Fig. 3
Section of the Ks spectrum of two stars that were observed using different instruments and/or different slit masks. Obj2 (top) was observed with MMIRS using the first (solid, black line) and the second (dashed, red line) slit mask. Obj5 (bottom) was observed with NTT/SofI (solid, black line) and Clay/MMIRS (red, dashed line). An arbitrary shift in flux was applied for better visual representation.
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