Fig. 5.
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Comparison between the luminosity of the 5.29 GHz CH2NH megamasers (this work) and the OH megamasers from Darling & Giovanelli (2002) and Wiggins et al. (2016). No OH megamaser has been observed yet in IRAS 17578−0400. All galaxies are labeled, and the best fit linear relationship (
, R = 0.97) is shown with a blue dotted line. The shaded blue area represents the uncertainty in the best fit.
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