Table 3.
Location of Redge for the galaxies in our sample.
| Name | Redge | μ(R =Redge) | μlim(3σ; area annulus at Redge) | Criteria | Rlast | ||||
|---|---|---|---|---|---|---|---|---|---|
| [″] | [kpc] | [mag arcsec−2] | [mag arcsec−2] | [″] | [kpc] | ||||
| FUV | NUV | FUV | NUV | ||||||
| NGC1042 | 180.0±3.8 | 11.78±0.25 | 28.95 | 28.50 | 31.40 | 31.48 | 1,2 | 260.0 | 17.02 |
| NGC2712 | 90.0±2.3 | 13.18±0.33 | – | 27.84 | – | 30.21 | 1 | 150.0 | 21.96 |
| NGC2903 | 450.0±3.8 | 21.82±0.18 | 29.71 | 29.00 | 31.20 | 31.01 | 1,2 | 620.0 | 30.06 |
| NGC3049 | 82.5±1.5 | 7.72±0.14 | 28.58 | 27.76 | 29.79 | 30.24 | 1 | 140.0 | 13.01 |
| NGC3198 | 400.0±3.8 | 25.02±0.24 | 29.26 | 29.21 | 32.61 | 32.35 | 1,2 | 580.0 | 36.27 |
| NGC3351 | 220.0±3.8 | 10.67±0.18 | 28.02 | 27.68 | 31.15 | 30.92 | 1,2 | 280.0 | 13.57 |
| NGC3368 | 255.0±3.8 | 13.85±0.21 | 29.27 | 28.33 | 31.58 | 31.99 | 2 | 400.0 | 21.72 |
| NGC3486 | 210.0±3.8 | 13.85±0.25 | 28.44 | 28.06 | 31.42 | 31.53 | 1,2 | 315.0 | 20.77 |
| NGC3596 | 140.0±1.5 | 7.67±0.08 | – | 28.63 | – | 30.33 | 1 | 160.0 | 8.77 |
| NGC3938 | 170.0±2.3 | 10.38±0.14 | – | 28.02 | – | 31.60 | 1 | 319.5 | 19.67 |
| NGC3972 | 105.0±1.5 | 10.59±0.15 | – | 27.43 | – | 29.05 | 1 | 130.0 | 13.11 |
| NGC4013 | 150.0±2.3 | 10.62±0.16 | 28.67 | 27.86 | 29.21 | 28.94 | 1 | 180.0 | 12.74 |
| NGC4220 | 40.0±1.5 | 3.94±0.15 | 26.25 | 25.33 | 29.30 | 29.37 | 1,2 | 110.0 | 10.83 |
| NGC4307 | 85.0±1.5 | 8.24±0.15 | 29.41 | 27.77 | 29.55 | 29.36 | 1 | 110.0 | 10.67 |
| NGC4321 | 280.0±3.8 | 20.63±0.28 | 30.17 | 28.81 | 31.94 | 31.85 | 1 | 420.0 | 30.95 |
| NGC4330 | 95.0±2.3 | 12.76±0.30 | 25.95 | 25.00 | 28.25 | 28.15 | 1 | 150.0 | 20.14 |
| NGC5248 | 280.0±3.8 | 20.23±0.27 | – | 29.40 | – | 31.14 | 1 | 330.0 | 23.84 |
| NGC5866 | 35.0±1.5 | 2.39±0.11 | 25.50 | 23.86 | 28.10 | 28.06 | 1,2 | 220.0 | 15.04 |
| NGC5907 | 330.0±3.8 | 26.40±0.30 | 26.71 | 26.38 | 29.58 | 30.87 | 1,2 | 600.0 | 48.00 |
| IC3211 | 37.5±0.8 | 15.45±0.31 | 27.95 | 27.72 | 30.31 | 30.04 | 1,2 | 45.0 | 18.54 |
Notes. The criteria used to select the location of the edge: sharp change on the outermost slope of the surface brightness profiles (1) and/or color reddening (2) are provided. The error bars on the location of the Redge correspond to half the width of the elliptical annuli used to derive the surface brightness profiles. The observed (neither corrected of inclination nor Galactic extinction) surface brightness at the edge of the galaxies (i.e., μFUV(Redge) and μNUV(Redge)) are included. Surface brightness limits in the equivalent area of the annuli where R=Redge are also provided. We also provide the last radii of the surface brightness profiles (Rlast), marked as a red ellipse on rightmost panels of Fig. 6. This radii corresponds to the last NUV point.
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