Table A.1.
Measured parameters for the sample of UDGs.
| Name | RA | Dec | q | PA | z | Ag | Ar | Re | R1 | RH | Log(M⋆/M⊙) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (deg) | (mag) | (mag) | (kpc) | (kpc) | (kpc) | ||||
| DF44 | 195.24167 | 26.97638 | 0.69 | 60.0 | 0.0231 | 0.034 | 0.024 | 3.31 | 4.34 | 3.33 | 8.16 |
| [KKS2000]04 | 40.44500 | −8.40258 | 0.87 | 40.0 | 0.0060 | 0.081 | 0.056 | 1.30 | 2.62 | 1.69 | 7.86 |
| UGC2162 | 40.09625 | 1.22917 | 0.77 | 25.0 | 0.0039 | 0.117 | 0.081 | 2.23 | 2.22 | 2.91 | 7.58 |
| UDG-B1 | 50.08800 | −1.17000 | 0.46 | 95.0 | 0.0212 | 0.213 | 0.148 | 3.93 | 4.11 | 6.94 | 7.90 |
| UDG-B3 | 49.96000 | −0.85500 | 0.86 | 41.0 | 0.0212 | 0.195 | 0.135 | 3.26 | 4.91 | 5.17 | 8.41 |
| UDG-B2 | 9.60000 | 1.10600 | 0.50 | 7.0 | 0.0141 | 0.060 | 0.041 | 1.76 | 1.92 | 3.28 | 7.29 |
| UDG-B4 | 9.88900 | 1.11500 | 0.67 | 107.0 | 0.0141 | 0.064 | 0.044 | 1.49 | 2.25 | 2.57 | 7.51 |
| UDG-B5 | 9.96900 | 0.38300 | 0.75 | 15.0 | 0.0141 | 0.058 | 0.040 | 2.95 | 4.06 | 4.64 | 8.11 |
| UDG-R1 | 9.97400 | 0.80800 | 0.64 | 167.0 | 0.0141 | 0.065 | 0.045 | 1.26 | 1.55 | 0.61 | 7.07 |
| UDG-R4 | 9.76900 | 1.09900 | 0.63 | 10.0 | 0.0141 | 0.059 | 0.041 | 1.52 | 1.61 | 1.22 | 7.30 |
| UDG-R5 | 358.61600 | 0.32200 | 0.59 | 120.0 | 0.0266 | 0.135 | 0.094 | 2.07 | 2.65 | 1.96 | 7.51 |
| UDG-R6 | 358.49700 | 0.45400 | 0.73 | 30.0 | 0.0266 | 0.135 | 0.093 | 1.78 | 3.95 | 2.55 | 8.03 |
Notes. We include the common name, position, axis ratio (q), and the position angle (PA) of the ellipses used to extract the surface brightness profiles (measured counter clockwise starting from the horizontal axis), the spectroscopic redshifts z (if available) of the galaxies (Román & Trujillo 2017b; Trujillo et al. 2017; van Dokkum et al. 2015b; Emsellem et al. 2019), Galactic extinctions both in the g and r bands (from NED), effective radius Re (measured in the g-band), the radial location R1 of the isomass contour at 1 M⊙ pc−2, the Holmberg Radius (RH; defined here using the isophote at 26 mag arcsec−2 in the g-band) and the stellar mass of galaxies (assuming a Chabrier IMF). The quantities are given showing only the significant figures up to which the values can be regarded reliable. The table for the dwarf galaxies is available in the online version of TCK20.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.