A Generalized Power-Law Diagnostic for Infrared Galaxies at z>1: Active
  Galactic Nuclei and Hot Interstellar Dust
  I present a generalized power-law diagnostic that allows to identify the
presence of active galactic nuclei (AGN) in infrared (IR) galaxies at z>1, down
to flux densities at which the extragalactic IR background is mostly resolved.
I derive this diagnostic from the analysis of 174 galaxies with Snu(24)>80
microJy and spectroscopic redshifts zspec>1 in the Chandra Deep Field South,
for which I study the rest-frame UV/optical/near-IR spectral energy
distributions (SEDs), after subtracting a hot-dust, power-law component with
three possible spectral indices alpha=1.3, 2.0 and 3.0. I obtain that 35% of
these 24micron sources are power-law composite galaxies (PLCGs), which I define
as those galaxies for which the SED fitting with stellar templates, without any
previous power-law subtraction, can be rejected with >2sigma confidence.
Subtracting the power-law component from the PLCG SEDs produces stellar-mass
correction factors <1.5 in >80% of cases. The PLCG incidence is especially high
(47%) at z=1.0-1.5. To unveil which PLCGs host AGN, I conduct a combined
analysis of 4Ms X-ray data, galaxy morphologies, and a greybody modelling of
the hot dust. I find that: 1) 77% of all the X-ray AGN in my 24micron sample at
z=1.0-1.5 are recognised by the PLCG criterion; 2) PLCGs with alpha=1.3 or 2.0
have regular morphologies and T_dust >~1000 K, indicating nuclear activity.
Instead, PLCGs with alpha=3.0 are characterised by disturbed galaxy dynamics,
and a hot interstellar medium can explain their dust temperatures T_dust
~700-800 K. Overall, my results indicate that the fraction of AGN among 24
micron sources is between ~30% and 52% at z=1.0-1.5.
