activity
19992023
most citedDiscovery of six Ly alpha emitters near a radio galaxy at z ~ 5.2

112 citations · 428 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2023★ 40 cited

The LOFAR LBA Sky Survey II. First data release

F. de Gasperin, H. W. Edler, W. L. Williams +27

The Low Frequency Array (LOFAR) is the only existing radio interferometer able to observe at ultra-low frequencies (<100 MHz) with high resolution (<15") and high sensitivity (<1 m…

astro-ph.CO2022★ 28 cited

Deep low-frequency radio observations of Abell 2256 II: The ultra-steep spectrum radio halo

K. Rajpurohit, E. Osinga, M. Brienza +17

We present the first detailed analysis of the radio halo in the merging galaxy cluster Abell 2256 using the LOFAR, uGMRT, and VLA. These observations combined with archival X-ray d…

astro-ph.GA2018★ 71 cited

Discovery of a radio galaxy at z = 5.72

A. Saxena, M. Marinello, R. A. Overzier +11

We report the discovery of the most distant radio galaxy to date, TGSS1530 at a redshift of close to the presumed end of the Epoch of Reionisation. The radio galaxy was se…

astro-ph.GA2018★ 31 cited

A search for faint high-redshift radio galaxy candidates at 150 MHz

A. Saxena, P. Jagannathan, H. J. A. Röttgering +6

Ultra-steep spectrum (USS) radio sources are good tracers of powerful radio galaxies at . Identification of even a single bright radio galaxy at can be used to detec…

astro-ph2006★ 6 cited

LOFAR - Opening up a new window on the Universe

H. J. A. Rottgering, R. Braun, P. D. Barthel +31

LOFAR, the Low Frequency Array, is a next-generation radio telescope that is being built in Northern Europe and expected to be fully operational at the end of this decade. It will…

astro-ph2005★ 84 cited

An Overdensity of Galaxies near the Most Distant Radio-Loud Quasar

W. Zheng, R. Overzier, R. J. Bouwens +41

A five square arcminute region around the luminous radio-loud quasar SDSS J0836+0054 (z=5.8) hosts a wealth of associated galaxies, characterized by very red (1.3 < i_775 - z_{850}…