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Fig. 5


NIBLES W20 H i line widths as a function of r-band luminosity, Lr, for all clear, non-confused detections. The red line indicates the upper envelope used in estimating the upper limits to total H i masses of our non-detections (see Table A.3) as a function of Lr, log(W20) = 0.62 + 0.21 log(Lr). The two sources (0117 and 2167; i.e., SHOC 30 and NGC 5675) which lie well above the line have exceptionally broad widths as they are either a merger or a possibly confused detection (see Appendix A).

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