IoA PATT grant 2009-11
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
This proposal requests funds to cover travel and subsistence expenses associated with observing time on international telescopes allocated by the PATT Committee during the two academic years 2009-10 and 2010-11. The aquisition of observational data form these facilities represents one of the key inputs responsible for the scientific productivity of the Institute of Astronomy. The scientific goals of the programme fall under the following main headings: (a) Quasars, AGN and quasar absorption lines; (b) X-ray astronomy; (c) Stellar astronomy; (d) The galaxy and the local universe; (e) Dark matter and galaxy clustering; (f) The high-redshift universe.
Organisations
People |
ORCID iD |
| Paul Hewett (Principal Investigator) |
Publications
Niederste-Ostholt M
(2010)
Alignment of brightest cluster galaxies with their host clusters
in Monthly Notices of the Royal Astronomical Society
Smart R
(2010)
The distance to the cool T9 brown dwarf ULAS J003402.77-005206.7
in Astronomy and Astrophysics
Erb D
(2010)
PHYSICAL CONDITIONS IN A YOUNG, UNREDDENED, LOW-METALLICITY GALAXY AT HIGH REDSHIFT
in The Astrophysical Journal
Wei L
(2010)
THE RELATIONSHIP BETWEEN MOLECULAR GAS AND STAR FORMATION IN LOW-MASS E/S0 GALAXIES
in The Astrophysical Journal
Tafelmeyer M
(2010)
Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans
in Astronomy & Astrophysics
Cooke R
(2010)
A newly discovered DLA and associated Lya emission in the spectra of the gravitationally lensed quasar UM 673A,B? A DLA and associated Lya emission in UM 673A,B
in Monthly Notices of the Royal Astronomical Society
Eales S
(2010)
The Herschel ATLAS
in Publications of the Astronomical Society of the Pacific
Pontzen A
(2010)
The nature of H i absorbers in gamma-ray burst afterglows: clues from hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Boquien M
(2010)
100 µ m and 160 µ m emission as resolved star-formation rate estimators in M 33 (HERM33ES)
in Astronomy and Astrophysics
Leitherer C
(2010)
A LIBRARY OF THEORETICAL ULTRAVIOLET SPECTRA OF MASSIVE, HOT STARS FOR EVOLUTIONARY SYNTHESIS
in The Astrophysical Journal Supplement Series