CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2
We examine the fraction of massive (M-* > 10(10)M(circle dot)) compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at z similar to 2. These cSFGs are likely the direct progenitors of the compact quiescent galaxies observed at this epoch, which are the first population...
Similar Items
-
Lyman continuum escape fraction of faint galaxies at z ~ 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC
by: Grazian, A., et al.
Published: (2017) -
Investigating the link between bulge growth and quenching in massive galaxies through polychromatic bulge-disk decompositions in the CANDELS fields
by: Dimauro, Paola
Published: (2017) -
STELLAR MASS–GAS-PHASE METALLICITY RELATION AT 0.5 ≤ z ≤ 0.7: A POWER LAW WITH INCREASING SCATTER TOWARD THE LOW-MASS REGIME
by: Guo, Yicheng, et al.
Published: (2016) -
THE EVOLUTION OF STAR FORMATION HISTORIES OF QUIESCENT GALAXIES
by: Pacifici, Camilla, et al.
Published: (2016) -
The AGN–Star Formation Connection: Future Prospects with JWST
by: Kirkpatrick, Allison, et al.
Published: (2017)