Emission lines were detected in 5 galaxies of the sample: UGC 4508, NGC 1889, NGC 3125, NGC 5237 and UGC 7354. Table 4 lists the detected emission lines of the respective galaxies and their properties. Analysis suggests photoionisation to be the main cause for the line emission, which is typical for H II regions.

The results for the stellar kinematics obtained for all 49 sample galaxies with absorption lines strong enough for fourier fitting are presented in the Appendix. The radial velocity and velocity dispersion profiles compare favorably with previously published measurements (Bender et al. 1994; Davies et al. 1983; Franx et al. 1989; Binney et al. 1990; Carollo & Danziger 1994a). The agreement of the kinematical profiles is for the major part within $1 \sigma$ deviation. For most of the galaxies of our sample no published h₃and h₄ are available for comparison.

Notes on individual objects:

IC 1729: Asymmetric radial velocity profile, central depression in the velocity dispersion profile.
NGC 1404: Disk without rotation within 0.1 $r_{\rm e}$ , velocity profile constant within 1 $r_{\rm e}$ , $h_3 \propto -v$ : typical example of decoupled central component kinematics.
UGC 4508: cE? High-intensity emission lines, low continuum.
NGC 1889: In interaction with the disklike galaxy NGC 1888, merger. The kinematic profiles overlap, resulting in a velocity dispersion profile and line strength increase outward. H $\alpha$ and [N II] line emission were detected, possibly from the neighboring galaxy. Liu & Kennicutt (1995) state NGC 1888 to be a spiral of the type Sa or Sb with dominent old stellar population and only weak line emission.
NGC 2663: Very small rotation, unusually high velocity dispersion. This galaxy is a massive brightest cluster member and characterized by very anisotropic dynamics (Carollo & Danziger 1994b). The galaxy also features a compact central radio source (Danziger & Goss 1983; Sadler et al. 1989).
NGC 2271: Kinematically decoupled central component within 1.5'' of the galaxy's center without rotation.
NGC 3078: Slightly asymmetric kinematically decoupled central component without rotation, also supported by a central depression in the Mg₂ profile (Carollo et al. 1993).
NGC 3125 = AM 1004-294: High intensity emission lines, low continuum. This is a bright, compact low-redshift galaxy in a cluster with regular outer isophotes and double knots, it is classified as an amorphous H II galaxy (Telles et al. 1997) or a blue compact dwarf (Marlowe et al. 1997).
NGC 3136: Counter-rotation disk 4'' away from the center of intensity with a diameter of 2''; significance is low.
NGC 3250: Counter-rotating disk 9'' away from the center of intensity with a diameter of 3'', h₃ $\propto$ -v, indicating decoupled central component kinematics (Bender et al. 1994). The Mg₂ profile of this galaxy also features a central depression (Carollo et al. 1993).
NGC 3268: This galaxy features rotation only at one side of the core probably due to the presence of dust. It also has a parsec-scale radio core (Slee et al. 1994). h₃ $\propto$ v, indicating a disk component (Bender et al. 1994).
NGC 3302: Dust lane along major axis.
NGC 3557B: Possible kinematically decoupled central component supported by the asymmetric rotational velocity profile and h₃ > 0, low significance because of low spatial resolution.
NGC 3636: E0 with low velocity dispersion ( $\sigma$ < 160 km s^-1).
NGC 3904: Rotation disk (r<6'') within the center, h₃ $\propto$ -v, indicating decoupled central component kinematics.
NGC 4105, NGC 4106 = AM 1204-292: Gravitational interaction, reciprocal influence of kinematics. NGC 4105 features decoupled fast rotation within 2'' of the galaxy's center, supported by the fact that h₃ resambles -v; NGC 4106 has an asymmetric rotational velocity profile and h₃ > 0. The latter is classified as lenticular in the ESO-Uppsala Sky Survey with a diffuse, round arm clearly visible, possibly produced by the interaction. RC3 classifies it for this reason as SBb, however the color is more consistent with an S0 (Reduzzi & Rampazzo 1996).
NGC 4697: Large E6 galaxy with only slight rotation, it also features a dust lane of intrinsically circular shape, located in the equitorial plane. The galaxy is flattened and may be an S0, the spheroidal part of NGC 4697 may well be a large bulge (Dejonghe et al. 1996).
NGC 5237 = AM 1334-423: Nearby irregular galaxy, high-intensity emission lines, low continuum. This galaxy is believed to be a remnant of a spiral which collided with Centaurus A (NGC 5128) 5 10⁸ yr ago, lost half its disk material, which now forms the conspicuous ring of gas and dust line in Centaurus A, and was ejected as a non-rotating shred of dusty, gas-rich disc material which appears as a blue irregular/starburst dwarf galaxy (Thomson 1992).
NGC 6861 = IC 4949: Unusually high velocity dispersion at the center, fast rotation. This is a massive S0 galaxy, possibly influenced by a bar component. This galaxy also features a compact radio source in its core (Slee et al. 1994).
UGC 7354 = A 1216+04: Only emission lines, no absorption lines detected. This is a blue compact dwarf (Papaderos et al. 1996) or a starburst galaxy (Campos-Aguilar & Moles 1991).

The ESO-Uppsala Sky Survey designates 25 galaxies as cluster members, 8 galaxies as group members, 3 galaxies as pairs (NGC 4105 with NGC 4106, NGC 5237 with a compact object) and 6 galaxies as field galaxies (IC 4797, NGC 2380, NGC 2865, NGC 2887, NGC 3302, NGC 3585). For 12 galaxies no such data was available.

Table 5 contains the most important measured or derived spectroscopic quantities of the sample galaxies. These mean parameters describe the individual galaxies sufficiently well for the investigation of correlations between different kinematic and non-kinematic properties and LOSVDs. All mean parameters refer to the galaxy properties within their effective radii.

Table 5: Measured spectroscopic parameters of the sample galaxies. Quantities marked with ^* are results of emission line measurements
galaxy $v_\textrm{\scriptsize sys}$ $v_\textrm{\scriptsize rot}$ ${\rm d}v/{\rm d}r_0$ $\sigma_0$ $\sigma_{\rm m}$ $\sigma_{{\rm e}/2}$ $\Delta\sigma_{{\rm e}/2}$ $(v/\sigma )^*$

[km s^-1] [km s^-1] [km s^-1 arcsec^-1] [km s^-1] [km s^-1] [km s^-1]

I1729 1441 $\pm$ 3 54 $\pm$ 4 21 $\pm$ 8 131 $\pm$ 7 130 $\pm$ 9 127 $\pm$ 18 -0.03 $\pm$ 0.14 0.45 $\pm$ 0.05

N1404 1834 $\pm$ 4 113 $\pm$ 10 1 $\pm$ 9 259 $\pm$ 5 247 $\pm$ 4 216 $\pm$ 10 -0.17 $\pm$ 0.04 1.30 $\pm$ 0.11

N1427 1417 $\pm$ 3 63 $\pm$ 10 9 $\pm$ 5 157 $\pm$ 4 150 $\pm$ 8 150 $\pm$ 8 -0.05 $\pm$ 0.06 0.61 $\pm$ 0.10

N1537 1407 $\pm$ 2 176 $\pm$ 8 18 $\pm$ 4 138 $\pm$ 4 121 $\pm$ 4 102 $\pm$ 11 -0.26 $\pm$ 0.08 2.03 $\pm$ 0.11

N1549 1198 $\pm$ 2 53 $\pm$ 12 0 $\pm$ 3 218 $\pm$ 3 191 $\pm$ 4 109 $\pm$ 11 -0.50 $\pm$ 0.05 0.61 $\pm$ 0.14

N1889 2406 $\pm$ 6 113 $\pm$ 13 9 $\pm$ 18 167 $\pm$ 11 -- -- -- --

2524 $\pm$ 8^* -- -- 89.4 $\pm$ 19.5^* -- -- -- --

N2271 2558 $\pm$ 6 263 $\pm$ 36 20 $\pm$ 7 237 $\pm$ 7 228 $\pm$ 8 235 $\pm$ 8 -0.01 $\pm$ 0.04 1.72 $\pm$ 0.24

N2325 2073 $\pm$ 5 9 $\pm$ 17 5 $\pm$ 17 206 $\pm$ 8 215 $\pm$ 13 179 $\pm$ 27 -0.13 $\pm$ 0.13 0.05 $\pm$ 0.09

N2380 1755 $\pm$ 4 68 $\pm$ 16 4 $\pm$ 10 200 $\pm$ 6 -- -- -- --

N2434 1358 $\pm$ 4 41 $\pm$ 15 7 $\pm$ 10 189 $\pm$ 6 170 $\pm$ 8 152 $\pm$ 10 -0.20 $\pm$ 0.06 0.89 $\pm$ 0.33

I2311 1636 $\pm$ 4 30 $\pm$ 18 7 $\pm$ 8 211 $\pm$ 5 189 $\pm$ 5 143 $\pm$ 13 -0.32 $\pm$ 0.07 0.50 $\pm$ 0.30

U4508 1865 $\pm$ 8^* -- -- 44.9 $\pm$ 3.1^* -- -- -- --

N2663 (major axis) 1987 $\pm$ 8 35 $\pm$ 31 6 $\pm$ 19 329 $\pm$ 11 -- -- -- --

N2663 (PA=98 $^\circ$ ) 1951 $\pm$ 8 13 $\pm$ 19 3 $\pm$ 13 321 $\pm$ 9 -- -- -- --

N2699 1715 $\pm$ 3 73 $\pm$ 6 17 $\pm$ 5 152 $\pm$ 6 -- -- -- --

N2887 2843 $\pm$ 6 6 $\pm$ 20 2 $\pm$ 19 296 $\pm$ 8 267 $\pm$ 7 187 $\pm$ 9 -0.37 $\pm$ 0.04 0.03 $\pm$ 0.12

N2865 2529 $\pm$ 4 72 $\pm$ 15 1 $\pm$ 10 184 $\pm$ 5 182 $\pm$ 5 175 $\pm$ 8 -0.05 $\pm$ 0.05 0.67 $\pm$ 0.14

N2872 3117 $\pm$ 9 190 $\pm$ 50 8 $\pm$ 16 281 $\pm$ 13 248 $\pm$ 10 154 $\pm$ 29 -0.45 $\pm$ 0.11 1.98 $\pm$ 0.53

N2888 2342 $\pm$ 3 54 $\pm$ 9 14 $\pm$ 6 138 $\pm$ 7 140 $\pm$ 7 141 $\pm$ 9 0.02 $\pm$ 0.08 0.65 $\pm$ 0.11

N2986 2174 $\pm$ 7 57 $\pm$ 12 30 $\pm$ 10 282 $\pm$ 13 243 $\pm$ 14 206 $\pm$ 31 -0.27 $\pm$ 0.11 0.61 $\pm$ 0.13

N3078 2428 $\pm$ 5 99 $\pm$ 8 30 $\pm$ 18 305 $\pm$ 6 292 $\pm$ 9 255 $\pm$ 16 -0.16 $\pm$ 0.05 0.75 $\pm$ 0.06

N3087 2511 $\pm$ 4 34 $\pm$ 8 13 $\pm$ 5 259 $\pm$ 6 246 $\pm$ 7 192 $\pm$ 24 -0.26 $\pm$ 0.10 0.30 $\pm$ 0.07

N3136 1670 $\pm$ 5 10 $\pm$ 16 2 $\pm$ 16 226 $\pm$ 5 197 $\pm$ 5 115 $\pm$ 12 -0.49 $\pm$ 0.06 0.07 $\pm$ 0.12

N3125 1077 $\pm$ 11^* -- -- 51.9 $\pm$ 4.0^* -- -- -- --

N3224 2898 $\pm$ 8 94 $\pm$ 26 25 $\pm$ 10 216 $\pm$ 16 206 $\pm$ 13 172 $\pm$ 19 -0.20 $\pm$ 0.11 0.94 $\pm$ 0.26

N3250 2704 $\pm$ 5 132 $\pm$ 9 21 $\pm$ 10 298 $\pm$ 6 262 $\pm$ 6 188 $\pm$ 16 -0.37 $\pm$ 0.06 0.81 $\pm$ 0.06

N3258 2646 $\pm$ 5 39 $\pm$ 9 14 $\pm$ 14 357 $\pm$ 6 319 $\pm$ 6 267 $\pm$ 18 -0.25 $\pm$ 0.05 0.29 $\pm$ 0.07

N3260 2248 $\pm$ 6 211 $\pm$ 16 39 $\pm$ 12 174 $\pm$ 9 147 $\pm$ 10 106 $\pm$ 24 -0.39 $\pm$ 0.14 2.71 $\pm$ 0.27

N3268 2575 $\pm$ 6 211 $\pm$ 38 47 $\pm$ 21 197 $\pm$ 10 177 $\pm$ 10 122 $\pm$ 17 -0.38 $\pm$ 0.09 1.91 $\pm$ 0.36

N3302 3742 $\pm$ 10 18 $\pm$ 41 12 $\pm$ 15 379 $\pm$ 17 309 $\pm$ 21 148 $\pm$ 21 -0.61 $\pm$ 0.06 0.10 $\pm$ 0.22

N3309 4024 $\pm$ 6 17 $\pm$ 10 12 $\pm$ 9 282 $\pm$ 10 -- -- -- --

N3377 591 $\pm$ 2 86 $\pm$ 4 25 $\pm$ 7 135 $\pm$ 7 115 $\pm$ 8 81 $\pm$ 22 -0.40 $\pm$ 0.17 0.88 $\pm$ 0.07

N3557B 2723 $\pm$ 4 124 $\pm$ 7 32 $\pm$ 11 201 $\pm$ 6 -- -- -- --

N3557 2885 $\pm$ 7 217 $\pm$ 11 26 $\pm$ 7 363 $\pm$ 14 276 $\pm$ 7 181 $\pm$ 17 -0.50 $\pm$ 0.05 1.26 $\pm$ 0.07

N3585 1333 $\pm$ 2 157 $\pm$ 3 19 $\pm$ 4 232 $\pm$ 3 218 $\pm$ 3 220 $\pm$ 8 -0.06 $\pm$ 0.04 0.80 $\pm$ 0.02

N3617 1955 $\pm$ 3 99 $\pm$ 20 9 $\pm$ 4 111 $\pm$ 8 111 $\pm$ 7 109 $\pm$ 20 -0.02 $\pm$ 0.20 1.40 $\pm$ 0.30

N3636 1609 $\pm$ 4 8 $\pm$ 14 4 $\pm$ 6 114 $\pm$ 10 -- -- -- --

N3904 1592 $\pm$ 3 69 $\pm$ 7 18 $\pm$ 5 211 $\pm$ 4 195 $\pm$ 5 118 $\pm$ 14 -0.44 $\pm$ 0.07 0.57 $\pm$ 0.06

N3923 1639 $\pm$ 4 53 $\pm$ 13 4 $\pm$ 10 290 $\pm$ 4 275 $\pm$ 6 176 $\pm$ 22 -0.39 $\pm$ 0.08 0.27 $\pm$ 0.07

N4033 1452 $\pm$ 3 99 $\pm$ 8 10 $\pm$ 6 134 $\pm$ 4 142 $\pm$ 4 161 $\pm$ 12 0.20 $\pm$ 0.10 0.60 $\pm$ 0.05

N4105 2147 $\pm$ 3 158 $\pm$ 14 19 $\pm$ 8 181 $\pm$ 4 165 $\pm$ 4 133 $\pm$ 6 -0.27 $\pm$ 0.04 1.62 $\pm$ 0.15

N4106 1861 $\pm$ 4 10 $\pm$ 5 9 $\pm$ 11 230 $\pm$ 5 216 $\pm$ 6 169 $\pm$ 9 -0.27 $\pm$ 0.04 0.09 $\pm$ 0.05

U7354 1505 $\pm$ 18^* -- -- 46.1 $\pm$ 4.9^* -- -- -- --

N4261 2038 $\pm$ 5 12 $\pm$ 16 1 $\pm$ 13 356 $\pm$ 5 294 $\pm$ 4 224 $\pm$ 14 -0.37 $\pm$ 0.04 0.12 $\pm$ 0.16

N4697 (PA=100 $^\circ$ ) 1050 $\pm$ 3 97 $\pm$ 7 27 $\pm$ 4 187 $\pm$ 6 172 $\pm$ 9 164 $\pm$ 12 -0.12 $\pm$ 0.07 0.77 $\pm$ 0.07

N4697 (minor axis) 1088 $\pm$ 3 27 $\pm$ 10 6 $\pm$ 4 181 $\pm$ 4 174 $\pm$ 4 177 $\pm$ 11 -0.02 $\pm$ 0.06 0.21 $\pm$ 0.08

N5061 1931 $\pm$ 3 59 $\pm$ 13 2 $\pm$ 7 220 $\pm$ 4 213 $\pm$ 4 229 $\pm$ 13 0.04 $\pm$ 0.06 0.66 $\pm$ 0.15

N5237 302 $\pm$ 3^* -- -- 48.5 $\pm$ 1.0^* -- -- -- --

N5903 2528 $\pm$ 4 9 $\pm$ 17 4 $\pm$ 11 212 $\pm$ 6 194 $\pm$ 6 177 $\pm$ 16 -0.16 $\pm$ 0.08 0.08 $\pm$ 0.17

I4797 2635 $\pm$ 3 137 $\pm$ 6 28 $\pm$ 9 245 $\pm$ 5 219 $\pm$ 4 159 $\pm$ 12 -0.35 $\pm$ 0.05 0.56 $\pm$ 0.03

N6861 2752 $\pm$ 7 240 $\pm$ 10 45 $\pm$ 11 382 $\pm$ 7 340 $\pm$ 6 297 $\pm$ 19 -0.22 $\pm$ 0.05 0.96 $\pm$ 0.04

N7029 2703 $\pm$ 5 132 $\pm$ 7 29 $\pm$ 6 201 $\pm$ 7 177 $\pm$ 6 106 $\pm$ 12 -0.48 $\pm$ 0.06 0.82 $\pm$ 0.05

N7049 2183 $\pm$ 5 171 $\pm$ 17 20 $\pm$ 12 267 $\pm$ 7 220 $\pm$ 7 114 $\pm$ 23 -0.57 $\pm$ 0.09 1.16 $\pm$ 0.12

N7196 2800 $\pm$ 7 243 $\pm$ 25 40 $\pm$ 18 260 $\pm$ 12 234 $\pm$ 9 229 $\pm$ 24 -0.12 $\pm$ 0.10 1.76 $\pm$ 0.19

I5297 2831 $\pm$ 6 113 $\pm$ 25 5 $\pm$ 19 267 $\pm$ 7 -- -- -- --

galaxy	$v_\textrm{\scriptsize sys}$	$v_\textrm{\scriptsize rot}$	${\rm d}v/{\rm d}r_0$	$\sigma_0$	$\sigma_{\rm m}$	$\sigma_{{\rm e}/2}$	$\Delta\sigma_{{\rm e}/2}$	$(v/\sigma )^*$
	[km s^-1]	[km s^-1]	[km s^-1 arcsec^-1]	[km s^-1]	[km s^-1]	[km s^-1]
I1729	1441 $\pm$ 3	54 $\pm$ 4	21 $\pm$ 8	131 $\pm$ 7	130 $\pm$ 9	127 $\pm$ 18	-0.03 $\pm$ 0.14	0.45 $\pm$ 0.05
N1404	1834 $\pm$ 4	113 $\pm$ 10	1 $\pm$ 9	259 $\pm$ 5	247 $\pm$ 4	216 $\pm$ 10	-0.17 $\pm$ 0.04	1.30 $\pm$ 0.11
N1427	1417 $\pm$ 3	63 $\pm$ 10	9 $\pm$ 5	157 $\pm$ 4	150 $\pm$ 8	150 $\pm$ 8	-0.05 $\pm$ 0.06	0.61 $\pm$ 0.10
N1537	1407 $\pm$ 2	176 $\pm$ 8	18 $\pm$ 4	138 $\pm$ 4	121 $\pm$ 4	102 $\pm$ 11	-0.26 $\pm$ 0.08	2.03 $\pm$ 0.11
N1549	1198 $\pm$ 2	53 $\pm$ 12	0 $\pm$ 3	218 $\pm$ 3	191 $\pm$ 4	109 $\pm$ 11	-0.50 $\pm$ 0.05	0.61 $\pm$ 0.14
N1889	2406 $\pm$ 6	113 $\pm$ 13	9 $\pm$ 18	167 $\pm$ 11	--	--	--	--
	2524 $\pm$ 8^*	--	--	89.4 $\pm$ 19.5^*	--	--	--	--
N2271	2558 $\pm$ 6	263 $\pm$ 36	20 $\pm$ 7	237 $\pm$ 7	228 $\pm$ 8	235 $\pm$ 8	-0.01 $\pm$ 0.04	1.72 $\pm$ 0.24
N2325	2073 $\pm$ 5	9 $\pm$ 17	5 $\pm$ 17	206 $\pm$ 8	215 $\pm$ 13	179 $\pm$ 27	-0.13 $\pm$ 0.13	0.05 $\pm$ 0.09
N2380	1755 $\pm$ 4	68 $\pm$ 16	4 $\pm$ 10	200 $\pm$ 6	--	--	--	--
N2434	1358 $\pm$ 4	41 $\pm$ 15	7 $\pm$ 10	189 $\pm$ 6	170 $\pm$ 8	152 $\pm$ 10	-0.20 $\pm$ 0.06	0.89 $\pm$ 0.33
I2311	1636 $\pm$ 4	30 $\pm$ 18	7 $\pm$ 8	211 $\pm$ 5	189 $\pm$ 5	143 $\pm$ 13	-0.32 $\pm$ 0.07	0.50 $\pm$ 0.30
U4508	1865 $\pm$ 8^*	--	--	44.9 $\pm$ 3.1^*	--	--	--	--
N2663 (major axis)	1987 $\pm$ 8	35 $\pm$ 31	6 $\pm$ 19	329 $\pm$ 11	--	--	--	--
N2663 (PA=98 $^\circ$ )	1951 $\pm$ 8	13 $\pm$ 19	3 $\pm$ 13	321 $\pm$ 9	--	--	--	--
N2699	1715 $\pm$ 3	73 $\pm$ 6	17 $\pm$ 5	152 $\pm$ 6	--	--	--	--
N2887	2843 $\pm$ 6	6 $\pm$ 20	2 $\pm$ 19	296 $\pm$ 8	267 $\pm$ 7	187 $\pm$ 9	-0.37 $\pm$ 0.04	0.03 $\pm$ 0.12
N2865	2529 $\pm$ 4	72 $\pm$ 15	1 $\pm$ 10	184 $\pm$ 5	182 $\pm$ 5	175 $\pm$ 8	-0.05 $\pm$ 0.05	0.67 $\pm$ 0.14
N2872	3117 $\pm$ 9	190 $\pm$ 50	8 $\pm$ 16	281 $\pm$ 13	248 $\pm$ 10	154 $\pm$ 29	-0.45 $\pm$ 0.11	1.98 $\pm$ 0.53
N2888	2342 $\pm$ 3	54 $\pm$ 9	14 $\pm$ 6	138 $\pm$ 7	140 $\pm$ 7	141 $\pm$ 9	0.02 $\pm$ 0.08	0.65 $\pm$ 0.11
N2986	2174 $\pm$ 7	57 $\pm$ 12	30 $\pm$ 10	282 $\pm$ 13	243 $\pm$ 14	206 $\pm$ 31	-0.27 $\pm$ 0.11	0.61 $\pm$ 0.13
N3078	2428 $\pm$ 5	99 $\pm$ 8	30 $\pm$ 18	305 $\pm$ 6	292 $\pm$ 9	255 $\pm$ 16	-0.16 $\pm$ 0.05	0.75 $\pm$ 0.06
N3087	2511 $\pm$ 4	34 $\pm$ 8	13 $\pm$ 5	259 $\pm$ 6	246 $\pm$ 7	192 $\pm$ 24	-0.26 $\pm$ 0.10	0.30 $\pm$ 0.07
N3136	1670 $\pm$ 5	10 $\pm$ 16	2 $\pm$ 16	226 $\pm$ 5	197 $\pm$ 5	115 $\pm$ 12	-0.49 $\pm$ 0.06	0.07 $\pm$ 0.12
N3125	1077 $\pm$ 11^*	--	--	51.9 $\pm$ 4.0^*	--	--	--	--
N3224	2898 $\pm$ 8	94 $\pm$ 26	25 $\pm$ 10	216 $\pm$ 16	206 $\pm$ 13	172 $\pm$ 19	-0.20 $\pm$ 0.11	0.94 $\pm$ 0.26
N3250	2704 $\pm$ 5	132 $\pm$ 9	21 $\pm$ 10	298 $\pm$ 6	262 $\pm$ 6	188 $\pm$ 16	-0.37 $\pm$ 0.06	0.81 $\pm$ 0.06
N3258	2646 $\pm$ 5	39 $\pm$ 9	14 $\pm$ 14	357 $\pm$ 6	319 $\pm$ 6	267 $\pm$ 18	-0.25 $\pm$ 0.05	0.29 $\pm$ 0.07
N3260	2248 $\pm$ 6	211 $\pm$ 16	39 $\pm$ 12	174 $\pm$ 9	147 $\pm$ 10	106 $\pm$ 24	-0.39 $\pm$ 0.14	2.71 $\pm$ 0.27
N3268	2575 $\pm$ 6	211 $\pm$ 38	47 $\pm$ 21	197 $\pm$ 10	177 $\pm$ 10	122 $\pm$ 17	-0.38 $\pm$ 0.09	1.91 $\pm$ 0.36
N3302	3742 $\pm$ 10	18 $\pm$ 41	12 $\pm$ 15	379 $\pm$ 17	309 $\pm$ 21	148 $\pm$ 21	-0.61 $\pm$ 0.06	0.10 $\pm$ 0.22
N3309	4024 $\pm$ 6	17 $\pm$ 10	12 $\pm$ 9	282 $\pm$ 10	--	--	--	--
N3377	591 $\pm$ 2	86 $\pm$ 4	25 $\pm$ 7	135 $\pm$ 7	115 $\pm$ 8	81 $\pm$ 22	-0.40 $\pm$ 0.17	0.88 $\pm$ 0.07
N3557B	2723 $\pm$ 4	124 $\pm$ 7	32 $\pm$ 11	201 $\pm$ 6	--	--	--	--
N3557	2885 $\pm$ 7	217 $\pm$ 11	26 $\pm$ 7	363 $\pm$ 14	276 $\pm$ 7	181 $\pm$ 17	-0.50 $\pm$ 0.05	1.26 $\pm$ 0.07
N3585	1333 $\pm$ 2	157 $\pm$ 3	19 $\pm$ 4	232 $\pm$ 3	218 $\pm$ 3	220 $\pm$ 8	-0.06 $\pm$ 0.04	0.80 $\pm$ 0.02
N3617	1955 $\pm$ 3	99 $\pm$ 20	9 $\pm$ 4	111 $\pm$ 8	111 $\pm$ 7	109 $\pm$ 20	-0.02 $\pm$ 0.20	1.40 $\pm$ 0.30
N3636	1609 $\pm$ 4	8 $\pm$ 14	4 $\pm$ 6	114 $\pm$ 10	--	--	--	--
N3904	1592 $\pm$ 3	69 $\pm$ 7	18 $\pm$ 5	211 $\pm$ 4	195 $\pm$ 5	118 $\pm$ 14	-0.44 $\pm$ 0.07	0.57 $\pm$ 0.06
N3923	1639 $\pm$ 4	53 $\pm$ 13	4 $\pm$ 10	290 $\pm$ 4	275 $\pm$ 6	176 $\pm$ 22	-0.39 $\pm$ 0.08	0.27 $\pm$ 0.07
N4033	1452 $\pm$ 3	99 $\pm$ 8	10 $\pm$ 6	134 $\pm$ 4	142 $\pm$ 4	161 $\pm$ 12	0.20 $\pm$ 0.10	0.60 $\pm$ 0.05
N4105	2147 $\pm$ 3	158 $\pm$ 14	19 $\pm$ 8	181 $\pm$ 4	165 $\pm$ 4	133 $\pm$ 6	-0.27 $\pm$ 0.04	1.62 $\pm$ 0.15
N4106	1861 $\pm$ 4	10 $\pm$ 5	9 $\pm$ 11	230 $\pm$ 5	216 $\pm$ 6	169 $\pm$ 9	-0.27 $\pm$ 0.04	0.09 $\pm$ 0.05
U7354	1505 $\pm$ 18^*	--	--	46.1 $\pm$ 4.9^*	--	--	--	--
N4261	2038 $\pm$ 5	12 $\pm$ 16	1 $\pm$ 13	356 $\pm$ 5	294 $\pm$ 4	224 $\pm$ 14	-0.37 $\pm$ 0.04	0.12 $\pm$ 0.16
N4697 (PA=100 $^\circ$ )	1050 $\pm$ 3	97 $\pm$ 7	27 $\pm$ 4	187 $\pm$ 6	172 $\pm$ 9	164 $\pm$ 12	-0.12 $\pm$ 0.07	0.77 $\pm$ 0.07
N4697 (minor axis)	1088 $\pm$ 3	27 $\pm$ 10	6 $\pm$ 4	181 $\pm$ 4	174 $\pm$ 4	177 $\pm$ 11	-0.02 $\pm$ 0.06	0.21 $\pm$ 0.08
N5061	1931 $\pm$ 3	59 $\pm$ 13	2 $\pm$ 7	220 $\pm$ 4	213 $\pm$ 4	229 $\pm$ 13	0.04 $\pm$ 0.06	0.66 $\pm$ 0.15
N5237	302 $\pm$ 3^*	--	--	48.5 $\pm$ 1.0^*	--	--	--	--
N5903	2528 $\pm$ 4	9 $\pm$ 17	4 $\pm$ 11	212 $\pm$ 6	194 $\pm$ 6	177 $\pm$ 16	-0.16 $\pm$ 0.08	0.08 $\pm$ 0.17
I4797	2635 $\pm$ 3	137 $\pm$ 6	28 $\pm$ 9	245 $\pm$ 5	219 $\pm$ 4	159 $\pm$ 12	-0.35 $\pm$ 0.05	0.56 $\pm$ 0.03
N6861	2752 $\pm$ 7	240 $\pm$ 10	45 $\pm$ 11	382 $\pm$ 7	340 $\pm$ 6	297 $\pm$ 19	-0.22 $\pm$ 0.05	0.96 $\pm$ 0.04
N7029	2703 $\pm$ 5	132 $\pm$ 7	29 $\pm$ 6	201 $\pm$ 7	177 $\pm$ 6	106 $\pm$ 12	-0.48 $\pm$ 0.06	0.82 $\pm$ 0.05
N7049	2183 $\pm$ 5	171 $\pm$ 17	20 $\pm$ 12	267 $\pm$ 7	220 $\pm$ 7	114 $\pm$ 23	-0.57 $\pm$ 0.09	1.16 $\pm$ 0.12
N7196	2800 $\pm$ 7	243 $\pm$ 25	40 $\pm$ 18	260 $\pm$ 12	234 $\pm$ 9	229 $\pm$ 24	-0.12 $\pm$ 0.10	1.76 $\pm$ 0.19
I5297	2831 $\pm$ 6	113 $\pm$ 25	5 $\pm$ 19	267 $\pm$ 7	--	--	--	--

3 Results