Using high-speed photometry techniques, three transits of the extrasolar planet across the disk of the star HD 209458 have been observed. The combination of a WET-style 3-channel photometer and an excellent site yielded millimagnitude photometric precision. The various techniques used to reduce the raw data obtained under different observing conditions are presented along with modelling of the transit light curves. Finally, a summary of what we have learned about this unique extrasolar planet is provided
Of the over 200 known extrasolar planets, 14 exhibit transits in front of their parent stars as seen...
Observations of stellar surfaces ndash; except for the Sun ndash; are hampered by their tiny angular...
We use multiband photometry to refine estimates for the planetary radius and orbital inclination of ...
We present the results of a program to develop techniques that enable high-resolution photometric me...
We report high-precision, high-cadence photometric measurements of the star HD 209458, which is know...
We present the results of a program to develop techniques that enable high-resolution photometric me...
This paper describes a photometry observation by an amateur astronomer of a transit of the extrasola...
We have observed four transits of the planet of HD 209458 using the STIS spectrograph on the Hubble ...
This dissertation describes an attempt to detect water in the atmosphere of the extrasolar planet HD...
Very precise photometry of transiting extrasolar planets can be used to learn about the physical str...
Extrasolar planet transit photometry is a relatively new astronomical technique developed over the p...
We report the detection of the primary transit of the extra-solar planet HD 80 606 b, thanks to pho...
International audienceWe report the detection of the primary transit of the extra-solar planet HD 80...
International audienceDuring its 39-month mission, Hipparcos observed the star HD 209458 on 89 occas...
Multicolor photometric observations of a planetary transit in the system HD 209458 are analyzed. The...
Of the over 200 known extrasolar planets, 14 exhibit transits in front of their parent stars as seen...
Observations of stellar surfaces ndash; except for the Sun ndash; are hampered by their tiny angular...
We use multiband photometry to refine estimates for the planetary radius and orbital inclination of ...
We present the results of a program to develop techniques that enable high-resolution photometric me...
We report high-precision, high-cadence photometric measurements of the star HD 209458, which is know...
We present the results of a program to develop techniques that enable high-resolution photometric me...
This paper describes a photometry observation by an amateur astronomer of a transit of the extrasola...
We have observed four transits of the planet of HD 209458 using the STIS spectrograph on the Hubble ...
This dissertation describes an attempt to detect water in the atmosphere of the extrasolar planet HD...
Very precise photometry of transiting extrasolar planets can be used to learn about the physical str...
Extrasolar planet transit photometry is a relatively new astronomical technique developed over the p...
We report the detection of the primary transit of the extra-solar planet HD 80 606 b, thanks to pho...
International audienceWe report the detection of the primary transit of the extra-solar planet HD 80...
International audienceDuring its 39-month mission, Hipparcos observed the star HD 209458 on 89 occas...
Multicolor photometric observations of a planetary transit in the system HD 209458 are analyzed. The...
Of the over 200 known extrasolar planets, 14 exhibit transits in front of their parent stars as seen...
Observations of stellar surfaces ndash; except for the Sun ndash; are hampered by their tiny angular...
We use multiband photometry to refine estimates for the planetary radius and orbital inclination of ...