Fig. 8.
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Differences between elemental species (on the x-axis) derived in this work from near-infrared IGRINS spectra (black dots) and those published by T24 using optical high-resolution spectra obtained with ESPaDOnS at the CFHT (red dots). On the y-axis, the difference is expressed in the [X/H] form. Each panel corresponds to a star in common in the two samples.
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