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
Verley S
(2010)
Properties of compact 250 µ m emission and H II regions in M 33 (HERM33ES)
in Astronomy and Astrophysics
Niederste-Ostholt M
(2010)
RE-ASSEMBLING THE SAGITTARIUS DWARF GALAXY
in The Astrophysical Journal
Scott K
(2011)
REDSHIFT DETERMINATION AND CO LINE EXCITATION MODELING FOR THE MULTIPLY LENSED GALAXY HLSW-01
in The Astrophysical Journal
Jones T
(2010)
Resolved spectroscopy of gravitationally lensed galaxies: recovering coherent velocity fields in subluminous z ~ 2-3 galaxies
in Monthly Notices of the Royal Astronomical Society
Barker M
(2009)
RESOLVING THE STELLAR OUTSKIRTS OF M81: EVIDENCE FOR A FAINT, EXTENDED STRUCTURAL COMPONENT
in The Astronomical Journal
Scholz A
(2011)
Rotation periods for very low mass stars in Praesepe Rotation periods in Praesepe
in Monthly Notices of the Royal Astronomical Society
Eisenstein D
(2011)
SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS
in The Astronomical Journal
Relaño M
(2010)
Spatially resolved study of the physical properties of the ionized gas in NGC 595
in Monthly Notices of the Royal Astronomical Society
Oliver S
(2010)
Specific star formation and the relation to stellar mass from 0 < z < 2 as seen in the far-infrared at 70 and 160 µ m
in Monthly Notices of the Royal Astronomical Society
Casey C
(2011)
Spectroscopic characterization of 250-µm-selected hyper-luminous star-forming galaxies 250-µm galaxies at z>1
in Monthly Notices of the Royal Astronomical Society