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
RodrÃguez-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
(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
(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
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
Scott N
(2009)
The SAURON Project - XIV. No escape from V esc : a global and local parameter in early-type galaxy evolution
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
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
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
Shaw M
(2012)
SPECTROSCOPY OF BROAD-LINE BLAZARS FROM 1LAC
in The Astrophysical Journal
Shaw M
(2009)
OPTICAL SPECTROSCOPY OF BRIGHT FERMI LAT BLAZARS
in The Astrophysical Journal
Shaw M
(2013)
SPECTROSCOPY OF THE LARGEST EVER ?-RAY-SELECTED BL LAC SAMPLE
in The Astrophysical Journal
Silverman J
(2013)
LATE-TIME SPECTRAL OBSERVATIONS OF THE STRONGLY INTERACTING TYPE Ia SUPERNOVA PTF11kx
in The Astrophysical Journal
Sobral D
(2011)
The dependence of star formation activity on environment and stellar mass at z~ 1 from the HiZELS-Ha survey? Star formation, environment & mass at z~1
in Monthly Notices of the Royal Astronomical Society
Sobral D
(2010)
The clustering and evolution of Ha emitters at z ~ 1 from HiZELS
in Monthly Notices of the Royal Astronomical Society
Taylor G
(2007)
Characteristics of EGRET Blazars in the VLBA Imaging and Polarimetry Survey (VIPS)
in The Astrophysical Journal
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
Tonegawa M
(2015)
FIELD: Automated emission line detection software for Subaru/FMOS near-infrared spectroscopy
in Publications of the Astronomical Society of Japan
Trinchieri G.
(2008)
DISCOVERY OF HOT GAS IN OUTFLOW IN NGC 3379
in ASTROPHYSICAL JOURNAL
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
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 |