PATT Travel for Oxford University
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
This application seeks funds to cover the cost of travel and subsistence for astronomers from Oxford University to work at and acquire data from telescopes around the world in order to make observations of stars, galaxies and quasars and futher explore the Universe.
Organisations
Publications
Caruana J
(2013)
No evidence for Lyman emission in spectroscopy of z > 7 candidate galaxies
in Monthly Notices of the Royal Astronomical Society
Sarzi M
(2007)
On the origin and fate of ionised-gas in early-type galaxies: The SAURON perspective
in New Astronomy Reviews
Shaw M
(2009)
OPTICAL SPECTROSCOPY OF BRIGHT FERMI LAT BLAZARS
in The Astrophysical Journal
Kassin S
(2011)
Oxford SWIFT integral field spectrograph and multiwavelength observations of the Eagle galaxy at z= 0.77 The Eagle galaxy at z = 0.77
in Monthly Notices of the Royal Astronomical Society
{Lynas-Gray}, A.~E.
(2012)
Photometric Variability of HD 4539?
Cenko S
(2012)
PTF10iya: a short-lived, luminous flare from the nuclear region of a star-forming galaxy PTF10iya: a short-lived, luminous flare
in Monthly Notices of the Royal Astronomical Society
Cappellari M
(2010)
Scaling relations in early-type galaxies from integral-field stellar kinematics
in Proceedings of the International Astronomical Union
Van Breukelen C
(2007)
Spectroscopic follow-up of a cluster candidate at z= 1.45 Spectroscopic follow-up of a cluster at z=1.45
in Monthly Notices of the Royal Astronomical Society
{Schoenaers}, C. And {Lynas-Gray}, A.~E.
(2008)
Spectroscopic Mode Identification in Slowly-Pulsating Subdwarf B Stars
Description | The grant has enabled Oxford staff members to travel to telescopes around the World, in order to make discoveries about the Universe through observations of stars, galaxies, supernovae and planets. The findings have been published in peer-reviewed journals. |
Exploitation Route | Scientists make use of the findings by devising new theories of the universe that match the observations, and by devsing new observations to further test those theories. The observations are also used in public talks and events. The results are also used to inform the design of future ground-based and space-based telescopes. |
Sectors | Aerospace, Defence and Marine,Construction,Digital/Communication/Information Technologies (including Software),Education,Culture, Heritage, Museums and Collections,Other |
Description | The findings have been published in scientific journals. They have also been used for education purposes and for public outreach events. These activities lead to an increased awareness of astronomy in the general public and potential increase in young people taking up physics at school and university level. |
First Year Of Impact | 2007 |
Sector | Aerospace, Defence and Marine,Construction,Digital/Communication/Information Technologies (including Software),Education,Other |
Impact Types | Cultural,Societal |