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

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. Aims. We appl...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2015-04, Vol.576, p.A134
Hauptverfasser:	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.
Format:	Artikel
Sprache:	eng
Schlagworte:	Amplification Astronomy Astrophysics Extrasolar planets Physics Planet detection Planetary atmospheres planetary systems planets and satellites: detection Spectral lines Spectroscopy techniques: radial velocities techniques: spectroscopic Wavelengths
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!