WASP Bridge - 1st April 2011 to 31th March 2012
Lead Research Organisation:
Queen's University Belfast
Department Name: Sch of Mathematics and Physics
Abstract
Funding is to continue operational costs of the SuperWASP-N instrument. In particular this will support the International costs and actual running costs for the instrument. The data reduction costs (PDRA) will be provided by QUB.
Organisations
Publications
Graczyk D
(2015)
The Araucaria project. Precise physical parameters of the eclipsing binary IO Aquarii
in Astronomy & Astrophysics
Mo nik T
(2015)
The central star candidate of the planetary nebula Sh2-71: photometric and spectroscopic variability
in Monthly Notices of the Royal Astronomical Society
Díaz R
(2016)
The HARPS search for southern extra-solar planets XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles ???
in Astronomy & Astrophysics
Motalebi F
(2015)
The HARPS-N Rocky Planet Search I. HD 219134 b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun ?
in Astronomy & Astrophysics
Armstrong D
(2015)
The host stars of Kepler 's habitable exoplanets: superflares, rotation and activity
in Monthly Notices of the Royal Astronomical Society
Dressing C
(2015)
THE MASS OF Kepler-93b AND THE COMPOSITION OF TERRESTRIAL PLANETS
in The Astrophysical Journal
Anderson D
(2015)
THE WELL-ALIGNED ORBIT OF WASP-84b: EVIDENCE FOR DISK MIGRATION OF A HOT JUPITER
in The Astrophysical Journal
West R
(2016)
Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b?
in Astronomy & Astrophysics
Anderson D
(2014)
Three newly discovered sub-Jupiter-mass planets: WASP-69b and WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary?†
in Monthly Notices of the Royal Astronomical Society
Burton J
(2014)
TIDALLY DISTORTED EXOPLANETS: DENSITY CORRECTIONS FOR SHORT-PERIOD HOT-JUPITERS BASED SOLELY ON OBSERVABLE PARAMETERS
in The Astrophysical Journal