BEACON eSpace at Jet Propulsion Laboratory >
JPL Technical Report Server >
JPL TRS 1992+ >
Please use this identifier to cite or link to this item:
|Title: ||Extremely red objects in the Lockman Hole|
|Authors: ||Wilson, G.|
Perez-Gonzalez, P. G.
Ivison, R. J.
Rigby, J. R.
Fazio, G. G.
Le Floch, E.
Engelbracht, C. W.
Gordon, K. D.
Hines, D. C.
Misselt, K. A.
Morrison, J. E.
Rieke, G. H.
Rieke, M. J.
|Issue Date: ||Sep-2004 |
|Publisher: ||The American Astronomical Society|
|Citation: ||The Astrophysical Journal Supplement Series, 154:107–111, 2004 September doi: 10.1086/422716|
|Abstract: ||We investigate extremely red objects (EROs) using near- and mid-infrared observations in five passbands (3.6 to 24 μm) obtained from the Spitzer Space Telescope, and deep ground-based R and K imaging. The great sensitivity of the Infrared Array Camera (IRAC) camera allows us to detect 64 EROs (a surface density of 2.90+/-0.36 arcmin-2 [3.6]AB<23.7) in only 12 minutes of IRAC exposure time, by means of an R-[3.6] color cut (analogous to the traditional red R-K cut). A pure infrared K-[3.6] red cut detects a somewhat different population and may be more effective at selecting z>1.3 EROs. We find ~17% of all galaxies detected by IRAC at 3.6 or 4.5 μm to be EROs. These percentages rise to about 40% at 5.8 μm, and about 60% at 8.0 μm. We utilize the spectral bump at 1.6 μm to divide the EROs into broad redshift slices using only near-infrared colors (2.2/3.6/4.5 μm). We conclude that two-thirds of all EROs lie at redshift z>1.3. Detections at 24 μm imply that at least 11% of 0.6<z<1.3 EROs and at least 22% of z>1.3 EROs are dusty star-forming galaxies.|
|Appears in Collections:||JPL TRS 1992+|
Items in DSpace are protected by copyright, but are furnished with U.S. government purpose use rights.