Table 7: Data used for the SED-calculations, V-magnitude with references for each photometric observation. Observations on the WULBV (Walraven) photometric system can be found in deWinter et al. (2001) with the exception of HD 139614 and SU Aur. Observations in the 4 IRAS bands (11.8, 24.4, 58.6 and 101 $\mu $m) can be found in NASA RP-1190 (1988).
PMS star UBVRI JHKLM
HD 97048  8.461,5,11  8.461,5,11
UX Ori 10.9112 10.9212
HD 163296  6.9015, 6.885  6.9015, 6.885
V380 Ori 10.4811,10.4410 10.4811,10.4411
HK Ori 11.5211,11.6510 11.6311,11.6510
KK Oph 11.825 11.915
BF Ori 11.045 11.035
HR 5999  6.8110  6.8010
HD 139614  8.2614  8.2614
V351 Ori  8.925  8.925
HD 104237  6.609  6.609
BN Ori  9.6813  9.6813
CQ Tau  9.82,9.457  9.457
NX Pup 10.243, 10.643 10.143
AK Sco  8.95, 9.03, 8.96, 9.0410  8.95, 9.02, 9.0410
SU Aur  9.024, 9.098, 9.1512  9.024, 9.078, 9.1512
1: vandenAncker (1996) 9: Hu et al. (1989)
2: Berdyugin et al. (1990, 1992)    10: Kilkenny et al. (1985)
3: Brand et al. (1983) 11: Remijn (1980)
4: Cohen & Schwartz (1976) 12: Rydgren et al. (1976)
5: deWinter et al. (2001) 13: Shevchenko et al. (1997)
7: Eiroa et al. (2002) 14: Sylvester et al. (1967)
8: Eugenio & Mendoza (1966) 15: Thé et al. (1985a)

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