Open Access

Table E.1.

Photometric corrections.

# I R V
(mag) (mag) (mag)
1 0.47 ± 0.09 0.57 ± 0.08 0.58 ± 0.08
2 0.43 ± 0.11 0.42 ± 0.12 0.41 ± 0.15
3 0.36 ± 0.12 0.34 ± 0.18 0.37 ± 0.21
4 0.52 ± 0.06 0.58 ± 0.07 0.55 ± 0.07
5 0.29 ± 0.22 0.26 ± 0.12 0.22 ± 0.18
6 0.43 ± 0.14 0.47 ± 0.11 0.46 ± 0.11
7 0.44 ± 0.07 0.52 ± 0.11 0.56 ± 0.14
8 0.37 ± 0.25 0.42 ± 0.25 0.42 ± 0.17
9 0.49 ± 0.15 0.58 ± 0.14 0.62 ± 0.13
10 0.46 ± 0.11 0.53 ± 0.08 0.55 ± 0.06
11 0.44 ± 0.18 0.48 ± 0.36 0.48 ± 0.41
12 1.07 ± 0.05 1.18 ± 0.05 1.17 ± 0.08
13 0.37 ± 0.27 0.42 ± 0.31 0.41 ± 0.15
14 0.47 ± 0.08 0.54 ± 0.10 0.49 ± 0.13
15 1.27 ± 0.09 1.33 ± 0.06 1.31 ± 0.06
16 0.77 ± 0.11 0.86 ± 0.14 0.91 ± 0.15
17 0.65 ± 0.10 0.74 ± 0.13 0.75 ± 0.21
18 0.16 ± 0.19 0.20 ± 0.10 0.18 ± 0.09
19 0.93 ± 0.37 1.01 ± 0.02 1.05 ± 0.02
20 0.50 ± 0.03 0.58 ± 0.04 0.62 ± 0.06
21 0.54 ± 0.02 0.61 ± 0.05 0.65 ± 0.12
22 0.62 ± 0.27 0.72 ± 0.36 0.75 ± 0.06

Notes. Corrections are defined as mean differences between MUSE and WFI (Beccari et al. 2015) magnitudes. Provided uncertainties are standard deviations of the difference between MUSE and WFI magnitudes.

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