activity
19932025
most citedThe host galaxies of luminous quasars

151 citations · 357 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2025

Reconstructing spatially-varying multiplicative bias for Stage IV weak lensing galaxy surveys with a quadratic estimator

Konstantinos Tanidis, David Alonso, Lance Miller +1

We present a quadratic estimator that detects and reconstructs spatially-varying multiplicative () bias in weak lensing shear measurements, by exploiting the mode coupling…

astro-ph.GA2025

Measuring the Evolution of Bulge, Disk and Colour Gradients in HST Observations of Galaxies with 3D Modelling

N. Welikala, L. Miller, A. N. Taylor +1

We measure galaxy structural properties and colour gradients using HST images to trace the evolution of galaxy components. We jointly fit 3D bulge and disk models to 2505 galaxies…

astro-ph.CO2025

Exploring the Masses of the Two Most Distant Gravitational Lensing Clusters at the Cosmic Noon

Jinhyub Kim, M. James Jee, Stefano Andreon +4

Observations over the past decade have shown that galaxy clusters undergo the most transformative changes during the epoch. However, challenges such as low lensing ef…

astro-ph2003★ 151 cited

The host galaxies of luminous quasars

D. J. E. Floyd, M. J. Kukula, J. S. Dunlop +5

We present results of a deep HST/WFPC2 imaging study of 17 quasars at z~0.4, designed to determine the properties of their host galaxies. The sample consists of quasars with absolu…

astro-ph1995★ 106 cited

AN IMAGING K-BAND SURVEY - II: THE REDSHIFT SURVEY AND GALAXY EVOLUTION IN THE INFRARED

Karl Glazebrook, J. A. Peacock, L. Miller +1

We present a redshift survey of 124 galaxies, from an imaging -band survey complete to . The optical-to-infrared colours are consistent with the range expected fro…

astro-ph1993★ 100 cited

An imaging K-band survey - I: The catalogue, star and galaxy counts

Karl Glazebrook, J. A. Peacock, C. A. Collins +1

We present results from a large area (552\,\sqamin) imaging -band survey to a 5 limit of . We have optical-infrared colours of almost all the objects in the sam…