The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing DOI : 10.1111/j.1365-2966.2005.09905.xPeer reviewe
We have measured the transmission spectrum of the extremely inflated hot Jupiter WASP-52b using simu...
We have used spectrophotometric data from the Hubble Space Telescope (HST) to eclipse-map the primar...
Measuring stellar parallax, position and proper motion is the task of astrometry. With the developme...
We have used maximum entropy eclipse-mapping to recover images of the visual surface brightness dist...
The aim of this work has been to increase our understanding of the surface brightness distributions ...
The variation of the specific intensity across the stellar disc is an essential input parameter in s...
We have used spectrophotometric data from nine Hubble Space Telescope orbits to eclipse-map the prim...
We have used contemporaneous spectra and V light curves to form spot models for RS CVn in 1991 and 1...
Using a time series of high-resolution spectra and high-quality multicolour photometry, we reconstru...
Starspots are an important manifestation of stellar activity and yet their distribution patterns on ...
A general introduction to the foundations of spot modelling is given. It considers geometric models ...
We have used spectrophotometric data from the Hubble Space Telescope to eclipse-map the primary comp...
Extremely large telescopes (ELTs) provide an opportunity to observe surface inhomogeneities for ultr...
Original article can be found at : http://www.aanda.org/ Copyright The European Southern Observatory...
Nearby active stars with relatively rapid rotation and large starspot structures offer the opportuni...
We have measured the transmission spectrum of the extremely inflated hot Jupiter WASP-52b using simu...
We have used spectrophotometric data from the Hubble Space Telescope (HST) to eclipse-map the primar...
Measuring stellar parallax, position and proper motion is the task of astrometry. With the developme...
We have used maximum entropy eclipse-mapping to recover images of the visual surface brightness dist...
The aim of this work has been to increase our understanding of the surface brightness distributions ...
The variation of the specific intensity across the stellar disc is an essential input parameter in s...
We have used spectrophotometric data from nine Hubble Space Telescope orbits to eclipse-map the prim...
We have used contemporaneous spectra and V light curves to form spot models for RS CVn in 1991 and 1...
Using a time series of high-resolution spectra and high-quality multicolour photometry, we reconstru...
Starspots are an important manifestation of stellar activity and yet their distribution patterns on ...
A general introduction to the foundations of spot modelling is given. It considers geometric models ...
We have used spectrophotometric data from the Hubble Space Telescope to eclipse-map the primary comp...
Extremely large telescopes (ELTs) provide an opportunity to observe surface inhomogeneities for ultr...
Original article can be found at : http://www.aanda.org/ Copyright The European Southern Observatory...
Nearby active stars with relatively rapid rotation and large starspot structures offer the opportuni...
We have measured the transmission spectrum of the extremely inflated hot Jupiter WASP-52b using simu...
We have used spectrophotometric data from the Hubble Space Telescope (HST) to eclipse-map the primar...
Measuring stellar parallax, position and proper motion is the task of astrometry. With the developme...
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