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
Roseboom I
(2012)
FMOS near-IR spectroscopy of Herschel -selected galaxies: star formation rates, metallicity and dust attenuation at z ~ 1 Near-IR spectroscopy of Herschel galaxies
in Monthly Notices of the Royal Astronomical Society
Potter W
(2013)
Synchrotron and inverse-Compton emission from blazar jets - II. An accelerating jet model with a geometry set by observations of M87
in Monthly Notices of the Royal Astronomical Society
Shapiro K
(2010)
The SAURON project - XV. Modes of star formation in early-type galaxies and the evolution of the red sequence
in Monthly Notices of the Royal Astronomical Society
Scott N
(2012)
An Oxford SWIFT integral field spectroscopy study of 14 early-type galaxies in the Coma cluster
in Monthly Notices of the Royal Astronomical Society
Khochfar S
(2011)
The ATLAS3D project - VIII. Modelling the formation and evolution of fast and slow rotator early-type galaxies within ?CDM Fast and slow rotators
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
Potter W
(2013)
Synchrotron and inverse-Compton emission from blazar jets - III. Compton-dominant blazars
in Monthly Notices of the Royal Astronomical Society
Maguire K
(2014)
Exploring the spectral diversity of low-redshift Type Ia supernovae using the Palomar Transient Factory
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
Bureau M
(2011)
The SAURON project - XVIII. The integrated UV-line-strength relations of early-type galaxies
in Monthly Notices of the Royal Astronomical Society
| 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 |