All Tables

Table 1: Diameters along the major axis, expressed as fractions of twice the truncation radius as given by van der Kruit & Searle, measured at various clip levels for 5 prominent edge-on galaxies that have clear evidence for truncations.
Table 2: Dimensions (in arcmin unless ratios) of edge-on galaxies in the van der Kruit & Searle sample as measured from the Sloan Digital Sky Survey and from the Digital Sky Survey 2 (red). The radius $R_{\rm max}$ is the truncation radius found by van der Kruit & Searle and has been listed for comparison. Values for radii and axis ratios have been rounded off to one decimal, but their ratios have been calculated before that.
Table 3: Results of the search for truncation radii and comparison to the results for the "hunting for warps'' of García-Ruiz et al. (2002). The galaxy types have been taken from that paper. The asterix in the third column indicates the galaxies for which the DSS2 had to be used. $R_{\rm H{\small I}}$ is the radius at which the face-on H I surface brightness is 1 $M_{\odot }$ pc^-2 and has been taken from García-Ruiz et al.
Table 4: Galaxies that have both a truncation in the stellar disk and a warp in the H I-layer and the parameter $R_{\rm warp}/R_{\rm max}$ .
Table 5: Distribution of the parameter $R_{\rm warp}/R_{\rm max}$ observed and expected from random orientations. The bottom line shows the probability that the observed and expected numbers are drawn from the same distribution.
Table 6: Characteristics (from Fig. 7 in García-Ruiz et al. 2002) in of the rotation curve at the positions of the onset of the warps for the galaxies in Table 4.
Table A.1: Dimensions (in arcmin unless ratios) of edge-on galaxies in Holmberg's (1958) sample.