Table 2: Details of the newly detected 6.7 GHz CH3OH masers. The first column lists the source name (associated IRAS source or the galactic coordinates). The next two columns give their J2000 equatorial coordinates. Column (4) shows the distances. Columns (5) and (6) present the integrated flux density and peak flux density. Columns (7) and (8) show the radial velocity of peak emission and the radial velocity range. Columns (9)-(11) present the infrared, CH3OH and H2O luminosities. The maser luminosities are calculated assuming isotropic emission.
$\textstyle \parbox{20mm}{% Source \\ name}$ $\textstyle \parbox{17mm}{% RA(2000)\\ \mbox{${\rm (^h\;\;\;^m\;\;\;^s)}$ }}$ $\textstyle \parbox{17mm}{% Dec(2000) \\ \mbox{$(\hbox{$^\circ$ }\;\;\;\hbox{$^\prime$ }\;\;\;\hbox{$^{\prime\prime}$ })$ }}$ $\textstyle \parbox{10mm}{% $D$\space \\ (kpc)}$ $\textstyle \parbox{15mm}{% $S_{\rm i}$\\ (Jy~km~s$^{-1}$ )}$ $\textstyle \parbox{10mm}{% $S_{\rm p}$\\ (Jy)}$ $\textstyle \parbox{10mm}{% $v_{\rm p}$\\ (km~s$^{-1}$ )}$ $\textstyle \parbox{12mm}{% $\Delta v$\\ (km~s$^{-1}$ )}$ $\textstyle \parbox{10mm}{% \par $L_{\rm IR}$\\ ($L_{\odot}$ )}$ $\textstyle \parbox{12mm}{% \par $L_{{\rm CH}_{3}{\rm OH}}$\\ ($L_{\odot}$ )}$ $\textstyle \parbox{10mm}{% \par $L_{{\rm H}_{2}{\rm O}}$\\ ($L_{\odot}$ )}$
05137+3919 $05\ 17\ 13.3$ +39 22 14 12.01 0.7 1.5 -16.2 -21.1, -16.0 6.1(4) 7.0(-7) 2.2(-4)
06446+0029 $06\ 47\ 12.9$ +00 26 07 6.01 2.8 1.6 48.6 42.7, 50.0 2.3(4) 7.0(-7) 1.5(-4)
18319-0802 18 34 38.2 -07 59 35 $2.8^{\ast}$ 2.2 2.1 35.7 31.0, 45.2 7.2(3) 1.2(-7) 4.5(-6)
18355-0650 18 38 14.3 -06 47 47 5.74 4.2 3.9 58.2 56.6, 62.1 7.4(5) 9.4(-7) 7.1(-6)
18403-0440 18 43 01.1 -04 36 41 3.34 0.3 1.0 20.1 19.8, 20.4 4.1(3) 2.3(-8) 3.2(-6)
G29.91-0.05 18 46 05.9 -02 42 27 $7.1^{\ast}$ 7.8 2.9 104.3 93.4, 105.3 -- 2.7(-6) 3.3(-5)
18479-0005 18 50 31.1 -00 01 54 13.02 1.3 1.5 27.4 24.9, 28.3 1.6(6) 1.5(-6) 9.0(-5)
20275+4001 20 29 24.9 +40 11 21 2.03 1.7 4.0 -6.9 -7.4, -6.5 6.7(4) 4.7(-8) 1.5(-5)
21306+5540 21 32 13.0 +55 52 56 8.61 1.5 1.1 -69.9 -73.7, -68.0 1.4(5) 7.8(-7) 9.9(-4)
22176+6303 22 19 18.3 +63 18 48 0.96 0.2 0.5 -2.0 -2.3, -1.1 2.4(4) 1.1(-9) 4.8(-7)
References for the distances:
1 Wouterloot et al. (1993). 2 Palagi et al. (1993). 3 Anglada et al. (1996). 4 van der Tak et al. (1999).
5 Wu et al. (2006). 6 Crampton & Fisher (1974).
$^{\ast}$ Heliocentric near kinematic distances.


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