A medium-deep survey of a minislice at the north Galactic Pole .2. The data

被引:11
作者
Willmer, CNA
Koo, DC
Ellman, N
Kurtz, MJ
Szalay, AS
机构
[1] UNIV CALIF SANTA CRUZ,BOARD STUDIES ASTRON & ASTROPHYS,SANTA CRUZ,CA 95064
[2] HARVARD SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138
[3] JOHNS HOPKINS UNIV,DEPT PHYS,BALTIMORE,MD 21218
[4] OBSERV NACL,BR-20921030 RIO JANEIRO,BRAZIL
[5] UNIV CALIF SANTA CRUZ,UCO LICK OBSERV,SANTA CRUZ,CA 95064
[6] PRINCETON UNIV OBSERV,PRINCETON,NJ 08544
基金
美国国家科学基金会;
关键词
cosmology; observations; galaxies; distances and redshifts; photometry; surveys;
D O I
10.1086/192298
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report 328 redshifts, b(J) magnitudes, and b(J) - r(F) colors of galaxies measured in a redshift survey of a 4 degrees x 0 degrees.67 slice close to the north Galactic pole. The faintest galaxies in this survey have a magnitude of b(J) similar to 20.5. The redshifts present external errors of the order of 70 km s(-1), and we estimate that the mean photometry errors are similar to 0.2 for magnitudes and similar to 0.3 for colors. The redshift completeness level of the sample is of the order of similar to 35% at b(J) = 20, and part of this rather low completeness is the result of the combination of limitations imposed by the multifiber system with the clustering of galaxies, and an insufficient number of configurations, At the nominal magnitude limit of the survey, we were able to measure redshifts for similar to 70% of the galaxies we observed. From the correlation between observed properties of the galaxies in this sample, we demonstrate that the mean surface brightness is a major limiting factor in our ability to measure redshifts of faint objects.
引用
收藏
页码:199 / 215
页数:17
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