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AGN in dusty Starbursts at z=2: feedback still to kick in
2020
Zenodo
We investigate a sample of 152 dusty sources at 1.5 < z < 2.5 to understand the connection of enhanced Star-Formation-Rate (SFR) and Black-Hole-Accretion-Rate (BHAR). The sources are Herschel-selected, having stellar masses M∗>10^10 Msun and SFR (∼100−1000M/yr) elevated(>4) above the star-forming "main sequence", classifying them as Starbursts (SB). Through a multiwavelength fitting approach (including a dusty torus component), we divided the sample into active SBs (dominated by an AGN
doi:10.5281/zenodo.3629787
fatcat:e7hvfga4hjctrjha5utiarkzwa