GaBoDS: the Garching-Bonn Deep Survey. III. Lyman-break galaxies in the Chandra Deep Field South

GaBoDS: the Garching-Bonn Deep Survey. III. Lyman-break galaxies in the Chandra Deep Field South
复制标题

GaBoDS:钱德拉深场南部的加兴-波恩深巡 III 莱曼断裂星系

DOI:
10.1051/0004-6361:20042544
复制
发表时间:
2005
影响因子:
6.5
通讯作者:
Hildebrandt
Hildebrandt
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Hildebrandt

文献摘要

参考文献

被引文献

相似文献

我们给出了我们在深CD马赛克图像中寻找高红移星系的第一个结果。作为更大规模调查的试点研究,使用WFI@MPG/ESO2.2m拍摄的钱德拉深场南部(CDF)的非常深的图像,采用Lyman-Break方法选择了1070个U波段和565个B波段辍学的大样本。这些Lyman-Break星系的数据以电子表格的形式公开。这些天体是Z~3和Z~4星系的良好候选者,这是由它们的光度学红移支持的。分析了这两个种群的视震级分布和聚集性,与前人的研究结果吻合较好。我们没有看到从z~3到z~4的连续聚类尺度长度的变化。在不久的将来,本文提出的技术将应用于整个调查中更大规模的U-辍学样本。
We present first results of our search for high-redshift galaxies in deep CCD mosaic images. As a pilot study for a larger survey, very deep images of the Chandra Deep Field South (CDFS), taken with WFI@MPG/ESO2.2m, are used to select large samples of 1070 U-band and 565 B-band dropouts with the Lyman-break method. The data of these Lyman-break galaxies are made public as an electronic table. These objects are good candidates for galaxies at z~3 and z~4 which is supported by their photometric redshifts. The distributions of apparent magnitudes and the clustering properties of the two populations are analysed, and they show good agreement to earlier studies. We see no evolution in the comoving clustering scale length from z~3 to z~4. The techniques presented here will be applied to a much larger sample of U-dropouts from the whole survey in near future.
加拿大-法国深田调查-II:莱曼断裂星系和z 3 处的星系团?
DOI: 10.1051/0004-6361:20031181
发表时间: 2003
影响因子: 6.5
作者:
S. Foucaud;H. McCracken;O. Fèvre;S. Arnouts;M. Brodwin;S. Lilly;D. Crampton;Y. Mellier
通讯作者: Y. Mellier
DOI: 10.1086/319715
发表时间: 2000
期刊: The Astrophysical Journal
影响因子: --
作者:
M. Giavalisco;M. Dickinson
通讯作者: M. Dickinson
莱曼断裂星系
DOI: 10.1146/annurev.astro.40.121301.111837
发表时间: 2002
影响因子: 33.3
作者:
M. Giavalisco
通讯作者: M. Giavalisco
C.A.诺曼:《天体物理学杂志》。
DOI: --
发表时间: --
期刊:
影响因子: --
作者:
通讯作者: --
斯巴鲁深场中 z=4 和 5 处莱曼裂痕星系的聚类:光度依赖性
DOI: --
发表时间: 2006
期刊: The Astrophysical Journal 637
影响因子: --
作者:
Takeshi Nishimura;Akichika Mikami;Juri Suzuki;Tetsuro Matsuzawa;西村剛;西村剛;Takeshi Nishimura;Takeshi Nishimura;Takeshi Nishimura;西村剛;西村剛;Takeshi Nishimura;Takeshi Nishimura;松下智直;Oka et al.;N.Kashikawa
通讯作者: N.Kashikawa