next up previous contents
Next: Possible Diffuse Sources Up: Diffuse Radio Sources in Previous: MOST Catalogue Data

Project Data

Cluster data that has been found or calculated as part of this project. Again, this data is best viewed using our web catalogue. The column headings are:
$\frac{1}{3}R_A$: 1/3 of the Abell radius, in arcminutes
z: redshift, from the ACO catalogue except where referenced otherwise (see table caption)
N: the number of radio sources $\ge$10 mJy within $\frac{1}{3}R_A$
fX: X-ray flux density in units of $10^{-12} \mbox{ erg s}^{-1} \mbox{cm}^{-2}$.
LX: X-ray luminosity in units of $10^{44} \mbox{ erg s}^{-1}$.
Ext: whether the cluster contains any extended emission - optical overlays were made for these clusters
Rating: for those clusters with a candidate diffuse source. See Section 3.4.
  The redshifts in this table are from the ACO catalogue [Abell et al.1989] except those marked. a - [Adami et al.1998]; b - [Collins et al.1995]; c - [Dalton et al.1994]; d - [Ebeling et al.1996]; e - [Einasto1997]; f - [Lambas et al.1992]; f* - et. al. [Lambas et al.1992]; g - [Mazure et al.1996]; h - [Melnick and Moles1987]; i - [Mould1991]; j - [Muriel et al.1990]; m - [Postman and Lauer1995]; l - [Unewisse1993]; m - [Vettolani et al.1990];

ACO $\frac{1}{3}R_A$ z ref. N XBACS REFLEX Ext Rating
A2717 11.3788 0.0498   4 9.5 1.01 7.762 0.811    
A2731 18.1624 0.0312   7         y  
A2799 8.9947 0.0630 a 2            
A2806 20.9102 0.0271   10     5.407 0.129 y  
A2819 7.5859 0.0747 g 2            
A2836 18.8889 0.0300 f 7            
A2854 9.2896 0.0610 a 4            
A2860 21.1443 0.0268   18         y  
A2870 22.6667 0.0250   13         y  
A2877 23.5131 0.0241   10 18.4 0.46 15.087 0.351 y  
A2911 28.0528 0.0202   10           2
A2954 10.0118 0.0566 g 4            
A3009 8.9805 0.0631   2         y  
A3027 7.4561 0.0760 c 1     3.300 0.810    
A3089 8.4325 0.0672 b 2            
A3093 9.6866 0.0585   2         y 2
A3100 8.9662 0.0632 f 2         y  
A3104 10.0295 0.0565 d 2 8.6 1.18 8.327 1.842    
A3108 8.9662 0.0632   1            
A3110 7.5055 0.0755   1            
A3111 6.8273 0.0830 a 3     29.217 7.141 y 1
A3122 8.3333 0.0680 a 2     6.414 1.110    
A3123 8.7179 0.0650   1            
A3125 9.5559 0.0593   4            
A3128 10.2286 0.0554   4 14.2 2.12 12.827 2.209 y  
A3133 10.4938 0.0540 f 3         y 1
A3135 8.9521 0.0633 g 3         y 2,3
A3144 13.3964 0.0423   2            
A3161 6.7061 0.0845 f* 3            
A3164 9.2744 0.0611   6 9.2 1.48 7.682 1.235 y 3
A3193 16.6667 0.0340   3            
A3202 14.6048 0.0388   3         y  
A3225 13.0870 0.0433   2         y  
A3266 9.5398 0.0594   7 48.5 6.15 49.501 7.550 y 1
A3301 10.5721 0.0536 g 6     7.581 0.934 y  
A3341 14.9123 0.0380 a 4 10.2 0.61 11.682 0.689    
A3351 6.9190 0.0819 g 6         y 2
A3356 8.1418 0.0696 f* 1            
A3372 7.0393 0.0805 f* 2         y 2
A3376 12.4542 0.0455   3 26.9 2.48 20.664 1.829 y 1
A3379 6.7061 0.0845 f* 0            
A3380 9.9941 0.0567   3     3.692 0.478    
A3381 20.0946 0.0282   13         y  
A3389 22.8495 0.0248   17 11.0 0.32     y 1
A3390 21.8790 0.0259 l 11 5.1 0.25 6.025 0.266 y  
A3392 10.2471 0.0553 l 2     10.044 1.287    
A3407 13.6876 0.0414 l 3            
A3408 14.0962 0.0402 l 8 7.2 0.5        
A3497 9.3049 0.0609 e 6 9.1 1.45 6.518 1.311    
A3505 7.0393 0.0805 f* 1         y 2
A3537 33.9321 0.0167   27            
A3553 11.2434 0.0504 m 3         y 2
A3556 11.9298 0.0475 f 5 9.1 0.94        
A3558 11.7566 0.0482   5 64.6 6.27 58.386 5.830 y  
A3560 11.4478 0.0495 i 4 14.0 1.32 14.251 1.347    
A3562 11.3560 0.0499   3 30.8 3.33 24.555 2.659 y  
A3564 11.5176 0.0492 l 4         y  
A3566 11.4017 0.0497 m 5         y 2
A3570 15.2330 0.0372   5     5.950 0.332    
A3571 14.2737 0.0397 h 3 109.5 7.36 114.977 7.762    
A3572 13.9918 0.0405 m 3         y  
A3575 15.1921 0.0373 k 6         y  
A3603 9.2896 0.0610 j 5         y  
A3651 9.6372 0.0588   4     7.561 1.108 y  
A3667 10.6918 0.0530   7 73.1 8.76 70.627 9.280    
A3682 6.1527 0.0921 g 2            
A3687 7.4660 0.0759   1         y  
A3706 28.3333 0.0200   19         y  
A3716 12.4269 0.0456   7 11.8 1.01     y 1
A3742 34.3434 0.0165   22            
A3747 18.5185 0.0306   11         y  
A3756 6.7061 0.0845 f* 2         y  
A3771 7.1189 0.0796   2     5.099 1.390    
A3782 10.1735 0.0557   4         y  
A3785 7.3118 0.0775   4         y  
A3799 12.5092 0.0453 g 8         y  
A3806 7.5859 0.0747   0 6.1 1.47 7.136 1.710    
A3809 9.1398 0.0620 a 3 13.2 2.25 9.276 0.900    
A3816 16.0985 0.0352   2     4.161 0.199 y  
A3822 7.4561 0.0760   1 16.2 3.99 15.994 3.972    
A3825 7.6165 0.0744   5 7.5 1.78 8.173 1.942    
A3826 7.5155 0.0754   2            
A3849 8.3579 0.0678   3         y  
A3851 10.7120 0.0529   7         y  
A3869 7.2650 0.0780 c 2 5.9 1.54 6.017 1.620 y  
A3879 25.2976 0.0224   10            
A3880 9.7533 0.0581 j 3 13.4 1.86     y 3
A3886 7.5556 0.0750   0            
A3895 9.6866 0.0585 b 3            
A3912 8.4451 0.0671 f 3            
A3925 10.9819 0.0516   1            
A4059 12.4269 0.0456   2 31.2 3.09 32.764 3.405    
                     

next up previous contents
Next: Possible Diffuse Sources Up: Diffuse Radio Sources in Previous: MOST Catalogue Data
Tara Murphy
1999-10-31