中文

VIMOS VLT深层调查:向IAB<=24公开发布1599个红移

天体物理学 2009-11-10 v1

摘要

This paper presents the VIMOS VLT Deep Survey around the Chandra Deep Field South (CDFS). We have measured 1599 new redshifts with VIMOS on the European Observatory Very Large Telescope - UT3, in an area 21x21.6 arcmin^2, including 784 redshifts in the Hubble Space Telescope - Advanced Camera for Surveys GOODS area. 30% of all objects with I_AB=24 have been observed independently of magnitude, indicating that the sample is purely magnitude limited. We have reached an unprecedented completeness level of 88% in terms of the ratio of secure measurements vs. observed objects, while 95% of all objects have a redshift measurement. A total of 1452 galaxies, 139 stars, 8 QSOs have a redshift identification, 141 of these being unsecure measurements. The redshift distribution down to I_AB=24 is peaked at a median redshift z=0.73, with a significant high redshift tail extending up to ~4. Several high density peaks in the distribution of galaxies are identified. In particular, the strong peak at z=0.735 contains more than 130 galaxies in a velocity range +/-2000 km/s distributed all across the transverse ~20 h^-1 Mpc of the survey. We are releasing all redshifts to the community, along with the cross identification with HST-ACS GOODS sources on the CENCOS database environment http://cencosw.oamp.fr.

关键词

引用

@article{arxiv.astro-ph/0403627,
  title  = {Modeling the Multiwavelength Spectra and Variability of BL Lacertae in 2000},
  author = {M. Boettcher and A. Reimer},
  journal= {arXiv preprint arXiv:astro-ph/0403627},
  year   = {2009}
}

备注

Accepted for publication in ApJ. Uses AASTEX LaTeX macros.41 pages, including 12 figures