Figure 3 from Discovery of Water at High Spectral Resolution in the Atmosphere of 51 Peg b

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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 3.

Detection strength (T, as described in Section 3.3) of an injected fake planet at the proposed planet velocity parameters from Brogi et al. (2013) for each CRIRES detector after each iteration of SYSREM. The horizontal dotted lines mark the maximum detection strength per detector for the injected model.

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