Exoplanet atmospheres at high spectral resolution: A CRIRES survey of hot-Jupiters

Ignas Snellen, Remco De Kok, Ernst De Mooij, Matteo Brogi, Bas Nefs, Simon Albrecht

Research output: Chapter in Book/Report/Conference proceedingConference paperAcademicpeer-review

4 Citations (Scopus)

Abstract

Recently, we presented the detection of carbon monoxide in the transmission spectrum of extrasolar planet HD209458b, using CRIRES, the Cryogenic high-resolution Infrared Echelle Spectrograph at ESO's Very Large Telescope (VLT). The high spectral resolution observations (R=100,000) provide a wealth of information on the planet's orbit, mass, composition, and even on its atmospheric dynamics. The new observational strategy and data analysis techniques open up a whole world of opportunities. We therefore started an ESO large program using CRIRES to explore these, targeting both transiting and non-transiting planets in carbon monoxide, water vapour, and methane. Observations of the latter molecule will also serve as a test-bed for METIS, the proposed mid-infrared imager and spectrograph for the European Extremely Large Telescope.

Original languageEnglish
Title of host publicationThe Astrophysics of Planetary Systems
Subtitle of host publicationFormation, Structure, and Dynamical Evolution
EditorsAlessandro Sozzetti, Mario Lattanzi, Alan Boss
Pages208-211
Number of pages4
EditionS276
DOIs
Publication statusPublished - Oct 2010
Externally publishedYes

Publication series

NameProceedings of the International Astronomical Union
NumberS276
Volume6
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Planetary systems
  • Techniques: spectroscopic

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