Table 2: Estimated luminosities and fluxes for the 18 dSph from Table 1. is the total luminosity and the luminosity from within the central 0.3 kpc. is the total flux and the flux from a central region subtending (about the angular resolution of Fermi above 3 GeV). The first number is the median over all subhalos matching the dSph distance and , the numbers in parentheses are the 16th and 84th percentiles. The table is ordered by decreasing .

Name
[kpc] [ ] [ ] [ ] [ ]

Segue 1 23 2.8 2.5 41 12
Ursa Major II 32 3.5 3.1 28 9.5
Ursa Minor 66 6.2 4.7 11 5.2
Draco 80 7.0 5.6 8.8 4.3
Carina 101 7.0 5.6 5.5 3.1
Wilman 1 38 0.88 0.85 4.9 2.6
Coma Berenices 44 1.2 1.1 4.8 2.5
Sculptor 80 2.9 2.5 3.7 2.0
Ursa Major I 106 3.3 2.5 2.3 1.3
Fornax 138 3.5 2.9 1.4 1.00
Sextans 86 1.2 1.1 1.3 0.86
Leo II 205 4.6 3.1 0.88 0.55
Canes Venatici I 224 4.6 3.1 0.73 0.48
Leo I 250 5.2 3.2 0.66 0.41
Hercules 138 1.4 1.2 0.57 0.42
Canes Venatici II 151 1.2 1.1 0.44 0.33
Leo T 417 3.5 2.2 0.16 0.12
Leo IV 158 0.14 0.13 0.043 0.039