All Tables

Table 1: Aperture photometry obtained with a radius of 0.7 $^{\prime \prime }$ on the main clusters detected in NGC 5253. Typical errors are less than 0.03 mag.
Table 2: ISOCAM photometry of NGC 5253.
Table 3: The compiled spectral energy distribution of Cluster 5. Aperture size are listed when appropriate (i.e. mostly for single-beam measurements). A few telescopes and filter bandwidths are missing because we were unable to find the information in the original papers.
Table 4: Parameters of the best-fitting dusty model. In the acceptable range, we give an indication of the range of values that, while producing a worse fit, still correspond to a model reproducing the data within the photometric uncertainties.