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Home All issues Volume 508 / No 1 (December II 2009) A&A, 508 1 (2009) 107-115 Full HTML
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Table 2:

WMAP sample evolutionary properties.
      2H0 = 70, $\Omega_{\rm M} = 0.3$, $\Omega_{\rm\Lambda} = 0.7$     2H0 = 50, $\Omega _{\rm M} = 0$, $\Omega _{\rm\Lambda } = 0$    
Class Number     $\langle z \rangle$ $\langle V/V_{\rm max} \rangle$ $\tau $ $\langle V/V_{\rm max} \rangle$ $\tau $

FSRQ 		137 $1.13\pm0.05$ $0.614\pm0.025$ $0.35^{\rm +0.07}_{-0.05}$ $0.621\pm0.025$ $0.26^{\rm +0.05}_{-0.03}$
BL Lacs 24 $0.56\pm0.09^a$ $0.619\pm0.059^b$ $0.31^{\rm +0.21}_{-0.08}$ $0.626\pm0.059^b$ $0.24^{\rm +0.15}_{-0.05}$
Radio Galaxies 15 $0.08\pm0.04$ $0.610\pm0.074$ ...c $0.610\pm0.074$ ...c
Unclassified blazars 11 $0.77\pm0.16^d$ $0.703\pm0.087^e$ $0.22^{\rm +0.11}_{-0.04}$ $0.713\pm0.087^e$ $0.17^{\rm +0.07}_{-0.03}$
SSRQ 9 $0.50\pm0.14$ $0.626\pm0.096$ ...c $0.632\pm0.096$ ...c
a Excluding the 6 sources without redshift; b assuming $z = \langle z \rangle$ for the sources without redshift; c $\langle V/V_{\rm max} \rangle$ not significantly different (<2$\sigma $) from 0.5: no evolution assumed; d excluding the 6 sources without redshift; e assuming z equal to the mean blazar redshift for the sources without redshift.

Source LaTeX | All tables | In the text

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