Context. There are a number of hardware upgrades for the Low-Frequency Array (LOFAR) currently under development. These upgrades are collectively referred to as the LOFAR 2.0 upgrade. The first stage of LOFAR 2.0 will introduce a distributed clock signal and allow for simultaneous observations using all the low-band and high-band antennas of the array. Aims. Our aim is to provide a tool for obtaining accurate simulations for LOFAR 2.0. Methods. We present our software for simulating LOFAR and LOFAR 2.0 observations, which includes realistic models for all important systematic effects such as the first- and second-order ionospheric corruptions, time-variable primary-beam attenuation, station-based delays, and bandpass response. The ionospher...
LOFAR is a revolutionary instrument, operating at low frequencies (ν ≤ 240 MHz). It will drive major...
International audienceThe Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extraga...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we pres...
To obtain high quality images with the Lofar low frequency radio telescope, accurate ionospheric cha...
This data accompanies the work "Investigating Ionospheric Calibration for LOFAR 2.0 with Simulated O...
Several low frequency radio astronomy arrays are currently under development. For example the LOFAR ...
Context. New generation low-frequency telescopes are exploring a new parameter space in terms of dep...
The Earth’s ionosphere is a highly variable medium on a wide range of spatio-temporal scales. The re...
Calibration of radio interferometric observations becomes increasingly difficult towards lower frequ...
We investigate systematic effects in direction-dependent gain calibration in the context of the Low-...
Abstract — One of the challenges in the design of the LOFAR radio telescope is the calibration of th...
The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic surveys. It has...
This paper is part of the 1st data release of the LoTSS Deep Fields. Electronic data catalogues will...
Context. The ionosphere is the main driver of a series of systematic effects that limit our ability ...
LOFAR is a revolutionary instrument, operating at low frequencies (ν ≤ 240 MHz). It will drive major...
International audienceThe Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extraga...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we pres...
To obtain high quality images with the Lofar low frequency radio telescope, accurate ionospheric cha...
This data accompanies the work "Investigating Ionospheric Calibration for LOFAR 2.0 with Simulated O...
Several low frequency radio astronomy arrays are currently under development. For example the LOFAR ...
Context. New generation low-frequency telescopes are exploring a new parameter space in terms of dep...
The Earth’s ionosphere is a highly variable medium on a wide range of spatio-temporal scales. The re...
Calibration of radio interferometric observations becomes increasingly difficult towards lower frequ...
We investigate systematic effects in direction-dependent gain calibration in the context of the Low-...
Abstract — One of the challenges in the design of the LOFAR radio telescope is the calibration of th...
The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic surveys. It has...
This paper is part of the 1st data release of the LoTSS Deep Fields. Electronic data catalogues will...
Context. The ionosphere is the main driver of a series of systematic effects that limit our ability ...
LOFAR is a revolutionary instrument, operating at low frequencies (ν ≤ 240 MHz). It will drive major...
International audienceThe Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extraga...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we pres...