Project support for WASP (Keele), supplement.
Lead Research Organisation:
Keele University
Department Name: Institute Env Physical Sci & App Maths
Abstract
The WASP project is current the world's most successful search for transiting exoplanets. This bridging application requests funds to continue operating the WASP-South facility and thus continue discovering new transiting extrasolar planets.
Organisations
People |
ORCID iD |
Coel Hellier (Principal Investigator) |
Publications
Southworth J
(2012)
Physical properties and radius variations in the HAT-P-5 planetary system from simultaneous four-colour photometry The physical properties of HAT-P-5
in Monthly Notices of the Royal Astronomical Society
Southworth J
(2010)
ERRATUM: "PHYSICAL PROPERTIES OF THE 0.94 DAY PERIOD TRANSITING PLANETARY SYSTEM WASP-18" (2009, ApJ, 707, 167)
in The Astrophysical Journal
Southworth J
(2011)
Homogeneous studies of transiting extrasolar planets - IV. Thirty systems with space-based light curves Studies of transiting extrasolar planets - IV
in Monthly Notices of the Royal Astronomical Society
Smolders K
(2012)
The Spitzer spectroscopic survey of S-type stars
in Astronomy & Astrophysics
Smith R
(2012)
Dust discs around intermediate-mass and Sun-like stars in the 16 Myr old NGC 1960 open cluster Debris discs in NGC 1960
in Monthly Notices of the Royal Astronomical Society
Smith R
(2011)
Debris discs in the 27 Myr old open cluster IC 4665 Debris discs in IC4665
in Monthly Notices of the Royal Astronomical Society
Smith D
(2011)
Herschel-ATLAS: counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue? Herschel-ATLAS: counterparts
in Monthly Notices of the Royal Astronomical Society
Smith A
(2011)
Thermal emission from WASP-33b, the hottest known planet? Thermal emission from WASP-33b
in Monthly Notices of the Royal Astronomical Society
Smith A
(2012)
WASP-36b: A NEW TRANSITING PLANET AROUND A METAL-POOR G-DWARF, AND AN INVESTIGATION INTO ANALYSES BASED ON A SINGLE TRANSIT LIGHT CURVE
in The Astronomical Journal
Smith A
(2013)
WASP-71b: a bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star
in Astronomy & Astrophysics
Description | Lots and lots of them |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Media (as a channel to the public) |
Results and Impact | We have particpated in dozens and dozens of such activites. Lots. We have about dozens and dozens of such feedbacks. |
Year(s) Of Engagement Activity | Pre-2006,2006,2007,2008,2009,2010,2011,2012,2013,2014 |