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Table 1.

Basic observational properties of our MUG sample from GAMA.

CATAID RA Dec zspec log10 Mstellar log10 ⟨Σ1.5 log10 ⟨Σe log10ρe
79071 219.96358837 0.11254047 0.1335 11.00 10.57 9.63 9.63
16143 217.73607469 0.74513527 0.1378 10.99 10.57 9.63 9.23
784327 178.74986841 −1.42614761 0.1625 11.12 11.00 10.16 10.16
609701 176.87118407 0.31908043 0.1774 10.94 10.54 9.61 9.22
493286 220.3298223 −1.28795637 0.1849 11.00 10.94 10.12 10.12
319149 213.61987948 1.85908419 0.1881 11.30 10.94 10.03 9.66
84466 178.0554695 0.56305098 0.1973 11.18 10.91 10.02 10.02
178241 179.75149717 −1.93248107 0.2059 11.02 10.51 9.54 9.54
93202 219.52825636 0.53898409 0.2104 10.94 10.61 9.70 9.36
63726 216.76230139 −0.29771 0.2223 11.06 10.77 9.87 9.55
765033 223.44512218 0.14390729 0.2360 10.95 10.61 9.69 9.33
4220443 181.69997991 −1.98105929 0.2541 11.11 10.99 10.14 9.94
422365 130.57463302 2.59286311 0.2582 11.53 11.05 10.09 9.64
71471 184.92124534 0.02897459 0.2592 11.04 10.89 10.05 10.05
3873542 129.17293417 −1.27914494 0.2609 11.19 10.81 9.89 9.51
300986 131.463188 1.15208397 0.2663 11.02 11.29 10.58 10.58
221269 185.47490703 1.6248479 0.2671 10.94 10.53 9.60 9.60
288762 180.01770455 1.78508059 0.2751 11.17 10.81 9.89 9.89
138954 184.98809975 −1.74957511 0.2767 11.14
855304 131.15298472 1.36284576 0.2879 10.97 11.18 10.45 10.45
791716 181.36721636 −1.46390455 0.2886 11.06
693193 223.21201479 −0.3199314 0.2989 11.16 10.87 9.98 9.66

723783 223.09000412 2.4662566 0.1975 10.83 11.07 10.35 10.35
486049 218.39660186 −1.74897733 0.2242 10.90 10.46 9.51 9.51
388238 139.19204138 2.54304803 0.2291 10.79 10.66 9.82 9.82
55006 180.21098968 −0.39229633 0.2603 10.84 10.52 9.61 9.27
750374 214.89578661 0.6837029 0.2799 10.87 10.68 9.82 9.82
3173601 182.42594704 1.27935477 0.2874 10.79 10.80 10.01 10.01
365375 140.28918164 2.62257045 0.2874 10.85 10.49 9.57 9.57

Notes. The division line splits the galaxies with stellar mass greater or lower than 8 × 1010 M. Columns: (1) GAMA ID, (2) Right Ascension (J2000), (3) Declination (J2000), (4) Spectroscopic redshift, (5) Stellar mass, in units of log(M), (6) 2D stellar surface density according to the prescriptions in Barro et al. (2013), in units of log(M kpc−1.5), (7) 2D stellar surface density in units of log(M kpc−2), (8) 3D stellar density in units of log(M kpc−3). The quantities in Cols. (6–8) are averaged within the effective radius.

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