Description of source "G340.97-1.03" from Ellingsen (2007)

this new detection shows emission over a velocity range of more than 10 km s1, separated into three distinct groups.

Most of the spectral features have a ux density of a few Jy, with the strongest at about 10 Jy. The measured position of the maser is offset by 3.5 arcmin from the GLIMPSE source and so the two are very unlikely to be associated.