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A. Gonzalez (Florida), A. Dey (NOAO), P. R. M. Eisenhardt (JPL), B. Jannuzi (NOAO), Y.-T. Lin (UIUC), E. McKenzie (Florida), J. J. Mohr (UIUC), S. N. Raines (Florida), S. A. Stanford (UC Davis, IGPP/LLNL), D. Stern (JPL), M. Brown (NOAO), R. J. Elston (Florida)
We present initial results from the FLAMINGOS Extragalactic Survey, a deep near-infrared imaging survey within the NOAO Deep Wide-Field Survey regions. This program is designed to study evolution of the galaxy and galaxy cluster populations out to z~. The field locations are selected to provide extensive overlap with observations at other wavelengths, and the target depths of the survey are Ks=20.5 and J=22 (Vega). The final observations for the survey were obtained in May, and final data reduction and quality assessment are nearing completion. During this talk we describe the initial science being done with the data set, highlight upcoming work, and discuss planned coordination with other surveys within the NDWFS region. Specific emphasis will be placed upon identification of galaxy clusters at z>1.
If you would like more information about this abstract, please follow the link to http://flamingos.astro.ufl.edu/extragalactic. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
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Bulletin of the American Astronomical Society, 36 #2
© YEAR. The American Astronomical Soceity.