PATT Travel for Oxford University
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
The application seeks funds to cover the cost of travel and subsistence from 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 further explore the Universe.
Organisations
Publications
Davis T
(2011)
The ATLAS3D project - V. The CO Tully-Fisher relation of early-type galaxies The CO-TFR of early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Bois M
(2010)
Formation of slowly rotating early-type galaxies via major mergers: a resolution study
in Monthly Notices of the Royal Astronomical Society
Kuntschner H
(2010)
The SAURON project - XVII. Stellar population analysis of the absorption line strength maps of 48 early-type galaxies
in Monthly Notices of the Royal Astronomical Society
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
Cappellari M
(2011)
The ATLAS3D project - VII. A new look at the morphology of nearby galaxies: the kinematic morphology-density relation The ATLAS3D project - VII. Morphology-density
in Monthly Notices of the Royal Astronomical Society
Cappellari M
(2011)
The ATLAS3D project - I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria The ATLAS3D project - I. The sample
in Monthly Notices of the Royal Astronomical Society
Young L
(2011)
The ATLAS3D project - IV. The molecular gas content of early-type galaxies? Molecular gas content of early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Nugent P
(2011)
Supernova SN 2011fe from an exploding carbon-oxygen white dwarf star
in Nature
Cappellari M
(2012)
Systematic variation of the stellar initial mass function in early-type galaxies
in Nature
Hallinan G
(2015)
Magnetospherically driven optical and radio aurorae at the end of the stellar main sequence.
in Nature
| Description | The grant has enabled 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. |
| Sectors | Aerospace Defence and Marine Construction Digital/Communication/Information Technologies (including Software) Education Culture Heritage Museums and Collections |
| Description | The findings have been published in scientific journals. hey 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 | 2011 |
| Sector | Aerospace, Defence and Marine,Construction,Education,Culture, Heritage, Museums and Collections,Other |
| Impact Types | Cultural Societal |
