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Photometric Redshifts in the IRAC Shallow Survey
Author(s) -
M. Brodwin,
M. J. I. Brown,
M. L. N. Ashby,
Chao Bian,
Kate Brand,
Anirban Dey,
Peter Eisenhardt,
Daniel J. Eisenstein,
Anthony H. Gonzalez,
J.S. Huang,
Buell T. Jannuzi,
C. S. Kochanek,
Eric McKenzie,
S. S. Murray,
M. A. Pahre,
H. A. Smith,
B. T. Soifer,
S. A. Stanford,
Daniel Stern,
R. Elston
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/507838
Subject(s) - redshift , physics , astrophysics , galaxy , photometric redshift , redshift survey , population , flux (metallurgy) , astronomy , chemistry , demography , sociology , organic chemistry
Accurate photometric redshifts are calculated for nearly 200,000 galaxies toa 4.5 micron flux limit of ~13 uJy in the 8.5 deg^2 Spitzer/IRAC Shallowsurvey. Using a hybrid photometric redshift algorithm incorporating bothneural-net and template-fitting techniques, calibrated with over 15,000spectroscopic redshifts, a redshift accuracy of \sigma = 0.06(1+z) is achievedfor 95% of galaxies at 01) galaxy clusters.We present one such spectroscopically confirmed cluster at =1.24, ISCSJ1434.5+3427. Finally, we present a measurement of the 4.5 micron-selectedgalaxy redshift distribution.

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