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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. 5.

Comparing calculated ﹩L_{\mathrm{X}\,}﹩‐values in different cosmologies. Plotted are the changes as a function of redshift, compared to the current ﹩\Omega _{m}=0.3﹩, ﹩\Omega _{\Lambda }=0.7﹩, ﹩H_{0}=70﹩ km s−1 Mpc−1 cosmology. Dotted lines are slight variations on the two basic parameters, without changing the Hubble constant. The solid line is the now obsolete ﹩\Omega _{m}=1﹩, ﹩\Omega _{\Lambda }=0﹩, ﹩H_{0}=50﹩ km s−1 Mpc−1 cosmology. The result of an approximate formula (Pen 1999) for ﹩\Omega _{m}=0.3﹩, ﹩\Omega _{\Lambda }=0.7﹩, ﹩H_{0}=70﹩ km s−1 Mpc−1 is also shown (dashed line).

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