Search Results - "De Bruyn, A. G."
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Foreground simulations for the LOFAR–epoch of reionization experiment
Published in Monthly notices of the Royal Astronomical Society (21-09-2008)“…Future high-redshift 21-cm experiments will suffer from a high degree of contamination, due both to astrophysical foregrounds and to non-astrophysical and…”
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Power spectrum extraction for redshifted 21-cm Epoch of Reionization experiments: the LOFAR case
Published in Monthly notices of the Royal Astronomical Society (11-07-2010)“…One of the aims of the Low Frequency Array (LOFAR) Epoch of Reionization (EoR) project is to measure the power spectrum of variations in the intensity of…”
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Post-correlation radio frequency interference classification methods
Published in Monthly notices of the Royal Astronomical Society (11-06-2010)“…We describe and compare several post-correlation radio frequency interference (RFI) classification methods. As data sizes of observations grow with new and…”
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Three episodes of jet activity in the Fanaroff–Riley type II radio galaxy B0925+420
Published in Monthly notices of the Royal Astronomical Society (11-12-2007)“…We present Very Large Array images of a ‘double–double radio galaxy’, a class of objects in which two pairs of lobes are aligned either side of the nucleus. In…”
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Detection and extraction of signals from the epoch of reionization using higher-order one-point statistics
Published in Monthly notices of the Royal Astronomical Society (11-03-2009)“…Detecting redshifted 21-cm emission from neutral hydrogen in the early Universe promises to give direct constraints on the epoch of reionization (EoR). It…”
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Non-parametric foreground subtraction for 21-cm epoch of reionization experiments
Published in Monthly notices of the Royal Astronomical Society (01-08-2009)“…One of the problems facing experiments designed to detect redshifted 21-cm emission from the epoch of reionization (EoR) is the presence of foregrounds which…”
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Fast large-scale reionization simulations
Published in Monthly notices of the Royal Astronomical Society (2009)“…We present an efficient method to generate large simulations of the epoch of reionization without the need for a full three-dimensional radiative transfer…”
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Foreground removal using fastica: a showcase of LOFAR-EoR
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…We introduce a new implementation of the fastica algorithm on simulated Low Frequency Array Epoch of Reionization data with the aim of accurately removing the…”
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Interstellar scintillation as the origin of the rapid radio variability of the quasar J1819+3845
Published in Nature (London) (03-01-2002)“…The liberation of gravitational energy as matter falls onto a supermassive black hole at the centre of a galaxy is believed to explain the high luminosity of…”
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A comprehensive radio view of the extremely bright gamma-ray burst 130427A
Published in Monthly notices of the Royal Astronomical Society (11-11-2014)“…GRB 130427A was extremely bright as a result of occurring at low redshift whilst the energetics were more typical of high-redshift gamma-ray bursts (GRBs). We…”
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Polarization leakage in epoch of reionization windows – I. Low Frequency Array observations of the 3C196 field
Published in Monthly notices of the Royal Astronomical Society (21-08-2015)“…Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially because, even after removing the foregrounds, the residual…”
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Post-correlation filtering techniques for off-axis source and RFI removal
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…Techniques to improve the data quality of interferometric radio observations are considered. Fundaments of fringe frequencies in the u v-plane are discussed…”
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Constraints on cosmological parameters from the analysis of the cosmic lens all sky survey radio-selected gravitational lens statistics
Published in Physical review letters (07-10-2002)“…We derive constraints on cosmological parameters and the properties of the lensing galaxies from gravitational lens statistics based on the final Cosmic Lens…”
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The Discovery of a Microarcsecond Quasar: J1819+3845
Published in The Astrophysical journal (01-02-2000)“…We report on the discovery of a source that exhibits over 300% amplitude changes in radio flux density on the period of hours. This source, J1819+3845, is the…”
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Extremely anisotropic scintillations
Published in Monthly notices of the Royal Astronomical Society (21-07-2009)“…A small number of quasars exhibit interstellar scintillation on time-scales less than an hour; their scintillation patterns are all known to be anisotropic…”
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Realistic simulations of the Galactic polarized foreground: consequences for 21-cm reionization detection experiments
Published in Monthly notices of the Royal Astronomical Society (21-12-2010)“…Experiments designed to measure the redshifted 21-cm line from the epoch of reionization (EoR) are challenged by strong astrophysical foreground contamination,…”
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Radio interferometric calibration using the SAGE algorithm
Published in Monthly notices of the Royal Astronomical Society (01-06-2011)“…The aim of the new generation of radio synthesis arrays such as LOw Frequency ARray (LOFAR) and Square Kilometre Array (SKA) is to achieve much higher…”
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The Cosmic Lens All-Sky Survey - I. Source selection and observations
Published in Monthly notices of the Royal Astronomical Society (01-05-2003)“…The Cosmic Lens All-Sky Survey (CLASS) is an international collaborative programme which has obtained high-resolution radio images of over 10 000 flat-spectrum…”
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The Cosmic Lens All-Sky Survey - II. Gravitational lens candidate selection and follow-up
Published in Monthly notices of the Royal Astronomical Society (01-05-2003)“…We report the final results of the search for gravitationally lensed flat-spectrum radio sources found in the combination of CLASS (Cosmic Lens All-Sky Survey)…”
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Astronomical constraints on the cosmic evolution of the fine structure constant and possible quantum dimensions
Published in Physical review letters (25-12-2000)“…We present measurements of absorption by the 21 cm hyperfine transition of neutral hydrogen toward radio sources at substantial look-back times. These data are…”
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