All Tables

Table 1: Photometry of the three EROs 1269, 822 and 850. Magnitudes are in the Vega system. Colors are measured within the aperture defined by the Ks-band isophote. The Ks-band magnitude is the MAG_AUTO measured by Sextractor.
Table 2: Parameters used to construct the grid of templates.
Table 3: Parameters resulting from the best fits of stellar population models to the photometric data for Sal, MS and Kro IMFs. The $\tilde\chi^2$ represent the reduced $\chi ^2$ . The model which formally provides the best fit (the lowest $\tilde\chi^2$ ) is marked with "*''. The V-band absolute magnitude has been derived by the Ks-band apparent magnitude. The absolute magnitudes in the Ks and in the V bands are corrected for the extinction.
Table 4: Ranges of stellar masses ( $\Delta\mathcal{M}_{\rm stars}^{\rm IMF}$ ) and of mass-to-Ks-band light ratios ( $\Delta M$ / $L_{K}^{\rm IMF}$ ) defined by the fitting models with different IMF (Sal, MS and Kro).