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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(375), p. 307-312

DOI: 10.1111/j.1365-2966.2006.11302.x

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K-band transit and secondary eclipse photometry of exoplanet OGLE-TR-113b

Journal article published in 2006 by I. A. G. Snellen, E. Covino ORCID
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

Abstract

We present high precision K-band photometry of the transit and secondary eclipse of extrasolar planet OGLE-TR-113, using the SOFI near-infrared instrument on ESO's NTT. Data were taken in 5 second exposures over two periods of 3-4 hours, using random jitter position offsets. In this way, a relative photometric precision of ~1% per frame was achieved, avoiding systematic effects that seem to become dominant at precisions exceeding this level, and resulting in an overall accuracy of 0.1% per ~10 minutes. The observations of the transit show a flat bottom light-curve indicative of a significantly lower stellar limb-darkening at near-infrared than at optical wavelengths. The observations of the secondary eclipse result in a 3 sigma detection of emission from the exoplanet at 0.17+-0.05%. However, residual systematic errors make this detection rather tentative. ; Comment: 6 pages, 7 figures: MNRAS accepted