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Home All issues Volume 499 / No 3 (June I 2009) A&A, 499 3 (2009) 679-695 Full HTML
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Table 3:

Radio information of halos and mini halos taken from the literature and reanalyzed in this work with the exponential model fit.

Cluster		 Type Reference z kpc/'' FWHM I0 re re $\langle J\rangle$ $\chi^2_{\rm RED}$
          arcsec $\mu $Jy/arcsec2 arcsec kpc erg s-1 Hz-1 cm-3  

A2744		 H Govoni et al. (2001a) 0.3080 4.50 50 $3.05^{\rm +0.12}_{-0.12}$ $61^{\rm +2}_{-2}$ $275^{\rm +9}_{-9}$ $2.5^{\rm +0.17}_{-0.16}\times 10^{-42}$ 1.5

A665		 H Giovannini Feretti (2000) 0.1819 3.03 53 $1.09^{\rm +0.08}_{-0.08}$ $78^{\rm +6}_{-5}$ $236^{\rm +18}_{-15}$ $7.0^{\rm +1.0}_{-1.0}\times 10^{-43}$ 0.9

A2219		 H Bacchi et al. (2003) 0.2256 3.59 53 $1.10^{\rm +0.08}_{-0.08}$ $100^{\rm +5}_{-4}$ $359^{\rm +18}_{-14}$ $5.4^{\rm +0.6}_{-0.6}\times 10^{-43}$ 3.7

A2255		 H Govoni et al. (2005) 0.0806 1.50 25 $0.65^{\rm +0.02}_{-0.02}$ $135^{\rm +4}_{-4}$ $203^{\rm +6}_{-6}$ $3.4^{\rm +0.20}_{-0.19}\times 10^{-43}$ 4.8

A773		 H Govoni et al. (2001a) 0.2170 3.48 30 $0.75^{\rm +0.07}_{-0.07}$ $32^{\rm +3}_{-3}$ $111^{\rm +10}_{-10}$ $1.1^{\rm +0.24}_{-0.2}\times 10^{-42}$ 0.7

A545		 H Bacchi et al. (2003) 0.1540 2.64 45 $1.31^{\rm +0.15}_{-0.13}$ $57^{\rm +4}_{-4}$ $150^{\rm +11}_{-11}$ $1.2^{\rm +0.22}_{-0.19}\times 10^{-42}$ 0.6

A2319		 H Feretti et al. (1997) 0.0557 1.07 30 $1.11^{\rm +0.04}_{-0.04}$ $185^{\rm +7}_{-6}$ $198^{\rm +7}_{-6}$ $5.4^{\rm +0.35}_{-0.36}\times 10^{-43}$ 2.4

A2218		 H Giovannini Feretti (2000) 0.1756 2.94 35 $1.06^{\rm +0.34}_{-0.27}$ $26^{\rm +9}_{-6}$ $76^{\rm +26}_{-18}$ $2.0^{\rm +1.4}_{-0.9}\times 10^{-42}$ 1.0

A2163		 H Feretti et al. (2001) 0.2030 3.31 62 $2.23^{\rm +0.07}_{-0.07}$ $119^{\rm +2}_{-2}$ $394^{\rm +7}_{-7}$ $9.2^{\rm +0.4}_{-0.4}\times 10^{-43}$ 2.1

A401		 H Bacchi et al. (2003) 0.0737 1.38 45 $0.44^{\rm +0.06}_{-0.05}$ $79^{\rm +15}_{-11}$ $109^{\rm +21}_{-15}$ $4.1^{\rm +1.3}_{-1.0}\times 10^{-43}$ 0.7

A2254		 H Govoni et al. (2001a) 0.1780 2.98 45 $1.56^{\rm +0.22}_{-0.20}$ $80^{\rm +19}_{-13}$ $238^{\rm +57}_{-39}$ $9.7^{\rm +3.4}_{-2.8}\times 10^{-43}$ 1.1

RXJ1314		 H Feretti et al. (2005) 0.2439 3.81 45 $1.05^{\rm +0.31}_{-0.25}$ $42^{\rm +16}_{-10}$ $160^{\rm +61}_{-38}$ $1.2^{\rm +0.8}_{-0.5}\times 10^{-42}$ 0.1

RXJ1347		 MH Gitti et al. (2007) 0.4510 5.74 18 $26.0^{\rm +40.7}_{-15.4}$ $9^{\rm +3}_{-2}$ $52^{\rm +17}_{-11}$ $1.8^{\rm +0.7}_{-0.5}\times 10^{-40}$ 0.2

A2390		 MH Bacchi et al. (2003) 0.2280 3.62 20 $60.8^{\rm +27.0}_{-21.1}$ $10^{\rm +1}_{-1}$ $ 36^{\rm +4}_{-4} $ $3.1^{\rm +1.0}_{-0.8}\times 10^{-40}$ 1.2

Perseus		 MH Pedlar et al. (1990) 0.0179 0.36 45 $99.6^{\rm +10.9}_{-10.6}$ $64^{\rm +4}_{-3}$ $23^{\rm +1}_{-1}$ $3.6^{\rm +0.5}_{-0.5}\times 10^{-40}$ 2.4
Column 2: type of diffuse emission contained (H = halo, MH = mini halo); Col. 6: FWHM of the circular Gaussian beam; Col. 10: average radio emissivity over the volume of a sphere of radius 3re, k-corrected with $\alpha =1$.

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