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Table 1

Best-fit parameters describing the luminosity density distribution of the baryonic matter of 15 HSB spiral and 15 LSB galaxies.

ID z l(0)b k a0,b Nb qb l(0)d k a0,d Nd qd
(109L⊙/kpc3) (kpc) (107L⊙/kpc3) (kpc)
ESO215G391 0.014 0.349 ± 0.003 0.404 ± 0.013 0.956 ± 0.042 0.742 ± 0.040 3.113 ± 0.007 6.082 ± 0.002 0.432 ± 0.003 0.098 ± 0.010
ESO322G761 0.015 1.3 ± 0.003 0.720 ± 0.011 0.780 ± 0.022 0.810 ± 0.018 35.62 ± 0.07 3.5 ± 0.002 0.87 ± 0.003 0.100 ± 0.002
ESO322G771 0.008 7.3 ± 0.006 0.140 ± 0.001 1.300 ± 0.002 0.640 ± 0.006 42 ± 0.02 2.800 ± 0.002 0.760 ± 0.011 0.140 ± 0.003
ESO322G821 0.015 4.3 ± 0.001 0.21 ± 0.005 1.66 ± 0.02 0.66 ± 0.080 12.6 ± 0.01 8.58 ± 0.056 0.659 ± 0.006 0.08 ± 0.034
ESO323G251 0.014 2.309 ± 0.005 0.458 ± 0.005 0.535 ± 0.006 0.462 ± 0.008 56.58 ± 0.04 2.467 ± 0.002 1.055 ± 0.008 0.154 ± 0.002
ESO374G021 0.009 58.4 ± 0.001 0.07 ± 0.004 1.92 ± 0.04 0.66 ± 0.04 158.0 ± 0.01 1.48 ± 0.04 1.40 ± 0.018 0.08 ± 0.02
ESO375G121 0.010 55.4 ± 0.001 0.08 ± 0.003 1.80 ± 0.03 0.67 ± 0.05 88.3 ± 0.01 2.70 ± 0.029 1.33 ± 0.008 0.08 ± 0.01
ESO376G021 0.014 28.3 ± 0.01 0.095 ± 0.002 1.64 ± 0.02 0.67 ± 0.41 51.0 ± 0.01 3.20 ± 0.087 1.01 ± 0.02 0.08 ± 0.17
ESO383G021 0.021 56.056 ± 0.05 0.130 ± 0.002 1.20 ± 0.001 0.43 ± 0.04 16 ± 0.05 2.6 ± 0.003 1.200 ± 0.003 0.200 ± 0.005
ESO383G881 0.014 3.89 ± 0.05 0.100 ± 0.012 1.61 ± 0.089 0.68 ± 0.09 17.2 ± 0.00 5.61 ± 0.03 0.776 ± 0.005 0.08 ± 0.04
ESO445G191 0.016 6.048 ± 0.004 0.129 ± 0.003 1.519 ± 0.029 0.741 ± 0.054 12.40 ± 0.08 5.631 ± 0.008 0.744 ± 0.003 0.148 ± 0.002
ESO446G011 0.023 2.2 ± 0.001 0.740 ± 0.007 1.100 ± 0.017 0.42 ± 0.020 8.000 ± 0.006 4.4 ± 0.001 1.1 ± 0.007 0.19 ± 0.008
ESO502G021 0.013 23.5 ± 0.003 0.09 ± 0.001 1.60 ± 0.01 0.80 ± 0.043 106.8 ± 0.01 2.16 ± 0.023 1.06 ± 0.01 0.08 ± 0.010
ESO509G801 0.022 0.972 ± 0.001 0.666 ± 0.022 0.963 ± 0.031 0.986 ± 0.023 2.036 ± 0.001 11.304 ± 0.001 0.564 ± 0.005 0.265 ± 0.005
ESO569G171 0.013 3.815 ± 0.003 0.385 ± 0.023 0.590 ± 0.06 0.713 ± 0.063 174 ± 2 1.643 ± 0.067 0.902 ± 0.018 0.146 ± 0.011
ID z l(0)b k a 0,b N b q b l(0)d k a 0,d N d q d
(107L⊙/kpc3) (kpc) (106L⊙/kpc3) (kpc)
F561-12 0.016 2.235 ± 0.002 0.877 ± 0.098 1.045 ± 0.088 0.894 ± 0.085 1.731 ± 0.001 9.482 ± 0.036 0.138 ± 0.048 0.292 ± 0.016
F563-13,⋆ 0.012 61.08 ± 0.20 0.174 ± 0.015 2.128 ± 0.019 0.855 ± 0.019 – – – –
F568-34 0.019 1.561 ± 0.007 2.290 ± 0.014 0.649 ± 0.018 0.936 ± 0.028 6.368 ± 0.05 11.087 ± 0.02 0.251 ± 0.002 0.100 ± 0.002
F579-V13 0.021 1.639 ± 0.002 1.283 ± 0.026 0.574 ± 0.054 0.888 ± 0.051 7.342 ± 0.01 6.741 ± 0.004 0.601 ± 0.005 0.262 ± 0.007
F583-13,⋆ 0.008 6.059 ± 0.008 0.390 ± 0.004 1.629 ± 0.007 0.625 ± 0.006 – – – –
F730-V15 0.036 4.351 ± 0.01 1.120 ± 0.025 1.217 ± 0.031 0.816 ± 0.018 5.434 ± 0.02 9.404 ± 0.004 0.43 ± 0.076 0.11 ± 0.014
UGC1284 0.015 9.360 ± 0.005 0.356 ± 0.014 1.595 ± 0.026 0.869 ± 0.034 2.983 ± 0.051 11.362 ± 0.005 0.690 ± 0.08 0.190 ± 0.026
UGC12302 0.012 1.9 ± 0.05 0.818 ± 0.028 1.002 ± 0.027 0.60 ± 0.018 9.7 ± 0.004 4.3 ± 0.005 1.0 ± 0.045 0.11 ± 0.011
UGC57504 0.014 12 ± 0.05 0.270 ± 0.004 1.5 ± 0.021 1.0 ± 0.024 6.6 ± 0.003 8.8 ± 0.006 0.430 ± 0.051 0.13 ± 0.009
UGC66145 0.021 167.8 ± 0.5 0.270 ± 0.005 1.47 ± 0.016 0.65 ± 0.05 5.7 ± 0.03 15.8 ± 0.008 0.752 ± 0.069 0.08 ± 0.02
UGC103105 0.002 9.4 ± 0.01 0.44 ± 0.014 0.88 ± 0.044 0.71 ± 0.01 17.5 ± 0.001 1.4 ± 0.12 1.1 ± 0.06 0.12 ± 0.01
UGC114545 0.022 127.5 ± 5 0.206 ± 0.011 1.4 ± 0.062 0.80 ± 0.02 64.4 ± 0.001 3.47 ± 0.099 1.09 ± 0.031 0.09 ± 0.01
UGC116165 0.017 83.1 ± 0.01 0.545 ± 0.043 1.23 ± 0.096 0.66 ± 0.04 43.8 ± 0.002 5.5 ± 0.31 0.844 ± 0.069 0.08 ± 0.02
UGC117485 0.018 114.4 ± 5 0.980 ± 0.010 0.847 ± 0.014 0.80 ± 0.04 286.1 ± 0.5 3.1 ± 0.17 1.19 ± 0.046 0.08 ± 0.03
UGC118195 0.014 88.01 ± 0.1 0.197 ± 0.002 1.081 ± 0.013 0.991 ± 0.013 130 ± 1 5.789 ± 0.002 0.753 ± 0.015 0.113 ± 0.001

Notes. The surface brightness photometry of the galaxies that were fit with the models are taken from (1) Palunas & Williams (2000), (2) van der Hulst et al. (1993), (3) de Blok et al. (1996), (4) de Blok et al. (1995), and (5) Kim (2007). The superscript asterisk indicates galaxies for which a bulge component fully describes the surface brightness density.

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