Table 5
Stellar mass and mass-to-light ratio estimates for two regions: from the base of the mountaintop to μB = 25 mag arcsec−2, and 26 ≤ μB ≤ 28 mag arcsec−2 .
| LARS |  |
26 ≤ μB ≤ 28 | |||||||
|---|---|---|---|---|---|---|---|---|---|
 |
LB | M⋆ |  |
M/LB | LB | M⋆ |  |
 |
|
| M⊙∕L⊙ | 109 L⊙ | 109 M⊙ | M⊙∕L⊙ | 109 L⊙ | 109 M⊙ | 109 L⊙ | |||
| 01† | 0.35 | 3.48 | 1.22 | 0.20 | 0.40 | 0.57 | 0.23 | 0.04 | 6.10 |
| 02 | 0.30 | 3.22 | 0.97 | 0.41 | 0.65 | 0.62 | 0.40 | 0.17 | 2.35 |
| 03 | … | … | … | … | … | … | … | … | … |
| 04 | 0.30 | 9.82 | 2.91 | 0.23 | 0.28 | 0.52 | 0.15 | 0.01 | 12.90 |
| 05† | 0.28 | 1.76 | 0.49 | 0.11 | … | 0.34 | … | … | 4.27 |
| 06 | 0.26 | 2.04 | 0.54 | 0.26 | … | 1.20 | … | … | 2.09 |
| 07 | 0.22 | 3.99 | 0.87 | 0.18 | 0.19 | 0.79 | 0.15 | 0.03 | 4.75 |
| 08 | 1.30 | 19.64 | 25.52 | 0.27 | … | 4.04 | … | … | 93.30 |
| 09 | 0.66 | 28.32 | 18.78 | 0.37 | 0.77 | 1.95 | 1.50 | 0.03 | 51.00 |
| 10† | 1.19 | 10.51 | 12.55 | 0.58 | 1.22 | 1.38 | 1.68 | 0.08 | 21.50 |
| 11 | 0.51 | 92.40 | 47.18 | 0.39 | … | 8.41 | … | … | 121.00 |
| 12 | 0.14 | 7.18 | 1.02 | 0.14 | … | 0.98 | … | … | 7.41 |
| 13† | 0.62 | 34.87 | 21.62 | 0.37 | … | 15.37 | … | … | 59.20 |
| 14† | 0.17 | 6.55 | 1.12 | 0.64 | … | 3.40 | … | … | 1.75 |
Notes. The model M/LB ratios are averages across the region for the former case, and either averages or extrapolation for the latter (see text). M/LB ratios from the two-population mix are marked with †. Columns 
represent the fraction that the estimated mass makes up of the total stellar SED mass modeled by Hayes et al. (2014).
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