Broad-band transmission spectrum and K-band thermal emission of WASP-43b as observed from the ground

Aims. WASP-43b is the closest-orbiting hot Jupiter, and it has high bulk density. It causes deep eclipse depths in the system's light curve in both transit and occultation that is attributed to the cool temperature and small radius of its host star. We aim to secure a broad-band transmission spectrum and to detect its near-infrared thermal emission in order to characterize its atmosphere.

• Publication year

  2014

• Venue

  Astronomy and Astrophysics

• Publication date

  2014-01-13

• Fields of study

  Physics, Environmental Science

• Identifiers
  DOI 10.1051/0004-6361/201322740arXiv 1401.3007
• External record

  Open on Semantic Scholar

• Source metadata

  Semantic Scholar

• No claims are published for this paper.

• No concepts are published for this paper.

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