Quota Studentships
Lead Research Organisation:
University College London
Department Name: Mullard Space Science Laboratory
Abstract
Doctoral Training Partnerships: a range of postgraduate training is funded by the Research Councils. For information on current funding routes, see the common terminology at https://www.ukri.org/apply-for-funding/how-we-fund-studentships/. Training grants may be to one organisation or to a consortia of research organisations. This portal will show the lead organisation only.
Organisations
People |
ORCID iD |
A Smith (Training Grant Holder) |
Publications
Pedram E
(2012)
A Survey of the Hard X-Ray Characteristics of Seismically Active and Quiet White-Light Flares
in Solar Physics
Soria R
(2011)
Accretion states of the Galactic microquasar GRS 1758-258 The Galactic microquasar GRS 1758-258
in Monthly Notices of the Royal Astronomical Society
König S
(2012)
CI, [CII] and CO observations towards TNJ 1338-1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11
in Journal of Physics: Conference Series
Rowan-Robinson M
(2010)
Cold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey? Cold dust and young starbursts
in Monthly Notices of the Royal Astronomical Society
Conley A
(2011)
DISCOVERY OF A MULTIPLY LENSED SUBMILLIMETER GALAXY IN EARLY HerMES HERSCHEL/SPIRE * DATA
in The Astrophysical Journal Letters
Riechers D
(2011)
DYNAMICAL STRUCTURE OF THE MOLECULAR INTERSTELLAR MEDIUM IN AN EXTREMELY BRIGHT, MULTIPLY LENSED z ? 3 SUBMILLIMETER GALAXY DISCOVERED WITH HERSCHEL
in The Astrophysical Journal
Hwang H
(2010)
Evolution of dust temperature of galaxies through cosmic time as seen by Herschel? Evolution of dust temperature of galaxies
in Monthly Notices of the Royal Astronomical Society
Eales S
(2010)
First results from HerMES on the evolution of the submillimetre luminosity function
in Astronomy and Astrophysics
Glenn J
(2010)
HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations HerMES P(D) fluctuation analysis
in Monthly Notices of the Royal Astronomical Society
Béthermin M
(2012)
HerMES: deep number counts at 250 µ m, 350 µ m and 500 µ m in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
in Astronomy & Astrophysics