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 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
{Schoenaers}, C. And {Lynas-Gray}, A.~E.
(2008)
Spectroscopic Mode Identification in Slowly-Pulsating Subdwarf B Stars
{Sale}, S.~E. And {Schoenaers}, C. And {Lynas-Gray}, A.~E.
(2008)
A New Determination of Abundances for the Subdwarf B Star HD 4539
{Lynas-Gray}, A.~E.
(2012)
Photometric Variability of HD 4539?
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
Yabe K
(2012)
NIR Spectroscopy of Star-Forming Galaxies at z ~ 1.4 with Subaru/FMOS: The Mass-Metallicity Relation
in Publications of the Astronomical Society of Japan
Yabe K
(2014)
The mass-metallicity relation at z ~ 1.4 revealed with Subaru/FMOS?
in Monthly Notices of the Royal Astronomical Society
Trinchieri G.
(2008)
DISCOVERY OF HOT GAS IN OUTFLOW IN NGC 3379
in ASTROPHYSICAL JOURNAL
Tonegawa M
(2015)
FIELD: Automated emission line detection software for Subaru/FMOS near-infrared spectroscopy
in Publications of the Astronomical Society of Japan
Tonegawa M
(2014)
A study of selection methods for Ha-emitting galaxies at z ~ 1.3 for the Subaru/FMOS galaxy redshift survey for cosmology (FastSound)
in Publications of the Astronomical Society of Japan
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. 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) Electronics 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 | 2009 |
Sector | Aerospace, Defence and Marine,Construction,Digital/Communication/Information Technologies (including Software),Education,Culture, Heritage, Museums and Collections,Other |
Impact Types | Cultural Societal |