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Table 3

Surface photometry parameters.

Galaxy PA° e M B

UM422 51 0.36 86.7 11.4 −18.27
UM439 −22 0.37 34.9 3.4 −16.58
UM446 −45 0.22 16.9 2.5 −15.67
UM452 −64 0.36 32.9 4.1 −16.65
UM456 35 0.36 37.8 5.4 −16.99
UM461 90 0.03 17.9 1.7 −15.14
UM462 67 0.12 34.9 3.3 −16.93
UM463 27 0.36 9.0 1.1 −13.90
UM465 20 0.16 35.4 3.6 −17.53
UM477 −75 0.17 152.4 17.1 −19.84
UM483 56 0.25 19.0 3.4 −16.84
UM491 30 0.27 21.6 3.4 −16.87
UM499 90 0.58 114.5 19.0 −19.57
UM500 2 0.16 43.8 7.2 −17.82
UM501 35 0.40 30.9 4.9 −16.06
UM504 −16 0.24 16.4 2.6 −16.29
UM523A 69 0.42 59.8 5.0 −17.09
UM523B −9 0.11 38.8 3.2 −16.71
UM533 −6 0.25 55.8 4.5 −16.29
UM538 −11 0.23 16.9 1.4 −13.66
UM559 89 0.55 32.0 3.3 −15.60

Notes.The position angle (PA°) in degrees and the ellipticity (e) were obtained from the B band image and applied to the remaining filters. The radius where the mean surface brightness is μB ≈ 26.5 mag arcsec-2 is the Holmberg radius, rH, and is given in arcseconds and kpc. The absolute B magnitude, MB, is calculated from the area inside rH and has been corrected for Galactic extinction (Schlegel et al. 1998). The MB errors are identical to the errors of the apparent B magnitude in Table 4.

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