most citedDetection of titanium oxide in the atmosphere of a hot Jupiter

194 citations · 256 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM20171 cited

Estimation of Exoplanetary Planet-to-Star Radius Ratio with Homomorphic Processing

Rodrigo Mahu, Patricio Rojo, Ali Dehghan Firoozabadi +3

In this paper a homomorphic filtering scheme is proposed to improve the estimation of the planet/star radius ratio in astronomical transit signals. The idea is to reduce the effect…

astro-ph.EP2017194 cited

Detection of titanium oxide in the atmosphere of a hot Jupiter

Elyar Sedaghati, Henri M. J. Boffin, Ryan J. MacDonald +6

As an exoplanet transits its host star, some of the light from the star is absorbed by the atoms and molecules in the planet's atmosphere, causing the planet to seem bigger; plotti…

astro-ph.IM20172 cited

Unsupervised Method for Correlated Noise Removal for Multi-wavelength Exoplanet Transit Observations

Ali Dehghan Firoozabadi, Alejandro Diaz, Patricio Rojo +4

Exoplanetary atmospheric observations require an exquisite precision in the measurement of the relative flux among wavelengths. In this paper, we aim to provide a new adaptive meth…

astro-ph.EP201724 cited

Probing the atmosphere of a sub-Jovian planet orbiting a cool dwarf

Elyar Sedaghati, Henri. M. J. Boffin, Laetitia Delrez +4

We derive the 0.01 m binned transmission spectrum, between 0.74 and 1.0 m, of WASP-80b from low resolution spectra obtained with the FORS2 instrument attached to ESO's Very L…

astro-ph.EP201533 cited

Regaining the FORS: optical ground-based transmission spectroscopy of the exoplanet WASP-19b with VLT+FORS2

E. Sedaghati, H. M. J. Boffin, Sz. Csizmadia +4

In the past few years, the study of exoplanets has evolved from being pure discovery, then being more exploratory in nature and finally becoming very quantitative. In particular, t…

astro-ph.SR20152 cited

Making FORS2 fit for exoplanet observations (again)

H. M. J. Boffin, G. Blanchard, O. A. Gonzalez +10

For about three years, it was known that precision spectrophotometry with FORS2 suffered from systematic errors that made quantitative observations of planetary transits impossible…