*  indicates indicate positional difference: 5-10arcsec for a single asterisk,
*  and 10-15arcsec for a double asterisk
a  Examination of the POSS plates, object colors, and magnitudes leads to this
a  identification, despite the positional disagreement.
b  Despite the approx. 1.5 arcsec positional discrepancy, this identification is
b  made on the basis of good agreement of object colors and magnitudes.
c  GSS 37's published position is 62 arcsec offset from BKLT 162642-242031.
d  BBRCG 6 and BBRCG 7 form a binary system unresolved by our survey.
e  BBRCG 8 and BBRCG 10 form a binary system unresolved by our survey.
f  GSS 40 is a blend of BKLT 162653-242229 and 162654-242231.
g  WL 21 and WL 22 are not listed in Wilking & Lada 1983 but are referred to in
g  Wilking et al. 1989.
h  BKLT 162658-243739E and W both fall within positional and photometric errors
h  of CRBR 51 = SKS 3-24.
i  Elias 28 is a pair of T-Tauri stars: BKLT 162658-244534 and 162658-244529
i  (Elias 1978).
j  VSSG 31 is a blend of BKLT 162704-242830 and 162706-242837.
k  VSSG 23 = Elias 30 both encompass the candidate 6[&farcs;]5 separation binary
k  pair BKLT 162710-241914 and 162710-241921
l  BKLT 162715-243843 = WL 20 is actually a triple system (M. Ressler 1996,
l  private commmunication) previously resolved as a binary.
m  VSSG 26 is a blend of these four sources, which include WL 3, WL 4, and WL 5.
n  SKS 3-55 is a candidate 3 arcsec separation binary composed of
n  BKLT 162731-243752 and 162731-243755.
o  VSSG 14 = Elias 36 is a blend of BKLT 162749-242522 and 162749-242540.
p  GY 426 = IRS 57 is a 4 arcsec separation binary candidate composed of
p  BKLT 162759-242159 and 162759-242202.
q  VSSG 15 = Elias 38 is a blend of BKLT 162809-242322 and 162810-242305.