AEGIS: A panchromatic study of IRAC-selected extremely red objects with confirmed spectroscopic redshifts

We study 87 extremely red objects (EROs), selected both to have color redder than R - [3.6] = 4.0 and to have confirmed spectroscopic redshifts. Together, these two constraints result in this sample populating a fairly narrow redshift range at 0.76 < z < 1.42. The key new ingredient in...

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Bibliographic Details
Main Authors: Wilson, G, Huang, J, Fazio, G, Yan, R, Koekemoer, A, Salim, S, Faber, S, Lotz, J, Willmer, C, Davis, M, Coil, A, Newman, J, Conselice, C, Papovich, C, Ashby, M, Barmby, P, Willner, S, Ivison, R, Miyazaki, S, Rigopoulou, D
Format: Journal article
Language:English
Published: Institute of Physics Publishing 2007
Description
Summary:We study 87 extremely red objects (EROs), selected both to have color redder than R - [3.6] = 4.0 and to have confirmed spectroscopic redshifts. Together, these two constraints result in this sample populating a fairly narrow redshift range at 0.76 < z < 1.42. The key new ingredient included here is deep Spitzer Space Telescope Infrared Array Camera (IRAC) data. Based on [3.6] - [8.0] color, we demonstrate that it is possible to classify EROs as early-type galaxies, dusty starburst galaxies, or active galactic nuclei (AGNs; power-law types). We present ultraviolet-to-mid-infrared spectral energy distributions (SEDs) and Advanced Camera for Surveys (ACS) images, both of which support our simple IRAC color classification. © 2007. The American Astronomical Society. All rights reserved.