DEEP U BAND AND R IMAGING OF GOODS-SOUTH: OBSERVATIONS, DATA REDUCTION AND FIRST RESULTS

被引:155
作者
Nonino, M. [1 ]
Dickinson, M. [2 ]
Rosati, P. [3 ]
Grazian, A. [4 ]
Reddy, N. [2 ]
Cristiani, S. [1 ]
Giavalisco, M. [5 ]
Kuntschner, H. [6 ]
Vanzella, E. [1 ]
Daddi, E. [7 ]
Fosbury, R. A. E. [6 ]
Cesarsky, C. [8 ]
机构
[1] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[2] Natl Opt Astron Observ, Tucson, AZ 85719 USA
[3] European So Observ, D-85748 Garching, Germany
[4] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
[5] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
[6] ST ECF, D-85748 Garching, Germany
[7] CEA, Lab AIM, Irfu SAp, F-91191 Gif Sur Yvette, France
[8] CEA Saclay, Haut Commissaire Energie Atom, FR-91191 Gif Sur Yvette, France
关键词
galaxies: evolution; galaxies: high-redshift; LYMAN-BREAK GALAXIES; STAR-FORMING GALAXIES; HIGH-REDSHIFT GALAXIES; REST-FRAME ULTRAVIOLET; STELLAR MASS DENSITY; FAINT-END SLOPE; LUMINOSITY FUNCTIONS; STANDARD STARS; FIELD-SOUTH; FORMATION HISTORY;
D O I
10.1088/0067-0049/183/2/244
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present deep imaging in the U band covering an area of 630 arcmin(2) centered on the southern field of the Great Observatories Origins Deep Survey (GOODS). The data were obtained with the VIMOS instrument at the European Southern Observatory (ESO) Very Large Telescope. The final images reach a magnitude limit U-lim approximate to 29.8 (AB, 1 sigma, in a 1 '' radius aperture), and have good image quality, with full width at half-maximum approximate to 0 ''.8. They are significantly deeper than previous U-band images available for the GOODS fields, and better match the sensitivity of other multiwavelength GOODS photometry. The deeper U-band data yield significantly improved photometric redshifts, especially in key redshift ranges such as 2 < z < 4, and deeper color-selected galaxy samples, e.g., Lyman break galaxies at z approximate to 3. We also present the co-addition of archival ESO VIMOS R-band data, with R-lim approximate to 29 (AB, 1 sigma, 1 '' radius aperture), and image quality approximate to 0 ''.75. We discuss the strategies for the observations and data reduction, and present the first results from the analysis of the co-added images.
引用
收藏
页码:244 / 260
页数:17
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