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Techniques: Spectroscopic
The GTC exoplanet transit spectroscopy survey. VIII. Flat transmission spectrum for the warm gas giant WASP-80b
Aims: We set out to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium temperature of 800 K, using …
H. Parviainen
,
E. Pallé
,
G. Chen
,
L. Nortmann
,
F. Murgas
,
G. Nowak
,
S. Aigrain
,
A. Booth
,
M. Abazorius
,
N. Iro
Posted Jan 1, 2018
Cite
DOI
arXiv
The GTC exoplanet transit spectroscopy survey. IV. Confirmation of the flat transmission spectrum of HAT-P-32b
We observed the hot Jupiter
HAT-P-32b
(also known as HAT-P-32Ab) to determine its optical transmission spectrum by measuring the …
L. Nortmann
,
E. Pallé
,
F. Murgas
,
S. Dreizler
,
N. Iro
,
A. Cabrera-Lavers
Posted Oct 1, 2016
Cite
DOI
arXiv
The GTC exoplanet transit spectroscopy survey. III. No asymmetries in the transit of CoRoT-29b
Context. The launch of the exoplanet space missions obtaining exquisite photometry from space has resulted in the discovery of …
E. Pallé
,
G. Chen
,
R. Alonso
,
G. Nowak
,
H. Deeg
,
J. Cabrera
,
F. Murgas
,
H. Parviainen
,
L. Nortmann
,
S. Hoyer
,
J. Prieto-Arranz
,
D. Nespral
,
A. Cabrera-Lavers
,
N. Iro
Posted May 1, 2016
Cite
DOI
arXiv
The GTC exoplanet transit spectroscopy survey. II. An overly large Rayleigh-like feature for exoplanet TrES-3b
Aims: We search for Rayleigh scattering and K and Na absorption signatures from the atmosphere of TrES-3b using ground-based …
H. Parviainen
,
E. Pallé
,
L. Nortmann
,
G. Nowak
,
N. Iro
,
F. Murgas
,
S. Aigrain
Posted Jan 1, 2016
Cite
DOI
arXiv
Further Constraints on the Optical Transmission Spectrum of HAT-P-1b
We report on novel observations of HAT-P-1 aimed at constraining the optical transmission spectrum of the atmosphere of its transiting …
M. Montalto
,
N. Iro
,
N.~C. Santos
,
S. Desidera
,
J.~H.~C. Martins
,
P. Figueira
,
R. Alonso
Posted Sep 1, 2015
Cite
DOI
arXiv
Transmission spectroscopy of the sodium 'D' doublet in WASP-17b with the VLT
The detection of increased sodium absorption during primary transit implies the presence of an atmosphere around an extrasolar planet, …
P.~L. Wood
,
P.~F.~L. Maxted
,
B. Smalley
,
N. Iro
Posted Apr 1, 2011
Cite
DOI
arXiv