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Fig. 6

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Maser luminosity versus the WISE MIR luminosity (upper panels for 3.4μm and 4.6 μm, lower panels for 12μm and 22 μm luminosity) of maser hosts. The Arecibo OHMs are shown in filled circles and other OHMs in filled triangles. The upper limits on OH line luminosity of the non-OHM sample were also presented (cross-triangles). The solid and the dashed line show linear fits without and with considering the Malmquist effect, respectively.

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