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Fig. 3.
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Comparison of the spectra of the maser emission at 22 (black), 183 (blue), and 380 (magenta) GHz in TXS 2226, after smoothing the spectra to the coarsest spectral resolution of the 183 GHz data (Δv ∼ 1.6 km s−1). The dashed green line indicates the systemic velocity of the galaxy in the radio convention (7270 km s−1).
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