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Discovery of Water at High Spectral Resolution in the Atmosphere of 51 Peg b

  • Authors: J. L. Birkby, R. J. de Kok, M. Brogi, H. Schwarz, and I. A. G. Snellen

2017 The Astronomical Journal 153 138.

  • Provider: AAS Journals

Caption: Figure 11.

Section of the summed and normalized CCF for 51 Peg b (solid black line), assuming ﹩{K}_{{\rm{P}}}=133﹩ km s−1. The dashed red line is the best-fitting Gaussian to the CCF centered at ﹩{V}_{\mathrm{sys}}=-33﹩ km s−1. The Gaussian has a ﹩\mathrm{FWHM}=5.6﹩ km s−1. The dotted blue line is the cross-correlation function of the best-matching template with itself after broadening the template to match a spectral resolution of R = 100,000.

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