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Table 4:   Parameters for YSOs in L1630N. Column 4: ^a the values estimated from our VIMOS spectra; ^b the values from Flaherty & Muzerolle (2008). Column 6: stellar bolometric luminosity derived from optical SED fitting (see Sect. 3.3.2). Column 9: classification based on the criteria in Appendix A. Column 11: aggregate/cluster population or distributed population. Columns 13-14: stellar masses and ages estimated using PMS evolutionary tracks from Dotter et al. (2008). Columns 16-18: accretion rates estimated with H, H, and He I 5876 Å emission line luminosities, respectively.

Table 5:   Parameters for YSOs in L1641. Column 4: ^a the values estimated from our VIMOS spectra; ^b the values from Allen (1995); ^c the values from Gâlfalk & Olofsson (2008). Column 6: stellar bolometric luminosity derived from optical SED fitting (see Sect. 3.3.2). Column 9: classification based on the criteria in Appendix A. Column 11: aggregate/cluster population or distributed population. Column 13-14: stellar masses and ages estimated using PMS evolutionary tracks from Dotter et al. (2008). Column 16-18: accretion rates estimated with H, H, and He I 5876Å emission line luminosities, respectively.

Table 6:   Photometric magnitudes of YSOs in L1630N.

Table 7:   Photometric magnitudes of YSOs in L1641.

Table 10:   The equivalent widths of emission lines on the optical spectra for YSOs in L1630N.

Table 11:   The equivalent widths of emission lines on the optical spectra for YSOs in L1641.

Table 16:   Photometric magnitudes for transition disk object candidates.