, H.S.B.; Carraro, R.; D'Eugenio, C.; Delhaize, J.; Kalita, B.S.; Leslie, S.K. (0000-0002-4826-8642); Molnár, D.C.; Novak, M.; Prandoni, I.; Smolčić, V.; Ao, Y.; Aravena, M.; Bournaud, F.; Collier, J.D.; Randriamampandry, S.M.; Randriamanakoto, Z.; Rodighiero, G.; Schober, J.; White, S.V.; Zamorani, G.
Published
2021
Publication type
Article / Letter to editor
Galaxies: star formationRadio continuum: galaxiesInfrared: galaxiesGalaxies: activeGalaxies: evolutionAstrophysics - astrophysics of galaxies
Date issued
2021
Language
English
Is part of
Astronomy & Astrophysics (2021), Vol. 647, p. 1-29
hdl
1887/3270720
doi
10.1051/0004-6361/202039647
URL
https://ui.adsabs.harvard.edu/abs/2021A&A...647A.123D