Transit photometry is a powerful technique for studying exoplanets. Transit observations from the ground of targets of magnitude V= 10 or brighter, however, are limited by scintillation noise due to Earth's atmosphere. Through turbulence profiling using instruments such as the stereo-SCIDAR, we have shown to able to accurately model scintillation noise, which is essential in order to fully account for the error budget of the observation. Through numerical modelling we find that employing scintillation reducing techniques enables an improvement of a factor between 1.36 — 1.6 on the astrophysical parameters
Transiting exoplanets provide opportunities for us to observe their atmospheres and to analyse them ...
The technique of transit spectroscopy has given us our first insights into the atmospheric features ...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...
Atmospheric scintillation caused by optical turbulence in the Earth’s atmosphere can be the dominant...
In this thesis, the effect of scintillation arising from atmospheric optical turbulence on exoplanet...
Scintillation noise due to the Earth's turbulent atmosphere can be a dominant noise source in high-p...
Scintillation noise due to the Earth's turbulent atmosphere can be a dominant noise source in high-p...
Ground-based photometry of bright stars is expected to be limited by atmospheric scintillation, alth...
Ground-based photometry of bright stars is expected to be limited by atmospheric scintillation, alth...
We describe a new concept to correct for scintillation noise on high-precision photometry in large a...
Stereo-SCIDAR (SCIntillation Detection and Ranging) is a development to the well known SCIDAR method...
High-precision fast photometry from ground-based observatories is a challenge due to intensity fluct...
© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Socie...
Aims. Scintillation noise is a major limitation of ground-based photometric precision. Methods. A...
A new generation of exoplanet research beckons and with it the need for simulation tools that accura...
Transiting exoplanets provide opportunities for us to observe their atmospheres and to analyse them ...
The technique of transit spectroscopy has given us our first insights into the atmospheric features ...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...
Atmospheric scintillation caused by optical turbulence in the Earth’s atmosphere can be the dominant...
In this thesis, the effect of scintillation arising from atmospheric optical turbulence on exoplanet...
Scintillation noise due to the Earth's turbulent atmosphere can be a dominant noise source in high-p...
Scintillation noise due to the Earth's turbulent atmosphere can be a dominant noise source in high-p...
Ground-based photometry of bright stars is expected to be limited by atmospheric scintillation, alth...
Ground-based photometry of bright stars is expected to be limited by atmospheric scintillation, alth...
We describe a new concept to correct for scintillation noise on high-precision photometry in large a...
Stereo-SCIDAR (SCIntillation Detection and Ranging) is a development to the well known SCIDAR method...
High-precision fast photometry from ground-based observatories is a challenge due to intensity fluct...
© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Socie...
Aims. Scintillation noise is a major limitation of ground-based photometric precision. Methods. A...
A new generation of exoplanet research beckons and with it the need for simulation tools that accura...
Transiting exoplanets provide opportunities for us to observe their atmospheres and to analyse them ...
The technique of transit spectroscopy has given us our first insights into the atmospheric features ...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...