Caltech Faint Galaxy Redshift Survey. VII. Data Analysis Techniques and Redshifts in the Field J0053+1234 | Zendy

Judith G. Cohen | Zendy; David W. Hogg | Zendy; M. A. Pahre | Zendy; R. D. Blandford | Zendy; P. L. Shopbell | Zendy; Kevin Richberg | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Caltech Faint Galaxy Redshift Survey. VII. Data Analysis Techniques and Redshifts in the Field J0053+1234

Author(s) -

Judith G. Cohen,

David W. Hogg,

M. A. Pahre,

R. D. Blandford,

P. L. Shopbell,

Kevin Richberg

Publication year - 1999

Publication title -

the astrophysical journal supplement series

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 3.546

H-Index - 277

eISSN - 1538-4365

pISSN - 0067-0049

DOI - 10.1086/313184

Subject(s) - redshift , physics , astrophysics , galaxy , redshift survey , sample (material) , spectral line , stars , field (mathematics) , astronomy , mathematics , pure mathematics , thermodynamics

We present the techniques used to determine redshifts and to characterize thespectra of objects in the Caltech Faint Galaxy Redshift Survey in terms ofspectral classes and redshift quality classes. These are then applied tospectra from an investigation of a complete sample of objects with $K_s<20$ magin a 2 by 7.3 arcmin^2 field at J005325+1234. Redshifts were successfullyobtained for 163 of the 195 objects in the sample; these redshifts lie in therange [0.173, 1.44] and have a median of 0.58 (excluding 24 Galactic stars).The sample includes two broad lined AGNs and one QSO.Comment: 20 pages, Latex, 3 figures, accepted for publication in the ApJ Supplement

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research