Evidence for a spectroscopic direct detection of reflected light from 51 Pegasi b

J. H. C. Martins; N. C. Santos; P. Figueira; J. P. Faria; M. Montalto; I. Boisse; D. Ehrenreich; C. Lovis; M. Mayor; C. Melo; F. Pepe; S. G. Sousa; S. Udry; D. Cunha

doi:10.1051/0004-6361/201425298

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Volume 576 (April 2015)

A&A, 576 (2015) A134

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Fig. 2

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Detection significance as a function of k_Planet. The red line corresponds to the k_Planet value for maximum detection. The maximum detection occurs for similar k_Planet values for both templates. The amplitude values set to zero corresponds to k_Planet values for which no Gaussian fit with our restrictions could be achieved. Left panel: using template #1; right panel: using template #2.

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