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Table 2:

Surface photometry of the low-luminosity galaxy sample.

Galaxy 		$n_{i^{\prime}}$ $n_{r^{\prime}}$ $n_{g^{\prime}}$ $\mu_{0}\hspace{ -1pt}_{_{B}}$ $r_{e_{i^{\prime}}}$ $r_{e_{r^{\prime}}}$ $r_{e_{g^{\prime}}}$ $\chi_{\nu,i^{\prime}}^{2}$ $\chi_{\nu,r^{\prime}}^{2}$ $\chi_{\nu,g^{\prime}}^{2}$

N5846_01 		1.84(4) 1.82(3) 1.64(3) 17.1(2) 1.6(4) 1.7(3) 1.6(3) 0.00043 0.00025 0.00055
N5846_02 1.12(3) 1.06(2) 1.10(2) 22.6(1) 6.9(8) 6.9(6) 7.0(5) 0.00528 0.00317 0.00229
N5846_03 1.08(1) 1.14(2) 1.11(2) 21.8(1) 5.1(2) 5.7(4) 5.9(5) 0.0018 0.00325 0.00221
N5846_04 1.43(2) 1.53(2) 1.30(2) 21.63(9) 8.4(9) 9.5(9) 7.6(5) 0.00159 0.00064 0.00099
N5846_05 1.31(2) 1.27(1) 1.14(2) 21.79(9) 6.1(5) 6.3(3) 5.7(3) 0.00288 0.00109 0.00217
N5846_09 0.91(9) 1.09(9) 1.3(1) 22.3(6) 9(3) 10(4) 12(7) 0.00681 0.00957 0.0078
N5846_10 1.4(3) 2.0(7) 1.9(8) 23(4) - - - 0.00468 0.00335 0.00513
N5846_11 1.01(3) 1.15(3) 1.34(5) 20.7(2) 9.0(9) 10(1) 10(2) 0.00824 0.00925 0.01286
N5846_13 1.22(2) 1.33(1) 1.21(1) 21.52(6) 11.3(8) 12.3(5) 10.9(7) 0.00286 0.00065 0.00066
N5846_15 1.8(6) 1.20(8) 1.5(1) 22.2(6) - 10(3) 13(7) 0.0038 0.00293 0.00142
N5846_16 1.42(2) 1.45(2) 1.43(2) 21.8(1) 10.0(9) 10.1(8) 10(1) 0.001 0.00069 0.00106
N5846_17 0.97(6) 1.11(6) 0.95(3) 21.9(2) 6(1) 7(2) 5.6(7) 0.00375 0.00238 0.00143
N5846_21 1.37(2) 1.21(1) 1.35(1) 20.79(6) 11(1) 9.7(5) 10.8(6) 0.00332 0.00085 0.0015
N5846_22 1.23(2) 1.23(2) 1.18(2) 21.8(1) 5.2(4) 5.3(3) 5.3(4) 0.00354 0.00212 0.00356
N5846_23 1.41(3) 1.31(3) 1.22(2) 21.9(1) 9(1) 8(1) 8.7(7) 0.00163 0.00327 0.00156
N5846_24 0.98(2) 0.93(1) 0.90(2) 21.72(9) 8.0(5) 7.7(4) 7.7(5) 0.00107 0.00118 0.0026
N5846_25 1.09(1) 1.02(1) 0.97(1) 21.18(5) 6.5(3) 6.3(3) 6.4(2) 0.00508 0.00374 0.0028
N5846_27 0.91(3) 0.81(2) 0.84(4) 22.4(2) 6.9(7) 6.0(5) 6.3(9) 0.00099 0.00075 0.0024
N5846_28 0.80(1) 0.81(1) 0.89(2) 21.05(9) 6.5(4) 6.0(3) 5.8(4) 0.00345 0.00289 0.00406
N5846_31 1.02(6) 1.10(5) 1.07(8) 22.2(4) 8(2) 9(2) 8(2) 0.00173 0.0018 0.00227
N5846_32 0.99(2) 0.99(1) 1.05(2) 21.83(9) 10.9(9) 11.3(7) 11.9(9) 0.0016 0.00131 0.00168
N5846_33 0.78(2) 0.79(2) 0.83(2) 23.3(1) 11(1) 12(1) 13(1) 0.00362 0.00173 0.00329
N5846_34 1.20(2) 1.23(3) 1.13(2) 22.5(1) 9.5(8) 10(1) 9.4(9) 0.00161 0.00255 0.00225
N5846_35 1.28(4) 1.26(3) 1.20(2) 22.2(1) 7(1) 7.1(9) 7.3(7) 0.00541 0.00358 0.00206
N5846_37 1.3(1) 1.1(1) 1.2(1) 22.9(6) 11(6) 7(2) 10(6) 0.00111 0.00376 0.00245
N5846_38 1.08(5) 1.02(4) 1.21(5) 21.8(2) 4.0(6) 3.8(5) 4.4(7) 0.00575 0.00515 0.00399
N5846_39 0.74(6) 0.99(3) 1.19(9) 22.1(4) 6(1) 6.1(6) 7(2) 0.0024 0.0019 0.00173
N5846_40 1.15(7) 1.38(5) 1.18(6) 22.5(3) 10(3) 13(3) 9(2) 0.00661 0.0016 0.00416
N5846_43 1.3(2) 1.8(4) 1.2(2) 23(1) 6(5) - 4(3) 0.00621 0.00222 0.00715
N5846_46 1.36(4) 1.36(5) 1.45(5) 19.6(2) 3.4(6) 3.3(7) 3.3(8) 0.0148 0.0148 0.00764
N5846_47 0.87(2) 0.82(2) 0.85(2) 22.3(1) 11(1) 10.6(9) 11(1) 0.00337 0.00217 0.00371
N5846_50 1.17(4) 1.27(3) 1.35(4) 21.6(2) 5.5(8) 5.8(8) 6(1) 0.00782 0.00516 0.00784
N5846_51 1.05(2) 1.21(2) 1.19(2) 20.9(1) 4.9(3) 5.5(5) 5.4(4) 0.00177 0.0034 0.00283
N5846_52 1.14(4) 1.78(9) 1.41(5) 21.7(3) 8(1) 14(8) 10(3) 0.00397 0.00245 0.00322
N5846_56 1.10(2) 1.09(2) 1.10(2) 22.12(9) 15(1) 15(1) 15(1) 0.00268 0.00264 0.00186

Notes. Surface brightnesses are shown in magnitudes arcsec-2, effective radii in arcseconds. Numbers in parantheses indicate errors of the last significant digit. The quality of the fits is shown in the last three columns.


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