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First Insights into the Spitzer Wide‐Area Infrared Extragalactic Legacy Survey (SWIRE) Galaxy Populations
Author(s) -
Carol J. Lonsdale,
M. Polletta,
J. Surace,
D. L. Shupe,
Fan Fang,
C. K. Xu,
H. E. Smith,
Brian Siana,
M. Rowan-Robinson,
T. Babbedge,
Seb Oliver,
Francesca Pozzi,
Payam Davoodi,
F. N. Owen,
Deborah Padgett,
Dave Frayer,
T. H. Jarrett,
Frank J. Masci,
J. O’Linger,
T. Conrow,
D. Farrah,
G. Morrison,
Nick Gautier,
A. Franceschini,
S. Berta,
I. Pérez-Fournón,
E. Hatziminaoglou,
A. Afonso-Luis,
H. Dole,
G. J. Stacey,
S. Serjeant,
M. Pierre,
Matt Griffin,
Rick Puetter
Publication year - 2004
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.1086/423206
Subject(s) - physics , galaxy , astrophysics , redshift , photometric redshift , astronomy , infrared , luminous infrared galaxy , active galactic nucleus
We characterize the SWIRE galaxy populations in the SWIRE validation fieldwithin the Lockman Hole, based on the 3.6-24$\mu$ Spitzer data and deepU,g',r',r' optical imaging within an area ~1/3 sq. deg for ~16,000Spitzer-SWIRE sources. The entire SWIRE survey will discover over 2.3 milliongalaxies at 3.6$\mu$m and almost 350,000 at 24$\mu$m; ~70,000 of these will be5-band 3.6-24$\mu$ detections. The colors cover a broad range, generally wellrepresented by redshifted spectral energy distributions of known galaxypopulations, however significant samples of unusually blue objects in the[3.6-4.5]$\mu$m color are found, as well as many objects very red in the3.6-24$\mu$m mid-IR. Nine of these are investigated and are interpreted asstar-forming systems, starbursts and AGN from z=0.37 to 2.8, with luminositiesfrom L$_{IR}$=10$^{10.3}$ to 10$^{13.7}$ L$_{\odot}$Comment: Accepted for publication in the ApJ Supplements Spitzer Special Issue 17 pages, 4 figure

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