Notes. The first column gives the band combination used to compute the SED, the second column gives the number of sources that are fitted. The third and fourth column separate the total number into disk-bearing and disk-less sources. The last row gives the overall numbers for the SED selection. We use the K_S to W3 range as the main SED fitting range to get the spectral index α, hence, only if a source is not covered in the K_S to W3 we use alternative band combinations, that follow after the first rows.