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Table B.4:

Parameters of the 44 GHz CH3OH maser (Class I) detected with the Nobeyama 45-m telescope for both high (the IRAS name begins with H) and low (the IRAS name is begins with L) sources.

Sourcea
$V_{\rm LSR}$ $\int F_\nu {\rm d}V$ V $\Delta V$ $F_{\nu}^{\rm peak}$
  (km s-1) (Jy km s-1) (km s-1) (km s-1) (Jy)
H05168+3634 -15.1 1.12 $\pm$ 0.2 -4.9 $\pm$ 0.2 1.3 $\pm$ 0.4 0.80
H05480+2545 -9.3b 3.3 $\pm$ 0.1 -9.79 $\pm$ 0.02 0.77 $\pm$ 0.05 4.08
H06103+3030 15.6 2.7 $\pm$ 0.6 16.4 $\pm$ 0.7 5 $\pm$ 1.5 0.51
H18089-1732 32.9 10.9 $\pm$ 0.4 31.94 $\pm$ 0.01 0.86 $\pm$ 0.04 11.8
H18151-1208 32.8 2.2 $\pm$ 0.2 30.5 $\pm$ 0.1 1.5 $\pm$ 0.3 1.34
    2.0 $\pm$ 0.4 33.8 $\pm$ 0.2 2.1 $\pm$ 0.5 0.89
H18159-1648 22.1 4.0 $\pm$ 0.6 13.2 $\pm$ 0.1 0.9 $\pm$ 0.1 3.95
    10.9 $\pm$ 0.6 19.5 $\pm$ 0.1 1.0 $\pm$ 0.1 10.01
    15.8 $\pm$ 0.6 20.9 $\pm$ 0.1 1.0 $\pm$ 0.1 6.97
    31.4 $\pm$ 0.6 22.9 $\pm$ 0.1 0.9 $\pm$ 0.1 32.11
    18.5 $\pm$ 0.6 23.9 $\pm$ 0.1 0.6 $\pm$ 0.1 27.9
H18316-0602 42.2 6.6 $\pm$ 0.1 42.060 $\pm$ 0.008 0.62 $\pm$ 0.02 9.88
    1.6 $\pm$ 0.2 43.10 $\pm$ 0.04 0.70 $\pm$ 0.09 2.07
    2.9 $\pm$ 0.4 44.52 $\pm$ 0.09 1.6 $\pm$ 0.3 1.67
H18360-0537 102.3 6.7 $\pm$ 0.4 102.4 $\pm$ 0.1 2.83 $\pm$ 0.2 2.23
    1.6 $\pm$ 0.4 106.4 $\pm$ 0.3 1.9 $\pm$ 0.7 0.74
H18507+0121 57.1 10.0 $\pm$ 0.4 60.33 $\pm$ 0.04 1.3 $\pm$ 0.1 7.00
H18517+0437 43.7 3.1 $\pm$ 0.2 43.97 $\pm$ 0.05 1.1 $\pm$ 0.1 2.70
H19043+0726 58.9 2.5 $\pm$ 0.2 58.69 $\pm$ 0.03 0.65 $\pm$ 0.09 3.52
    1.1 $\pm$ 0.2 59.89 $\pm$ 0.08 0.7 $\pm$ 0.2 1.31
H19088+0902 59.6 10 $\pm$ 1 58.67 $\pm$ 0.07 2.2 $\pm$ 0.2 2.0
H19388+2357 34.6 1.8 $\pm$ 0.4 35.4 $\pm$ 0.2 1.6 $\pm$ 0.4 1.07
H20050+2720 6.4 2.0 $\pm$ 0.2 6.6 $\pm$ 0.1 1.8 $\pm$ 0.3 1.09
H20062+3550 0.6 2.5 $\pm$ 0.2 0.60 $\pm$ 0.06 1.0 $\pm$ 0.1 2.36
H20126+4104 -3.9 8.9 $\pm$ 0.4 -2.43 $\pm$ 0.04 2.0 $\pm$ 0.1 4.17
H20188+3928 1.5 2 $\pm$ 1 3 $\pm$ 1 3 $\pm$ 2 0.76
H21391+5802 0.4 4.2 $\pm$ 0.2 -0.49 $\pm$ 0.02 0.73 $\pm$ 0.08 5.33
    5.4 $\pm$ 0.4 6.6 $\pm$ 0.1 2.3 $\pm$ 0.3 2.25
H22506+5944 -51.5 3 $\pm$ 1 -51.3 $\pm$ 0.1 1.6 $\pm$ 0.6 1.81
    4 $\pm$ 2 -48 $\pm$ 1 5 $\pm$ 2 0.8
L00420+5530 -51.20 1.6 $\pm$ 0.4 -48.8 $\pm$ 0.3 2.0 $\pm$ 0.5 0.8
L18018-2426 10.5 241.1 $\pm$ 0.4 11.280 $\pm$ 0.003 0.669 $\pm$ 0.002 339
L18024-2119 0.5 10.0 $\pm$ 0.4 0.31 $\pm$ 0.02 1.28 $\pm$ 0.05 7.34
    3.1 $\pm$ 0.4 2.7 $\pm$ 0.1 2.3 $\pm$ 0.3 1.4
L18144-1723 47.3 42.1 $\pm$ 0.2 48.590 $\pm$ 0.005 1.54 $\pm$ 0.01 25.6
L18162-1612 61.8 5.1 $\pm$ 0.2 62.80 $\pm$ 0.03 0.84 $\pm$ 0.07 3.2
L18396-0431 97.3 1.0 $\pm$ 0.2 97.6 $\pm$ 0.1 1.0 $\pm$ 0.3 1.0
L19092+0841 58.0 4.0 $\pm$ 0.4 59.07 $\pm$ 0.4 5.7 $\pm$ 0.7 0.65
L23385+6053 -50.0 2.9 $\pm$ 0.4 -50.6 $\pm$ 0.3 3.2 $\pm$ 0.7 0.9

Notes.  (a) ``L'' and ``H'' indicate if the source belongs to the low or high sample; (b) from NH3 observations performed with the Nobeyama 45-m telescope.


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