activity
20122017
most citedInitial LOFAR observations of Epoch of Reionization windows: II. Diffuse polarized emission in the ELAIS-N1 field

82 citations · 177 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2017★ 17 cited

VOEvent Standard for Fast Radio Bursts

Emily Petroff, Leon Houben, Keith Bannister +13

Fast radio bursts are a new class of transient radio phenomena currently detected as millisecond radio pulses with very high dispersion measures. As new radio surveys begin searchi…

astro-ph.CO2015★ 2 cited

Polarization leakage in Epoch of Reionization windows: I. LOFAR observations of the 3C196 field

K. M. B. Asad, L. V. E. Koopmans, V. Jelić +25

Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially because, even after removing the foregrounds, the residual Stokes maps conta…

astro-ph.IM2014★ 25 cited

Lunar occultation of the diffuse radio sky: LOFAR measurements between 35 and 80 MHz

H. K. Vedantham, L. V. E. Koopmans, A. G. de Bruyn +91

We present radio observations of the Moon between and MHz to demonstrate a novel technique of interferometrically measuring large-scale diffuse emission extending far bey…

astro-ph.GA2014★ 82 cited

Initial LOFAR observations of Epoch of Reionization windows: II. Diffuse polarized emission in the ELAIS-N1 field

V. Jelic, A. G. de Bruyn, M. Mevius +106

This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to address its possible implications for the extraction of the cosmological 21-cm signal…

astro-ph.IM2013

LEDDB: LOFAR Epoch of Reionization Diagnostic Database

O. Martinez-Rubi, V. K. Veligatla, A. G. de Bruyn +6

One of the key science projects of the Low-Frequency Array (LOFAR) is the detection of the cosmological signal coming from the Epoch of Reionization (EoR). Here we present the LOFA…

astro-ph.CO2012★ 51 cited

Imaging neutral hydrogen on large-scales during the Epoch of Reionization with LOFAR

S. Zaroubi, A. G. de Bruyn, G. Harker +17

The first generation of redshifted 21 cm detection experiments, carried out with arrays like LOFAR, MWA and GMRT, will have a very low signal-to-noise ratio per resolution element…