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.

Publications

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{Sale}, S.~E. And {Schoenaers}, C. And {Lynas-Gray}, A.~E. (2008) A New Determination of Abundances for the Subdwarf B Star HD 4539

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Schoenaers C (2007) A new slowly pulsating subdwarf-B star: HD 4539 in Communications in Asteroseismology

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Ganda K (2007) Absorption-line strengths of 18 late-type spiral galaxies observed with SAURON in Monthly Notices of the Royal Astronomical Society

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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

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Richards J (2011) BLAZARS IN THE FERMI ERA: THE OVRO 40 m TELESCOPE MONITORING PROGRAM in The Astrophysical Journal Supplement Series

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Healey S (2008) CGRaBS: An All-Sky Survey of Gamma-Ray Blazar Candidates in The Astrophysical Journal Supplement Series

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McDermid R (2007) Connecting stars and ionised gas with integral-field spectroscopy in New Astronomy Reviews

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Brassington N. J. (2008) DEEP CHANDRA MONITORING OBSERVATIONS OF NGC 3379: CATALOG OF SOURCE PROPERTIES in ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

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Brassington N (2009) DEEP CHANDRA MONITORING OBSERVATIONS OF NGC 4278: CATALOG OF SOURCE PROPERTIES in The Astrophysical Journal Supplement Series

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Krajnovi?? D (2009) Determination of masses of the central black holes in NGC 524 and 2549 using laser guide star adaptive optics in Monthly Notices of the Royal Astronomical Society

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Trinchieri G. (2008) DISCOVERY OF HOT GAS IN OUTFLOW IN NGC 3379 in ASTROPHYSICAL JOURNAL

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Fabbiano G (2010) FIELD AND GLOBULAR CLUSTER LOW-MASS X-RAY BINARIES IN NGC 4278 in The Astrophysical Journal

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Bois M (2010) Formation of slowly rotating early-type galaxies via major mergers: a resolution study in Monthly Notices of the Royal Astronomical Society

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Keel W (2013) Galaxy Zoo: A Catalog of Overlapping Galaxy Pairs for Dust Studies in Publications of the Astronomical Society of the Pacific

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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

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Mould J (2012) INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES in The Astrophysical Journal Supplement Series

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Duc P (2011) Investigating the Merger Origin of Early-type Galaxies using Ultra-deep Optical Images in Proceedings of the International Astronomical Union

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Cappellari, M (2010) Measuring the Low Mass End of the M center dot - sigma Relation in HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION

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Krajnovic, D And McDermid, RM And Cappellari, M And Davies, RL (2010) Measuring the Low Mass End of the M center dot - sigma Relation

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Bureau M (2011) Molecular Gas and Star Formation in Local Early-type Galaxies in Proceedings of the International Astronomical Union

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Davies R (2011) New views of old galaxies in Astronomy & Geophysics

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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

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Caruana J (2013) No evidence for Lyman   emission in spectroscopy of z > 7 candidate galaxies in Monthly Notices of the Royal Astronomical Society

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Shaw M (2009) OPTICAL SPECTROSCOPY OF BRIGHT FERMI LAT BLAZARS in The Astrophysical Journal

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{Lynas-Gray}, A.~E. (2012) Photometric Variability of HD 4539?

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Cappellari M (2010) Scaling relations in early-type galaxies from integral-field stellar kinematics in Proceedings of the International Astronomical Union

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Van Breukelen C (2007) Spectroscopic follow-up of a cluster candidate at z= 1.45 Spectroscopic follow-up of a cluster at z=1.45 in Monthly Notices of the Royal Astronomical Society

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{Schoenaers}, C. And {Lynas-Gray}, A.~E. (2008) Spectroscopic Mode Identification in Slowly-Pulsating Subdwarf B Stars

 
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