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Table 3

Colors and luminosities of MIR counterparts of methanol and non-methanol sources.

Name l b 1 rms LSR velocity range [3.6]–[4.5] [4.5]–[5.8] Luminosity (L) at
(deg) (deg) (mJy) (km s-1) 3.6 μ m 4.5 μm 5.8 μm

G037.7534-00.1892 37.753421 –0.189203 20 18; 108 2.21 1.43 0.91 3.82 7.88
G037.7540-00.1853 37.754001 –0.185311 80 18; 108 2.55 1.52 0.26 1.50 3.35
G037.7541-00.1874 37.754118 –0.187425 80 18; 108 1.51 0.21 0.46
G037.7510-00.1906 37.750999 –0.190664 80 18; 108 0.88 2.90 0.68 0.83 6.66
G037.7632-00.2150 37.763260 –0.215031 90 18; 108 2.16 1.13 10.56 41.84 65.51
G040.2819-00.2197 40.281918 –0.219794 10 18; 108 1.21 0.36 3.86 28.47 21.87
G040.4249+00.7000 40.424941 0.700050 22 30; 60 1.49 1.98 7.27 15.55 53.02
G040.4308+00.7062 40.430894 0.706228 90 30; 60 8.45 -
G040.4184+00.7039 40.418421 0.703903 80 30; 60 1.96 0.97 0.20 0.68 0.91
G041.1232-00.2203 41.123224 –0.220356 15 18; 108 1.19 0.85 1.38 -
G041.1566-00.1968 41.156641 –0.196881 10 18; 108 1.84 0.23 0.67 -
G041.1580-00.1941 41.158047 –0.194100 70 18; 108 0.26 1.50 4.59 3.17 6.94
G041.1565-00.1985 41.156513 –0.198536 70 18; 108 1.73 0.13 0.35 -
G041.1560-00.2010 41.156050 –0.201089 70 18; 108 2.04 0.39 0.13 0.48 0.38
G041.2261-00.1970 41.226184 –0.197014 15 18; 108 1.15 1.84 2.87 -
G041.3475-00.1364 41.347554 –0.136439 10 30; 60 1.30 3.54 6.46
G045.4671+00.0530a 45.467151 0.053064 7 18; 108 2.41 1.56 1.60 8.01 18.48
G045.4661+00.0457 45.466154 0.045739 60 18; 108 9.11
G045.4692+00.0511 45.469271 0.051114 60 18; 108 1.16 0.77 8.73 13.80 15.47
G045.4725+00.1335b 45.472562 0.133497 17 18; 108 1.30 13.90 25.48
G045.4699+00.1327 45.469912 0.132772 70 18; 108 2.11 1.12 4.30
G045.4925+00.1257 45.492565 0.125750 10 18; 108 2.23 0.19 0.26 1.10 0.72
G059.7828+00.0647 59.782861 0.064733 6 30; 60 1.85 0.07 54.14 161.88 83.85

Notes. The W49N region is omitted because of its methanol maser emission complexity and the lack of IR data at sufficient resolution. The MIR objects showing maser emission are in bold. Weak and diffuse 4.5 μm emission also appears from

(a)

G45.4547+00.05986 and

(b)

G45.47658+00.13171 and G45.46791+00.13492, but MIR flux densities are not listed in the GLIMPSE catalog owing to very extended and complex morphology.

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