All Tables

• Table 1: WFI observations of the open cluster NGC 6611, obtained on 29 July 2000.
• Table 2: Results of the cross-identifications.
• Table 4: Number of stars in WFI and ACIS FOV and the number of X-ray sources with excesses in the infrared bands specified in the first column.
• Table 3: Part of the electronic multiband catalog.
• Table A.1: Zero-points, coefficients of the colors and temporal terms for the CCDs, used in the transformation (2).
• Table A.2: Coefficients of the position's polynomials used for the photometric calibration in all the CCDs.