activity
20172026
most citedThe environment and host haloes of the brightest z~6 Lyman-break galaxies

20 citations · 23 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

MIGHTEE/COSMOS-3D: The discovery of three spectroscopically confirmed radio-selected star-forming galaxies at z=4.9-5.6

R. G. Varadaraj, A. Saxena, S. Fakiolas +10

Radio observations offer a dust-independent probe of star formation and active galactic nucleus (AGN) activity, but sufficiently deep data are required to access the crossover lumi…

astro-ph.GA2025

Euclid: Discovery of bright Lyman-break galaxies in UltraVISTA and Euclid COSMOS

R. G. Varadaraj, R. A. A. Bowler, M. J. Jarvis +163

We present a search for Lyman-break galaxies using the near-infrared UltraVISTA survey in the COSMOS field, reaching depths in of 26.2. W…

astro-ph.GA2025

Evidence for inverse Compton scattering in high-redshift Lyman-break galaxies

I. H. Whittam, M. J. Jarvis, Eric J. Murphy +13

Radio continuum emission provides a unique opportunity to study star-formation unbiased by dust obscuration. However, if radio observations are to be used to accurately trace star-…

astro-ph.GA2025★ 2 cited

A 15 Mpc rotating galaxy filament at redshift z = 0.032

Madalina N. Tudorache, S. L. Jung, M. J. Jarvis +6

Understanding the cold atomic hydrogen gas (HI) within cosmic filaments has the potential to pin down the relationship between the low density gas in the cosmic web and how the gal…

astro-ph.CO2025★ 1 cited

Angular correlation functions of bright Lyman-break galaxies at

Isabelle Ye, Philip Bull, Rebecca A. A. Bowler +3

We investigate the clustering of Lyman-break galaxies at redshifts of 3 5 within the COSMOS field by measuring the angular two-point correlation function. Our…

astro-ph.GA2017★ 20 cited

The environment and host haloes of the brightest z~6 Lyman-break galaxies

P. W. Hatfield, R. A. A. Bowler, M. J. Jarvis +1

By studying the large-scale structure of the bright high-redshift Lyman-break galaxy (LBG) population it is possible to gain an insight into the role of environment in galaxy forma…