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

Over the past decade, several works have used the ratio between total (rest 8−1000 μm) infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (qIR), often referred to as the infrared-radio correlation (IRRC), to calibrate the radio emission as a star formation rate (SFR) indicator. Pr...

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Bibliographic Details
Main Authors:	Delvecchio, I, Daddi, E, Sargent, MT, Jarvis, MJ, Elbaz, D, Jin, S, Liu, D, Whittam, IH, Algera, H, Carraro, R, D'Eugenio, C, Delhaize, J, Kalita, BS, Leslie, S, Molnar, DC, Novak, M, Prandoni, I, Smolcic, V, Ao, Y, Aravena, M, Bournaud, F, Collier, JD, Randriamampandry, SM, Randriamanakoto, Z, Rodighiero, G, Schober, J, White, SV, Zamorani, G
Format:	Journal article
Language:	English
Published:	European Southern Observatory 2021

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

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