activity
19952024
most citedThe UKIRT Infrared Deep Sky Survey (UKIDSS)

2.5k citations · 16.8k across the 147 of their papers we have counts for

collaborators

150 papers

astro-ph.GA2024★ 12 cited

[OIII] emission in z=2 quasars with and without Broad Absorption Lines

Matthew J. Temple, Amy L. Rankine, Manda Banerji +6

Understanding the links between different phases of outflows from active galactic nuclei is a key goal in extragalactic astrophysics. Here we compare [OIII] 4960,5008 outflow s…

astro-ph.CO2024★ 550 cited

Euclid. I. Overview of the Euclid mission

Euclid Collaboration, Y. Mellier, Abdurro'uf +1134

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Eucl…

astro-ph.GA2023★ 13 cited

No redshift evolution in the rest-frame UV emission line properties of quasars from z=1.5 to z=4.0

Matthew Stepney, Manda Banerji, Paul C. Hewett +4

We analyse the rest-frame UV spectra of 2,531 high-redshift (3.5<z<4.0) quasars from the Sloan Digital Sky Survey DR16Q catalogue. In combination with previous work, we study the r…

astro-ph.GA2023★ 49 cited

Testing AGN outflow and accretion models with CIV and HeII emission line demographics in z=2 quasars

Matthew J. Temple, James H. Matthews, Paul C. Hewett +6

Using 190,000 spectra from the seventeenth data release of the Sloan Digital Sky Survey, we investigate the ultraviolet emission line properties in z=2 quasars. Specifically, we qu…

astro-ph.GA2021★ 27 cited

HST/WFC3 grism observations of clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H maps

Jasleen Matharu, Adam Muzzin, Gabriel B. Brammer +12

We present and publicly release (https://www.gclasshst.com) the first spatially resolved H maps of star-forming cluster galaxies at , made possible with the Wide Field C…

astro-ph.GA2021★ 70 cited

Modelling type 1 quasar colours in the era of Rubin and Euclid

Matthew J. Temple, Paul C. Hewett, Manda Banerji

We construct a parametric SED model which is able to reproduce the average observed SDSS-UKIDSS-WISE quasar colours to within one tenth of a magnitude across a wide range of redshi…