Ground-based Near-infrared Spectroscopy of HD 209458b with Palomar/TripleSpec

Details Ground-based Near-infrared Spectroscopy of HD 209458b with Palomar/TripleSpec Ground-based Near-infrared Spectroscopy of HD 209458b with Palomar/TripleSpec

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..290z&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.290

Physics

Scientific paper

We present J, H, and K-band infrared spectroscopy of the exoplanet HD 209458b using Palomar/TripleSpec. Preliminary reductions of secondary transit emission data indicate an upper limit on the planet-to-star emission ratio of 5×10-3±1.7×10-3. This initial result is consistent with previous Hubble/NICMOS observations by Swain et al. (2009) [5] and illustrates Palomar/ TripleSpec's potential for exoplanet spectroscopy.

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