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

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

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

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

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Context. The detection of reflected light from an exoplanet is a difficult technical challenge at optical wavelengths. Even though this signal is expected to replicate the stellar signal, not only is it several orders of magnitude fainter, but it is also hidden among the stellar noise.

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《Astronomy and astrophysics》 |2015年第1期|共9页
作者
Martins J. H. C.; Santos N. C.; Figueira P.Faria J. P.Montalto M.Boisse I.Ehrenreich D.Lovis C.Mayor M.Melo C.Pepe F.Sousa S. G.Udry S.Cunha D.;
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作者单位

Univ Porto, CAUP, Inst Astrofis & Ciencias Espaco, P-4150762 Oporto, Portugal;

Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France;

Univ Geneva, Observ Geneve, CH-1290 Sauverny, SwitzerlandEuropean So Observ, Santiago 19, Chile;

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原文格式 PDF
正文语种英语
中图分类天文学;
关键词
planetary systems; planets and satellites: detection; techniques: spectroscopic; techniques: radial velocities;

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

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