PATT Travel for Oxford University
Lead Research Organisation:
UNIVERSITY OF OXFORD
Department Name: Oxford Physics (Keble Road)
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
Falcón-Barroso J
(2011)
The SAURON project - XIX. Optical and near-infrared scaling relations of nearby elliptical, lenticular and Sa galaxies The SAURON project - XIX
in Monthly Notices of the Royal Astronomical Society
Bois M
(2011)
The ATLAS3D project - VI. Simulations of binary galaxy mergers and the link with fast rotators, slow rotators and kinematically distinct cores The ATLAS3D project - VI. Binary galaxy mergers
in Monthly Notices of the Royal Astronomical Society
Maguire K
(2012)
Hubble Space Telescope studies of low-redshift Type Ia supernovae: evolution with redshift and ultraviolet spectral trends NUV observations of SNe Ia
in Monthly Notices of the Royal Astronomical Society
Jeong H
(2012)
The SAURON project - XXI. The spatially resolved UV-line strength relations of early-type galaxies The SAURON project - XXI
in Monthly Notices of the Royal Astronomical Society
Serra P
(2012)
The ATLAS3D project - XIII. Mass and morphology of H i in early-type galaxies as a function of environment The ATLAS3D project - XIII. Neutral hydrogen
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
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
Davis TA
(2013)
A black-hole mass measurement from molecular gas kinematics in NGC4526.
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 |