All Tables

Table 1: Main data of the sample of 20 WR galaxies analyzed in this work.
Table 2: Journal of observations for broad-band optical filters. All exposure times are provided in seconds. Note that in some cases there are several observations per filter. Dates follow the format year/month/day.
Table 3: Log of our NIR observations, all completed at CST. Dates follow the format year/month/day.
Table 4: Log of the H $\alpha$ observations. Times are indicated in seconds. Dates follow the format year/month/day.
Table 5: Results for the broad-band optical/ NIR photometry of our WR galaxies sample. E(B-V) was determined from the C(H $\beta$ ) calculated from our optical spectra. All magnitudes and colors have been corrected for extinction; optical colors have been also corrected for the emission of the ionized gas. Except for NGC 5253, absolute magnitudes were computed using the distances provided by our optical spectra. See figures for the identification of the different regions inside galaxies.
Table 6: Correction for the contribution of the nebular emission in optical colors. Corrections have been done applying $(X-Y)_{\rm e}=(X-Y)-\Delta (X-Y)$ , being (X-Y) the color derived from photometry, $(X-Y)_{\rm e}$ the color corrected for emission lines and $\Delta (X-Y)$ the correction given in this table.
Table 7: Results of the H $\alpha$ photometry of the galaxies and regions analyzed in this work. The H $\alpha$ flux is corrected for both extinction and the contribution of the [N II] emission lines. Last column shows the age of the last starbursting episode derived comparing W(H $\alpha$ ) with the predictions given by Leitherer et al. (1999) models.