The central energy source of 70micron-selected galaxies: Starburst or AGN?
M. Symeonidis, D. Rosario, A. Georgakakis, J. Harker, E. S. Laird and, M. J. Page

TL;DR
This study investigates the energy sources of 70-micron-selected galaxies, finding most are starburst-dominated with a small fraction hosting energetically significant AGN, and the AGN fraction increases with infrared luminosity.
Contribution
First comprehensive AGN census in 70-micron-selected galaxies showing star formation as the primary power source, with a detailed analysis of AGN prevalence across luminosity classes.
Findings
13% of galaxies show AGN signatures.
AGN fraction increases from 0% in starbursts to 23% in ULIRGs.
All galaxies are primarily powered by star formation.
Abstract
We present the first AGN census in a sample of 61 galaxies selected at 70microns, a wavelength which should strongly favour the detection of star-forming systems. For the purpose of this study we take advantage of deep Chandra X-ray and Spitzer infrared (3.6-160micron) data, as well as optical spectroscopy and photometry from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) survey for the Extended Groth Strip (EGS) field. We investigate spectral line diagnostics ([OIII]/Hbeta and [NeIII]/[OII] ratios, Hdelta Balmer absorption line equivalent widths and the strength of the 4000Ang break), X-ray luminosities and spectral energy distributions (SEDs). We find that the 70micron sources are undergoing starburst episodes and are therefore characterised by a predominance of young stars. In addition, 13 per cent of the sources show AGN signatures and hence potentially host an AGN. When the…
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