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Table B.1.

Parameters of the OHM candidates from ALFALFA.

AGC Name OH Position beamF PAF beamC PAC ΔF σF σC
(J2000) (") × (") (°) (") × (") (°) (kHz) (mJy) (mJy)
102708 000337.0+253215 2.64×2.39 35.6 35.0×26.6 -45.7 48 0.82 1.07
102850 002958.8+305739 4.35×2.85 37 39.6×27.1 -55.9 48 1.07 1.53
114732 010110.7+094626 3.66×2.79 42.3 40.2×31.9 -73.1 48 0.93 1.50
115713 014135.19+165730.73* 2.55×2.02 41.8 36.4×28.2 -33.9 48 1.08 1.81
115018 015847.1+073159 3.12×2.32 52.1 34.6×32.5 -67.8 48 0.74 1.45
124351 021751.0+072447 4.14×2.60 63 46.0×30.3 80 48 0.72 1.42
749309 101102.9+274020 2.66×2.32 31.9 40.9×25.5 -30.4 48 0.70 1.13
219835 113034.2+322208 2.84×2.39 31 42.9×24.4 -42 48 1.33 3.15
249507 140340.34+295456.39* 2.64×1.72 37.3 36.2×23.6 -22.8 48 0.94 1.46
322231 223605.9+095743 3.31×2.53 55.1 39.3×30.8 -71.2 48 0.87 1.34

Notes: Col. 2: OH position from the ALFALFA survey by Haynes et al. (2018). The ’*’ sign stands for the OH position and is obtained by this work (see Fig. 1). Cols. 3-6: Beam FWHM using GMRT full array and GMRT central array, respectively. Col. 7: Channel width for binned 2 channels for improving the sensitivity. Cols. 8-9: Noise level for the channel images with the bandwidth listed in Col. 7.

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