Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies, and Stellar, planetary, and galactic studies.
Beyond-classical computation in quantum simulation
Quantum critical dynamics in a 5,000-qubit programmable spin glass
Herschel Multitiered Extragalactic Survey: clusters of dusty galaxies uncovered by Herschel★ and Planck†
HerMES: point source catalogues from Herschel-SPIRE observations II★
Detection of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>B</mml:mi></mml:math>-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
HerMES: COSMIC INFRARED BACKGROUND ANISOTROPIES AND THE CLUSTERING OF DUSTY STAR-FORMING GALAXIES
The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3
HerMES: CANDIDATE HIGH-REDSHIFT GALAXIES DISCOVERED WITH<i>HERSCHEL</i>/SPIRE,
HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS
Lancaster EPrints (Lancaster University) 2013cited by 114position: middle
A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUND
Inferring the mass of submillimetre galaxies by exploiting their gravitational magnification of background galaxies
The<i>Herschel</i>Multi-tiered Extragalactic Survey: HerMES
HerMES: deep number counts at 250 <i>μ</i>m, 350 <i>μ</i>m and 500 <i>μ</i>m in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
EVIDENCE FOR ENVIRONMENTAL CHANGES IN THE SUBMILLIMETER DUST OPACITY
HerMES: unveiling obscured star formation – the far-infrared luminosity function of ultraviolet-selected galaxies at z ∼ 1.5
Measuring star formation in high-z massive galaxies: a mid-infrared to submillimetre study of the GOODS NICMOS Survey sample