Project support for the Wide Area Search for Planets

Lead Research Organisation: University of St Andrews
Department Name: Physics and Astronomy

Abstract

Questions such as ``how many stars have planets around them?'' and ``how many habitable planets are there?'' interest both astronomers and everyone else. To answer them we need to find planets that can be studied in detail, seeking to understand the processes by which planets form and solar systems evolve. Of the two hundred planets that astronomers have found orbiting other stars we can learn most about those that transit in front of their star. We can measure how big they are, how heavy they are, and thus deduce their density and what they are made of. And by looking at how their atmosphere absorbs the light of their star we can discover the composition of their atmospheres. The WASP project aims to monitor 40 million of the brightest stars, looking for the tiny dips in their light caused by a planet passing in front of them. We will survey the sky for the transiting planets that are relatively close to Earth, which we can study in detail to enable us to understand how planetary systems form and evolve. The next generation of space missions, such as the James Webb Space Telescope, the successor to Hubble, will prioritize the study of planets around other stars. The WASP project will find the planets that will make the best and most interesting targets.

Publications

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Fares R (2013) A small survey of the magnetic fields of planet-host stars? in Monthly Notices of the Royal Astronomical Society

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Smith A (2009) A SuperWASP search for additional transiting planets in 24 known systems in Monthly Notices of the Royal Astronomical Society

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Galianni P (2013) A test of the failed disc wind scenario for the origin of the broad-line region in active galactic nuclei in Monthly Notices of the Royal Astronomical Society

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Brothwell R (2014) A window on exoplanet dynamical histories: Rossiter-McLaughlin observations of WASP-13b and WASP-32b in Monthly Notices of the Royal Astronomical Society

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Davies C (2014) Accretion discs as regulators of stellar angular momentum evolution in the ONC and Taurus-Auriga in Monthly Notices of the Royal Astronomical Society

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Clarke C (2008) Accretion-driven core collapse and the collisional formation of massive stars in Monthly Notices of the Royal Astronomical Society

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Doyle A (2013) Accurate spectroscopic parameters of WASP planet host stars? in Monthly Notices of the Royal Astronomical Society

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Greaves J (2013) Alignment in star-debris disc systems seen by Herschel in Monthly Notices of the Royal Astronomical Society: Letters

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Nisi RS (2014) An altitude and distance correction to the source fluence distribution of TGFs. in Journal of geophysical research. Space physics

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Brown D (2011) Are falling planets spinning up their host stars? Are falling planets spinning up their host stars? in Monthly Notices of the Royal Astronomical Society

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Bonomo A (2015) Characterization of small planets with Kepler and HARPS-N in EPJ Web of Conferences

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Vidotto A. A. (2015) Cool Stars and Space Weather in 18th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun

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Maxted P (2011) Discovery of a stripped red giant core in a bright eclipsing binary system? J0247-25 in Monthly Notices of the Royal Astronomical Society

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Gómez Maqueo Chew Y (2013) Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii in Astronomy & Astrophysics

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Brown D (2014) Discrepancies between isochrone fitting and gyrochronology for exoplanet host stars? in Monthly Notices of the Royal Astronomical Society

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Haywood R (2014) Disentangling planetary orbits from stellar activity in radial-velocity surveys in International Journal of Astrobiology

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Xiang Y (2014) Distribution and evolution of starspots on the RS CVn binary II Pegasi in 2004 in Monthly Notices of the Royal Astronomical Society

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Brown D (2011) Do falling planets cause stellar spin-up? in Proceedings of the International Astronomical Union

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Herrero E (2014) Doppler-beaming in the Kepler light curve of LHS 6343 A in Astronomy & Astrophysics

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Smalley B (2014) Eclipsing Am binary systems in the SuperWASP survey in Astronomy & Astrophysics

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Llama J (2013) Exoplanet transit variability: bow shocks and winds around HD 189733b in Monthly Notices of the Royal Astronomical Society

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Enoch B (2012) Factors affecting the radii of close-in transiting exoplanets in Astronomy & Astrophysics

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Baldry I (2014) Galaxy And Mass Assembly (GAMA): AUTOZ spectral redshift measurements, confidence and errors in Monthly Notices of the Royal Astronomical Society

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Kelvin L (2014) Galaxy And Mass Assembly (GAMA): stellar mass functions by Hubble type in Monthly Notices of the Royal Astronomical Society

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Pascucci I (2010) Gas Evolution in the Planet-Forming Region of Disks in Proceedings of the International Astronomical Union

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Bonnell I (2008) Gravitational fragmentation and the formation of brown dwarfs in stellar clusters Formation of brown dwarfs in Monthly Notices of the Royal Astronomical Society

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Anderson D (2010) H -band thermal emission from the 19-h period planet WASP-19b in Astronomy and Astrophysics

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Dumusque X (2015) HARPS-N OBSERVES THE SUN AS A STAR in The Astrophysical Journal

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Barnes J (2008) HD 179949b: a close orbiting extrasolar giant planet with a stratosphere? in Monthly Notices of the Royal Astronomical Society

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Holdsworth D (2014) High-frequency A-type pulsators discovered using SuperWASP?† in Monthly Notices of the Royal Astronomical Society

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Southworth J (2009) High-precision photometry by telescope defocusing - I. The transiting planetary system WASP-5 in Monthly Notices of the Royal Astronomical Society

 
Description SuperWASP is the UK's leading extra-solar planet detection program comprised of a consortium of eight academic institutions. SuperWASP consists of two robotic observatories that operate continuously throughout the year, allowing coverage of both hemispheres of the sky. The first, SuperWASP-North, is located on the island of La Palma among the Isaac Newton Group (ING) of telescopes. The second, SuperWASP-South, is located at the site of the South African Astronomical Observatory (SAAO), just outside Sutherland, South Africa. The observatories each consist of eight wide-angle cameras that simultaneously monitor the sky for planetary transit events. The eight cameras allow the monitoring of millions of stars simultaneously, enabling the detection of rare transit events. WASP has to date yielded over 150 discoveries of giant planets in close orbits about their host stars, making it the world's leading ground-based transit survey.
Exploitation Route Education; Data mining of public archive.
Sectors Aerospace, Defence and Marine,Digital/Communication/Information Technologies (including Software),Education

URL http://exoplanetarchive.ipac.caltech.edu/docs/SuperWASPMission.html
 
Description WASP planet discoveries formed the basis for a number of successful press releases.
First Year Of Impact 2008
Sector Education
Impact Types Cultural,Policy & public services

 
Description WASP 
Organisation Keele University
Country United Kingdom 
Sector Academic/University 
PI Contribution Design and implementation of WASP data-analysis pipeline. Design and implementation of WASP transit-search software. Design and implementation of WASP transit-fitting and orbit-determination software.
Collaborator Contribution QUB: Fabrication, installation and operation of SuperWASP. Keele: Fabrication, installation and operation of WASP-South. Leicester: Design, implementation and maintenance of WASP data archive.
Impact Over 200 Publications
 
Description WASP 
Organisation Open University
Department School of Physical Sciences
Country United Kingdom 
Sector Academic/University 
PI Contribution Design and implementation of WASP data-analysis pipeline. Design and implementation of WASP transit-search software. Design and implementation of WASP transit-fitting and orbit-determination software.
Collaborator Contribution QUB: Fabrication, installation and operation of SuperWASP. Keele: Fabrication, installation and operation of WASP-South. Leicester: Design, implementation and maintenance of WASP data archive.
Impact Over 200 Publications
 
Description WASP 
Organisation Queen's University Belfast
Department Sonic Arts Research Centre (SARC)
Country United Kingdom 
Sector Academic/University 
PI Contribution Design and implementation of WASP data-analysis pipeline. Design and implementation of WASP transit-search software. Design and implementation of WASP transit-fitting and orbit-determination software.
Collaborator Contribution QUB: Fabrication, installation and operation of SuperWASP. Keele: Fabrication, installation and operation of WASP-South. Leicester: Design, implementation and maintenance of WASP data archive.
Impact Over 200 Publications
 
Description WASP 
Organisation University of Leicester
Department Department of Physics & Astronomy
Country United Kingdom 
Sector Academic/University 
PI Contribution Design and implementation of WASP data-analysis pipeline. Design and implementation of WASP transit-search software. Design and implementation of WASP transit-fitting and orbit-determination software.
Collaborator Contribution QUB: Fabrication, installation and operation of SuperWASP. Keele: Fabrication, installation and operation of WASP-South. Leicester: Design, implementation and maintenance of WASP data archive.
Impact Over 200 Publications