Simon Dye

TL;DR: In this article, the authors used the science demonstration field data of the Herschel Astrophysical Terahertz Large Area Survey to study how star formation, traced by the far-infrared Herschel data, is related to both the accretion luminosity and redshift of quasars selected from the SDSS and the 2dF-SDSS luminous red galaxy (LRG) and Quasar Spectroscopic Catalogue survey.

TL;DR: In this article, the authors used data from the Herschel-ATLAS to investigate the evolution of the far-infrared-radio correlation over the redshift range 0 5 sigma sources in the Science Demonstration Field and cross-matching these data with radio data from Faint Images of the Radio Sky at Twenty-Centimetres (FIRST) survey and the NRAO Very Large Array (VLA) Northern Sky Survey (NVSS).

TL;DR: In this article, the authors used the semi-linear method of Warren & Dye (2003), which pixelises the source surface brightness distribution, to invert the Einstein ring for sets of parameterised lens models.

TL;DR: The robustness of adaptive SLI provides a firm foundation for the development of a strong lens modelling pipeline, which will become necessary in the short-term future to cope with the increasing rate of discovery of new strong lens systems.

TL;DR: In this paper, the authors describe the updated quasar candidate selection procedure, report the discovery of 16 quasars at $6.4\lesssim z \lesssim6.7$ and present the quasar luminosity function (QLF).