activity
20092019
most citedIonospheric Calibration of Low Frequency Radio Interferometric Observations using the Peeling Scheme: I. Method Description and First Results

368 citations · 1.3k across the 13 of their papers we have counts for

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6 papers · 1 filter

astro-ph.IM2019★ 31 cited

Precision requirements for interferometric gridding in 21-cm power spectrum analysis

A. R. Offringa, F. Mertens, S. van der Tol +4

We analyse the accuracy of radio interferometric gridding of visibilities with the aim to quantify the Epoch of Reionization (EoR) 21-cm power spectrum bias caused by gridding, ult…

astro-ph.IM2016★ 139 cited

Probing Ionospheric Structures using the LOFAR radio telescope

M. Mevius, S. van der Tol, V. N. Pandey +24

LOFAR is the LOw Frequency Radio interferometer ARray located at mid-latitude (). Here, we present results on ionospheric structures derived from 29 LOFAR nighttim…

astro-ph.IM2016★ 282 cited

LOFAR facet calibration

R. J. van Weeren, W. L. Williams, M. J. Hardcastle +39

LOFAR, the Low-Frequency Array, is a powerful new radio telescope operating between 10 and 240 MHz. LOFAR allows detailed sensitive high-resolution studies of the low-frequency rad…

astro-ph.IM2010★ 3 cited

Progress with the LOFAR Imaging Pipeline

George Heald, John McKean, Roberto Pizzo +14

One of the science drivers of the new Low Frequency Array (LOFAR) is large-area surveys of the low-frequency radio sky. Realizing this goal requires automated processing of the int…

astro-ph.IM2010★ 76 cited

Calibration Challenges for Future Radio Telescopes

Stefan J. Wijnholds, Sebastiaan van der Tol, Ronald Nijboer +1

Instruments for radio astronomical observations have come a long way. While the first telescopes were based on very large dishes and 2-antenna interferometers, current instruments…

astro-ph.IM2009★ 368 cited

Ionospheric Calibration of Low Frequency Radio Interferometric Observations using the Peeling Scheme: I. Method Description and First Results

H. T. Intema, S. van der Tol, W. D. Cotton +3

Calibration of radio interferometric observations becomes increasingly difficult towards lower frequencies. Below ~300 MHz, spatially variant refractions and propagation delays of…