All Tables

• Table 1: Average angular offsets between the peak and the optical counterpart.
• Table B.1: The 58 fields used for this work.
• 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.
• Table B.3: Shear-selected mass concentrations (part 2).
• Table B.4: Shear-selected mass concentrations (part 3).
• Table B.5: Bright (classes 1 to 4) and dark (5-6) peaks for the various survey data sources. The columns contain the data source, the number of bright and dark peaks, the ratio between dark and bright peaks, the average exposure times and image seeing, the area covered, plus the number of bright and dark peaks per unit area. For the COMBO-17 field we give in parenthesis the corresponding values when the known structures are subtracted.
• Table B.6: Number of bright (classes 1-4) and dark (5-6) peaks and their ratios for the S- and the P-statistics.