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GOODS-ALMA 2.0: Last gigayear star formation histories of the so-called starbursts within the main sequence
L. Ciesla, C. Gómez-Guijarro, V. Buat +8
Recently, a population of compact main sequence (MS) galaxies exhibiting starburst-like properties have been identified in the GOODS-ALMA blind survey at 1.1mm. Several evolution s…
A super-linear "radio-AGN main sequence'' links mean radio-AGN power and galaxy stellar mass since z3
I. Delvecchio, E. Daddi, M. T. Sargent +17
Mapping the average AGN luminosity across galaxy populations and over time encapsulates important clues on the interplay between supermassive black hole (SMBH) and galaxy growth. T…
Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3
E. Daddi, R. M. Rich, F. Valentino +12
We present Keck Cosmic Web Imager (KCWI) observations of giant Lya halos surrounding 9 galaxy groups and clusters at 2<z<3.3, including five new detections and one upper limit. We…
The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4
E. Daddi, I. Delvecchio, P. Dimauro +8
We analyse measurements of the evolving stellar mass (M0) at which the bending of the star-forming main sequence (MS) occurs over 0<z<4. We find M0~10^10Msun over 0<z<1, then M0 ri…
Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions
E. Bernhard, C. N. Tadhunter, J. C. S. Pierce +4
We use deep Herschel observations of the complete 2Jy sample of powerful radio AGNs in the local universe (0.05 < z < 0.7) to probe their cool interstellar medium (ISM) contents an…