activity
20142023
most citedThe LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release

654 citations · 1.1k across the 11 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA201645 cited

A large H survey of star formation in relaxed and merging galaxy cluster environments at

Andra Stroe, David Sobral, Ana Afonso +4

We present the first results from the largest H survey of star formation and AGN activity in galaxy clusters. Using 9 different narrow band filters, we select H emitt…

astro-ph.GA201614 cited

The growth of typical star-forming galaxies and their super massive black holes across cosmic time since z~2

João Calhau, David Sobral, Andra Stroe +5

Understanding galaxy formation and evolution requires studying the interplay between the growth of galaxies and the growth of their black holes across cosmic time. Here we explore…

astro-ph.GA2016107 cited

The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.23

David Sobral, Jorryt Matthee, Philip Best +6

We present the CAlibrating LYMan- with H (CALYMHA) pilot survey and new results on Lyman- (Lya) selected galaxies at z~2. We use a custom-built Lya narrow-band filter at t…

astro-ph.GA201475 cited

The rise and fall of star-formation in merging galaxy clusters

Andra Stroe, David Sobral, William Dawson +6

CIZA J2242.8+5301 (`Sausage') and 1RXS J0603.3+4213 (`Toothbrush') are two low-redshift (), massive (), post-core passage merging clusters, whi…

astro-ph.GA201468 cited

Spectral age modelling of the `Sausage' cluster radio relic

Andra Stroe, Jeremy J. Harwood, Martin J. Hardcastle +1

CIZA J2242.8+5301 is a post-core passage, binary merging cluster that hosts a large, thin, arc-like radio relic, nicknamed the `Sausage', tracing a relatively strong shock front. W…

astro-ph.GA2014

The spectral structure and energetics of powerful radio sources

J. J. Harwood, M. J. Hardcastle, J. H. Croston +3

Determining the energy spectrum of an electron population can give key insights into the underlying physics of a radio source; however, the lack of high resolution, broad-bandwidth…