MIGHTEE: Multi-wavelength counterparts in the COSMOS field von Whittam, I.H, Prescott, M, Hale, C.L, Jarvis, M.J, Heywood, I, An, F, Glowacki, Marcin, Maddox, N, Marchetti, L, Morabito, L.K, Adams, N.J, Bowler, R.A.A, Hatfield, P.W, Varadaraj, R.G, Collier, J, Frank, B, Taylor, A.R, Santos, M.G, Vaccari, M, Afonso, J, Ao, Y, Delhaize, J, Knowles, K, Kolwa, S, Randriamampandry, S.M, Randriamanakoto, Z, Smirnov, O, Smith, D.J.B, White, S.V

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MIGHTEE: deep 1.4 GHz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei von Hale, C.L, Whittam, I.H, Jarvis, M.J, Best, P.N, Thomas, N.L, Heywood, I, Prescott, M, Adams, N, Afonso, J, An, F, Bowler, R.A.A, Collier, Jordan, Cook, R.H.W, Davé, R, Frank, B.S, Glowacki, M, Hatfield, P.W, Kolwa, S, Lovell, C.C, Maddox, N, Marchetti, L, Morabito, L.K, Murphy, E, Prandoni, I, Randriamanakoto, Z, Taylor, A.R

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

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