Table B.2: Shear-selected mass concentrations (part 1). The first column contains a label for the peak, and the second one indicates if the detection was made with either the S- or the P-statistics (or both). The next two columns contain the corresponding significances. The classification shows if along the line of sight an overdensity of galaxies is found, with class 1 meaning a very obvious overdensity, and class 6 no overdensity. The richness indicates how many galaxies were found as compared to the average density in this field, and we give the distance between the peak and the optical counterpart. Finally, we have the name of the survey field in which the detection was made, and possibly a redshift for the counterpart. An asterisk behind the redshifts indicates that it is based on the measurement of less than three galaxies.

Peak		 stat $\nu_{{\rm s}}~$ $\nu_{{\rm p}}~$ class rich dist scale $x_{\rm c}$ Field z

#001		 S 4.40   4 30 90 2 $.\!\!^{\prime}$8 2.0 SGP  
#002 S 4.09   4 20 90 2 $.\!\!^{\prime}$4 2.0 SGP  
#003 S 4.17   3 25 90 3 $.\!\!^{\prime}$6 2.0 SGP  
#004 SP 5.01 4.26 1 40 10 19 $.\!\!^{\prime}$8 0.025 SGP 0.257
#005 S 4.31   2 35 60 6 $.\!\!^{\prime}$3 0.05 SGP 0.5
#006 S 4.13   5 30 40 5 $.\!\!^{\prime}$6 0.025 SGP  
#007 S 4.15   5 50 0 5 $.\!\!^{\prime}$6 0.025 SGP  
#008 S 4.51   6     7 $.\!\!^{\prime}$9 2.0 SGP  
#009 S 4.22   2 40 20 3 $.\!\!^{\prime}$6 0.1 SGP  
#010 S 4.17   6     2 $.\!\!^{\prime}$0 2.0 FDF  
#011 S 4.09   5 20 60 1 $.\!\!^{\prime}$6 1.0 FDF  
#012 SP 4.64 8.53 5 15 60 5 $.\!\!^{\prime}$6 0.5 CDFS  
#013 P   4.09 5 20 60     CDFS  
#014 P   7.39 4 15 60     CDFS  
#015 P   4.08 4 30 10     CDFS  
#016 SP 4.12 5.34 5 15 60 2 $.\!\!^{\prime}$4 2.0 CDFS  
#017 S 4.02   2 30 50 2 $.\!\!^{\prime}$4 0.2 CDFS 0.135
#018 P   4.64 2 35 60     CDFS 0.146
#019 P   6.79 5 10 70     CDFS  
#020 P   5.98 6         CDFS  
#021 P   4.07 5 10 70     DEEP2E  
#022 P   4.35 5 10 50     DEEP2F  
#023 S 5.02   6     4 $.\!\!^{\prime}$8 0.2 AM1  
#024 S 4.05   4 25 90 9 $.\!\!^{\prime}$9 2.0 AM1  
#025 S 4.54   4 20 50 3 $.\!\!^{\prime}$2 0.2 AM1  
#026 S 4.10   5 10 50 2 $.\!\!^{\prime}$4 2.0 Comp  
#027 P   4.35 5 10 60     Comp  
#028 SP 4.39 5.05 6     4 $.\!\!^{\prime}$0 0.1 SHARC2  
#029 S 4.12   2 30 90 2 $.\!\!^{\prime}$0 2.0 SHARC2  
#030 P   6.58 3 30 30     A901  
#031 P   4.51 5 10 40     A901  
#032 P   4.37 5 10 30     A901  
#033 P   7.06 2 35 30     A901  
#034 P   5.59 3 20 30     A901 0.169*
#035 S 4.63   3 15 50 6 $.\!\!^{\prime}$3 2.0 A901  
#036 P   7.08 2 45 60     A901 0.161
#037 P   5.01 4 15 60     A901  
#038 P   4.60 4 25 50     A901  
#039 SP 6.30 10.01 1 50 70 19 $.\!\!^{\prime}$8 0.1 A901 0.161
#040 P   6.08 3 35 50     A901 0.165
#041 P   4.52 4 20 80     Pal3  
#042 S 4.13   3 25 40 2 $.\!\!^{\prime}$8 2.0 Pal3 0.189*
#043 P   5.14 4 20 40     Pal3 0.094, 0.123, 0.215
#044 P   4.26 3 30 40     CL1037-1243  
#045 P   5.00 6         CL1040-1155  
#046 S 4.19   2 40 70 2 $.\!\!^{\prime}$4 0.5 CL1040-1155  
#047 P 3.53 4.06 5 5 120     CL1040-1155  
#048 S 4.07   6     9 $.\!\!^{\prime}$9 1.0 CL1040-1155  
#049 S 4.18   5 5 80 5 $.\!\!^{\prime}$6 0.1 CL1054-1245 0.122*
#050 S 4.07   6     3 $.\!\!^{\prime}$6 0.05 CL1054-1146  

Source LaTeX | All tables | In the text