Ben Tunbridge
University of Manchester
3 Papers
7 Citations
Ben Tunbridge is an academic researcher from University of Manchester. The author has contributed to research in topics: Weak gravitational lensing & Galaxy. The author has an hindex of 3, co-authored 3 publications.
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Papers
SuperCLASS – III. Weak lensing from radio and optical observations in Data Release 1
Ian Harrison,Michael L. Brown,Ben Tunbridge,Daniel Thomas,Tom Hillier,Alasdair Thomson,Lee Whittaker,Filipe B. Abdalla,Richard A. Battye,Anna Bonaldi,Stefano Camera,Caitlin M. Casey,C. Demetroullas,Christopher A. Hales,Christopher A. Hales,Neal Jackson,Scott T. Kay,Sinclaire M. Manning,Aaron Peters,C. J. Riseley,C. J. Riseley,Robert A. Watson +21 more
TL;DR: In this article, the authors describe the first results on weak gravitational lensing from the SuperCLASS survey: the first survey specifically designed to measure the weak lensing effect in radio-wavelength data, both alone and in cross-correlation with optical data.
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SuperCLASS – I. The super cluster assisted shear survey: Project overview and data release 1
Richard A. Battye,Michael L. Brown,Caitlin M. Casey,Ian Harrison,Neal Jackson,Ian Smail,Robert A. Watson,Christopher A. Hales,Christopher A. Hales,Sinclaire M. Manning,Chao-Ling Hung,C. J. Riseley,C. J. Riseley,Filipe B. Abdalla,Mark Birkinshaw,C. Demetroullas,Scott Chapman,Robert Beswick,T. W. B. Muxlow,Anna Bonaldi,Stefano Camera,Tom Hillier,Scott T. Kay,Aaron Peters,David B. Sanders,Daniel Thomas,Alasdair Thomson,Ben Tunbridge,Lee Whittaker +28 more
TL;DR: The SuperCLuster Assisted Shear Survey (SuperCLASS) as mentioned in this paper is a legacy project using the e-MERLIN interferometric array to detect the effects of weak lensing in the radio in preparation for similar measurements with the SKA.
Radio–optical galaxy shape correlations in the COSMOS field
TL;DR: In this paper, the authors investigate the correlations in galaxy shapes between optical and radio wavelengths using archival observations of the COSMOS field and show that cross-correlation studies between different wavebands will become increasingly important for precision cosmology as future large surveys may be dominated by systematic rather than statistical errors.