Table 4: Basic properties of the sample galaxies.

Ident.		 $V_{\rm HI}$ Spec. $M_{\rm HI}$ $M_{\rm HI}/L_B$ W50 MB
  km s-1 forma $10^{9}~M_{\odot}$ ${M}_\odot$/ $L_{\odot,B}$ km s-1 mag

ne-112		 11 014 LS 1.7 0.24 156 -19.1
ne-142 11 726 FT 1.8 3.7 128 -16.2
ne-178 11 591 DH 5.8 0.56 191 -19.5
ne-204 11 451 G 2.9 6.8 62 -16.0
ne-208 11 521 G 1.3 1.1 218 -17.1
ne-240 (11 645) - (1.7) (1.5) (262) -18.2
ne-250 11 686 FT 4.4 0.96 283 -19.8
ne-398 - - - - - -16.3
ce-042 11 910 DH 1.7 0.51 127 -17.2
ce-048 (11 145) - (1.9) (3.5) (171) -15.4
ce-060 (11 100) - (2.2) (2.1) (171) -
ce-061 (10 104) - (18.2) (7.3) (216) -
ce-143 11 603 G 0.74 0.35: 95 -18.0
ce-176 9919 LS 3.4 1.0 150 -18.3
ce-200 (9938) - (0.90) (0.43) (216) -17.6
sw-103 10 999 DH 0.95 1.1 155 -16.8
sw-194 (10 159) - (2.0) 15.7: (395) -14.8
sw-222 10076 G 4.2 0.35: 192 -19.8
47-138 (11 284) - (1.2) 0.30 (216) -18.4
47-154 (10 633) - (0.74) - (372) -
47-166 9887 DH 4.4 1.4 248 -15.0
47-211 10 460 DH 4.4 0.41 280 -19.8

a The H  I spectrum forms are: DH double horned, FT flat topped, G Gaussian, and LS lop-sided.

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