Publication
Galaxy size trends as a consequence of cosmology
We show that recently documented trends in galaxy sizes with mass and redshift can be understood in terms of the influence of underlying cosmic evolution; a...
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PublicationGalaxy sizes and the galaxy-halo connection - I. The remarkable tightness of the size distributionsThe mass and structural assembly of galaxies is a matter of intense debate. Current theoretical models predict the existence of a linear relationship between...
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PublicationGalaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0We present the galaxy stellar mass function and its evolution in clusters from z˜ 0.8 to the current epoch, based on the WIde-field Nearby Galaxy-cluster Survey...
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PublicationGalaxy-galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlationThe DMASS sample is a photometric sample from the DES Year 1 data set designed to replicate the properties of the CMASS sample from BOSS, in support of a joint...
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PublicationGalaxy-wide radio-induced feedback in a radio-quiet quasarWe report the discovery of a radio-quiet type 2 quasar (SDSS J165315.06+234943.0 nicknamed the `Beetle' at z = 0.103) with unambiguous evidence for active...
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PublicationGAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxiesWe use multiwavelength data from the Galaxy And Mass Assembly (GAMA) and Herschel-ATLAS (H-ATLAS) surveys to compare the relationship between various dust...
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PublicationGamma-ray observations of MAXI J1820+070 during the 2018 outburstMAXI J1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018...
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PublicationGas and dust from solar metallicity AGB starsWe study the asymptotic giant branch (AGB) evolution of stars with masses between 1 M⊙and8.5 M⊙. We focus on stars with a solar chemical composition, which...
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PublicationGas expulsion by quasar-driven winds as a solution to the overcooling problem in galaxy groups and clustersGalaxy groups are not scaled down versions of massive galaxy clusters - the hot gas in groups [known as the intragroup medium (IGrM)] is, on average, less dense...