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Fig. A.2
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6.7 GHz maser velocity-integrated flux density (grey labels and circles) of G26 superimposed with the 3.4 μm (W1) and 4.6 μm (W2) NEOWISE light curves. The average magnitudes are shown for 21 NEOWISE epochs, and the bars denote the standard deviation. The dark grey line shows the average maser light curves.
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