Bibcode
Murgas, F.; Pallé, E.; Parviainen, H.; Chen, G.; Nortmann, L.; Nowak, G.; Cabrera-Lavers, A.; Iro, N.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 605, id.A114, 8 pp.
Fecha de publicación:
9
2017
Revista
Número de citas
15
Número de citas referidas
12
Descripción
Context. Transiting planets offer an excellent opportunity for
characterizing the atmospheres of extrasolar planets under very
different conditions from those found in our solar system. Aims:
We are currently carrying out a ground-based survey to obtain the
transmission spectra of several extrasolar planets using the 10 m Gran
Telescopio Canarias. In this paper we investigate the extrasolar planet
WASP-48b, a hot Jupiter orbiting around an F-type star with a period of
2.14 days. Methods: We obtained long-slit optical spectroscopy of
one transit of WASP-48b with the Optical System for Imaging and
low-Intermediate-Resolution Integrated Spectroscopy (OSIRIS)
spectrograph. We integrated the spectrum of WASP-48 and one reference
star in several channels with different wavelength ranges, creating
numerous color light curves of the transit. We fit analytic transit
curves to the data taking into account the systematic effects present in
the time series in an effort to measure the change of the planet-to-star
radius ratio (Rp/Rs) across wavelength. The change
in transit depth can be compared with atmosphere models to infer the
presence of particular atomic or molecular compounds in the atmosphere
of WASP-48b. Results: After removing the transit model and
systematic trends to the curves we reached precisions between 261 ppm
and 455-755 ppm for the white and spectroscopic light curves,
respectively. We obtained Rp/Rs uncertainty values
between 0.8 × 10-3 and 1.5 × 10-3 for
all the curves analyzed in this work. The measured transit depth for the
curves made by integrating the wavelength range between 530 nm and 905
nm is in agreement with previous studies. We report a relatively flat
transmission spectrum for WASP-48b with no statistical significant
detection of atmospheric species, although the theoretical models that
fit the data more closely include TiO and VO.
The transit light curves are only available at the CDS via anonymous ftp
to http://cdsarc.u-strasbg.fr
(http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/605/A114
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