Fig. 16 from The Chandra Deep Field–South: Optical Spectroscopy. I.

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Chandra Deep Field–South: Optical Spectroscopy. I.

Authors: G. P. Szokoly, J. Bergeron, G. Hasinger, I. Lehmann, L. Kewley, V. Mainieri, M. Nonino, P. Rosati, R. Giacconi, R. Gilli, R. Gilmozzi, C. Norman, M. Romaniello, E. Schreier, P. Tozzi, J. X. Wang, W. Zheng, and A. Zirm

Szokoly et al. 2004 The Astrophysical Journal Supplement Series 155 271.

Provider: AAS Journals

Caption: Fig. 16.

Redshift distribution of the various classes of X‐ray sources as well as their cumulative distribution. Object XID 138a and 138b are counted as two separate objects. The four extended objects (249, 566, 594, and 645) are not included. Two bin sizes (﹩\Delta z=0.01﹩ and 0.1) are selected to show the excess of objects around ﹩z=0.674﹩ and 0.734.

Other Images in This Article

Copyright and Terms & Conditions