AEGIS: A Panchromatic Study of IRAC-selected Extremely Red Objects with Confirmed Spectroscopic Redshifts
arXiv:astro-ph/0608447 · doi:10.1086/517923
Abstract
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 into early-type, dusty starburst, or power-law (AGN) 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.
9 pages, 5 figures, ApJL AEGIS special edition, in press
References in corpus (24)
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- Infrared luminosity functions from the Chandra Deep Field South : the Spitzer view on the history of dusty star formation at 0<z<1
- Subaru Prime Focus Camera -- Suprime-Cam --
- A new photometric technique for the joint selection of star-forming and passive galaxies at 1.4<z<2.5
- Obscured and unobscured active galactic nuclei in the Spitzer Space Telescope First Look Survey
- A Significant Population of Red, Near-IR Selected High Redshift Galaxies
- The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1
- Spitzer Observations of Massive Red Galaxies at High Redshift
- A Census of Optical and Near-Infrared Selected Star-Forming and Passively Evolving Galaxies at Redshift Z~2
- Evolution and Color-Dependence of the Galaxy Angular Correlation Function: 350,000 Galaxies in 5 Square Degrees
- The DEEP Groth Strip Galaxy Redshift Survey. III. Redshift Catalog and Properties of Galaxies
- Spitzer observations of MAMBO galaxies: weeding out active nuclei in starbursting proto-ellipticals
- Mid-infrared properties of X-ray sources in the Extended Groth Strip
- Morphologies and Spectral Energy Distributions of Extremely Red Galaxies in the GOODS-South Field
- Simulating the Spitzer mid-IR color-color diagrams
- IRAC Imaging of Lockman Hole
- SPITZER Observations of z~3 Lyman Break Galaxies: stellar masses and mid-infrared properties
- Infrared Luminous Lyman Break Galaxies: A Population that Bridges LBGs and SCUBA Galaxies
- The relative abundances of ellipticals and starbursts among the Extremely Red Galaxies
- Far-infrared characterization of an ultra-luminous starburst associated with a massively-accreting black hole at z=1.15
- AEGIS: The Diversity of Bright Near-IR Selected Distant Red Galaxies
- Extremely Red Objects in The Lockman Hole
- AEGIS: Infrared Spectroscopy of An Infrared Luminous Lyman Break Galaxy at z=3.01
- AEGIS: Galaxy Spectral Energy Distributions from the X-Ray to Radio
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- The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets
- AEGIS20: a radio survey of the Extended Groth Strip
- The Evolution of Dusty Star Formation and Stellar Mass Assembly in Clusters: Results from the IRAC 3.6um, 4.5um, 5.8um and 8.0um Cluster Luminosity Functions
- The Faint and Extremely Red K-band Selected Galaxy Population in the DEEP2/Palomar Fields
- Far-infrared characterization of an ultra-luminous starburst associated with a massively-accreting black hole at z=1.15
- Host galaxy colour gradients and accretion disc obscuration in AEGIS z~1 X-ray-selected active galactic nuclei
- Classification of Extremely Red Objects in the COSMOS Field
- On the Stellar Populations in Faint Red Galaxies in the Hubble Ultra Deep Field
- Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
- The Clustering of Extremely Red Objects
- Classification of Extremely Red Objects in the Hubble Ultra Deep Field
- On the nature of red galaxies: the Chandra perspective
- Morphology and structure of extremely red objects at in the CANDELS-COSMOS field
- The Young Stellar Population of the Nearby Late-Type Galaxy NGC 1311