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Fig. 1


GMOS (top) and MOSFIRE (bottom) spectra of exoplanet host star GJ 3470 (black) and simultaneously-observed comparison star TYC 1363-2087-1 (gray). The former is a main-sequence M dwarf, while the latter is a rather hotter giant. The short black bars in the top panel indicate the locations of the gaps between the GMOS CCDs.

This figure is made of several images, please see below:

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