Spectral features of Earth-like planets and their detectability at different orbital distances around F, G, and K-type stars

Astronomy and Astrophysics

Volumn 553, Issue , 2013, Pages

  Hedelt, P ^a,b,c   Von Paris, P ^a,b,c   Godolt, M ^d   Gebauer, S ^d   Grenfell, J L ^d   Rauer, H ^a,d   Schreier, F ^a   Selsis, F ^b,c   Trautmann, T ^a  

^a GERMAN AEROSPACE CENTER DLR   (Germany)

^b UNIVERSITÉ DE BORDEAUX   (France)

^c CNRS   (France)

^d TECHNISCHE UNIVERSITÄT BERLIN   (Germany)

Author keywords

Planets and satellites: atmospheres; Planets and satellites: composition; Planets and satellites: detection; Radiative transfer; Techniques: imaging spectroscopy

Indexed keywords

EXTREMELY LARGE TELESCOPES; GROUND-BASED OBSERVATIONS; HIGH-RESOLUTION SPECTRA; JAMES WEBB SPACE TELESCOPE; PLANETS AND SATELLITES: ATMOSPHERES; PLANETS AND SATELLITES: COMPOSITIONS; PLANETS AND SATELLITES: DETECTIONS; TECHNIQUES: IMAGING SPECTROSCOPIES;

CARBON DIOXIDE; EXTRASOLAR PLANETS; INSTRUMENTS; INTERPLANETARY FLIGHT; METHANE; OPTICAL TELESCOPES; PHOTOMETRY; RADIATIVE TRANSFER; STARS;

SATELLITES;

EID: 84876571097     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117723     Document Type: Article

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