An HST Optical to Near-IR Transmission Spectrum of the Hot Jupiter WASP-19b: Detection of Atmospheric Water and Likely Absence of TiO

We measure the transmission spectrum of WASP-19b from 3 transits using low-resolution optical spectroscopy from the HST Space Telescope Imaging Spectrograph (STIS). The STIS spectra cover a wavelength range of 0.29-1.03 microns with resolving power R=500. The optical data are combined with archival...

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Bibliográfalaš dieđut
Váldodahkkit:	Huitson, C, Sing, D, Pont, F, Fortney, J, Burrows, A, Wilson, P, Ballester, G, Nikolov, N, Gibson, N, Deming, D, Aigrain, S, Evans, T, Henry, G, Etangs, A, Showman, A, Vidal-Madjar, A, Zahnle, K
Materiálatiipa:	Journal article
Giella:	English
Almmustuhtton:	2013

An HST Optical to Near-IR Transmission Spectrum of the Hot Jupiter WASP-19b: Detection of Atmospheric Water and Likely Absence of TiO

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