A population of extreme mid-to-near-infrared sources: obscured AGN and dusty starbursts

Details A population of extreme mid-to-near-infrared sources: obscured AGN and dusty starbursts A population of extreme mid-to-near-infrared sources: obscured AGN and dusty starbursts

2004-05-07

arxiv.org/abs/astro-ph/0405161v2

Astron.Astrophys. 427 (2004) 795-801

Astronomy and Astrophysics

Astrophysics

8 pages, 3 figures. A&A accepted version. Results unchanged but discussion is significantly expanded

Scientific paper

10.1051/0004-6361:20041616

We present a sample of mid-infrared detected sources from the European Large Area ISO Survey (ELAIS) regions characterised by strong mid-IR radiation with faint near-IR and optical counterparts. These extreme mid-to-near-IR objects (EMNOs) are defined here by a flux ratio of f_15um / f_2.2um > 25. This population is not obvious in deeper small area ISO surveys, though it produces more than 20% of the observed cosmic IR background radiation (CIRB) at 15um above 1 mJy. Near-future large area deep mid-IR surveys with the Spitzer Space Telescope, however, are bound to uncover large amounts of these objects, which we argue to most likely be obscured AGN, based on SED shapes and X-ray data. Very strong dusty starbursts at z>1 may also have high mid-to-near-IR flux ratios, but using the MIR/NIR and FIR/MIR ratios these may be separated. Most of our EMNOs appear to be ULIRGs, half are also extremely red objects (ERO). A curious case of a low redshift, less luminous object with a very young stellar population is also found. We predict that the simple broad band selection method makes EMNOs a useful window into high-redshift obscured nuclear activity and its sought after relation to star-formation, in a similar way that EROs have been used to define samples of high-redshift early type galaxies.

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