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
Magdis G
(2012)
THE MOLECULAR GAS CONTENT OF z = 3 LYMAN BREAK GALAXIES: EVIDENCE OF A NON-EVOLVING GAS FRACTION IN MAIN-SEQUENCE GALAXIES AT z > 2
in The Astrophysical Journal
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
Maguire K
(2011)
PTF10ops - a subluminous, normal-width light curve Type Ia supernova in the middle of nowhere PTF10ops: A subluminous, normal-width SN Ia
in Monthly Notices of the Royal Astronomical Society
Martig M
(2013)
The ATLAS3D project - XXII. Low-efficiency star formation in early-type galaxies: hydrodynamic models and observations
in Monthly Notices of the Royal Astronomical Society
McDermid R
(2007)
Connecting stars and ionised gas with integral-field spectroscopy
in New Astronomy Reviews
McDermid R
(2012)
The star-formation histories of early-type galaxies from ATLAS 3D
in Proceedings of the International Astronomical Union
Mould J
(2012)
INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES
in The Astrophysical Journal Supplement Series
Nobuta K
(2012)
BLACK HOLE MASS AND EDDINGTON RATIO DISTRIBUTION FUNCTIONS OF X-RAY-SELECTED BROAD-LINE AGNs AT z ~ 1.4 IN THE SUBARU XMM-NEWTON DEEP FIELD
in The Astrophysical Journal
Nugent P
(2011)
Supernova SN 2011fe from an exploding carbon-oxygen white dwarf star
in Nature
Peletier R
(2007)
The SAURON project - XI. Stellar populations from absorption-line strength maps of 24 early-type spirals
in Monthly Notices of the Royal Astronomical Society
Peletier R
(2012)
The SAURON project - XX. The Spitzer [3.6] - [4.5] colour in early-type galaxies: colours, colour gradients and inverted scaling relations The SAURON project - XX
in Monthly Notices of the Royal Astronomical Society
Perez M. S
(2009)
Inflow and outflow from the accretion disc of the microquasar SS 433: UKIRT spectroscopy
in Monthly Notices of the Royal Astronomical Society
Richards J
(2011)
BLAZARS IN THE FERMI ERA: THE OVRO 40 m TELESCOPE MONITORING PROGRAM
in The Astrophysical Journal Supplement Series
Riddick F
(2007)
An optical spectroscopic HR diagram for low-mass stars and brown dwarfs in Orion Low-mass stars and brown dwarfs in Orion
in Monthly Notices of the Royal Astronomical Society
RodrÃÂguez-López C
(2010)
The rapidly pulsating sdO star, SDSS J160043.6+074802.9
in Monthly Notices of the Royal Astronomical Society
Romani R
(2010)
THE BALMER-DOMINATED BOW SHOCK AND WIND NEBULA STRUCTURE OF ?-RAY PULSAR PSR J1741-2054
in The Astrophysical Journal
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
Sarzi M
(2010)
The SAURON project - XVI. On the sources of ionization for the gas in elliptical and lenticular galaxies
in Monthly Notices of the Royal Astronomical Society
Sarzi M
(2010)
The SAURON project - XVI. On the sources of ionization for the gas in elliptical and lenticular galaxies
in Monthly Notices of the Royal Astronomical Society
Sarzi M
(2013)
The ATLAS3D project - XIX. The hot gas content of early-type galaxies: fast versus slow rotators
in Monthly Notices of the Royal Astronomical Society
Sarzi M
(2011)
The planetary nebulae population in the central regions of M32: the SAURON view PNe in the central regions of M32
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
Schoenaers C
(2007)
A new slowly pulsating subdwarf-B star: HD 4539
in Communications in Asteroseismology
| 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 |