Search Results - "Yatawatta, S."
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Adaptive weighting in radio interferometric imaging
Published in Monthly notices of the Royal Astronomical Society (11-10-2014)“…Radio interferometers observe the Fourier space of the sky, at locations determined by the array geometry. Before a real space image is constructed by a…”
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Improved upper limits on the 21 cm signal power spectrum of neutral hydrogen at z ≈ 9.1 from LOFAR
Published in Monthly notices of the Royal Astronomical Society (01-04-2020)“…ABSTRACT A new upper limit on the 21 cm signal power spectrum at a redshift of z ≈ 9.1 is presented, based on 141 h of data obtained with the Low-Frequency…”
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Constraining the intergalactic medium at z ≈ 9.1 using LOFAR Epoch of Reionization observations
Published in Monthly notices of the Royal Astronomical Society (01-04-2020)“…ABSTRACT We derive constraints on the thermal and ionization states of the intergalactic medium (IGM) at redshift ≈ 9.1 using new upper limits on the 21-cm…”
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The first power spectrum limit on the 21-cm signal of neutral hydrogen during the Cosmic Dawn at z = 20–25 from LOFAR
Published in Monthly notices of the Royal Astronomical Society (2019)“…ABSTRACT Observations of the redshifted 21-cm hyperfine line of neutral hydrogen from early phases of the Universe such as Cosmic Dawn and the Epoch of…”
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Robust radio interferometric calibration using the t-distribution
Published in Monthly notices of the Royal Astronomical Society (11-10-2013)“…A major stage of radio interferometric data processing is calibration or the estimation of systematic errors in the data and the correction for such errors. A…”
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The AARTFAAC Cosmic Explorer: observations of the 21-cm power spectrum in the EDGES absorption trough
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT The 21-cm absorption feature reported by the EDGES collaboration is several times stronger than that predicted by traditional astrophysical models. If…”
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Upper Limits on the 21 cm Epoch of Reionization Power Spectrum from One Night with LOFAR
Published in The Astrophysical journal (20-03-2017)“…We present the first limits on the Epoch of Reionization 21 cm H i power spectra, in the redshift range z = 7.9-10.6, using the Low-Frequency Array (LOFAR)…”
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Probing ionospheric structures using the LOFAR radio telescope
Published in Radio science (01-07-2016)“…LOFAR is the LOw‐Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we present results on ionospheric structures derived from 29 LOFAR…”
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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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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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A numerical study of 21-cm signal suppression and noise increase in direction-dependent calibration of LOFAR data
Published in Monthly notices of the Royal Astronomical Society (01-01-2022)“…ABSTRACT We investigate systematic effects in direction-dependent gain calibration in the context of the Low-Frequency Array (LOFAR) 21-cm Epoch of…”
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Wide-field LOFAR-LBA power-spectra analyses: impact of calibration, polarization leakage, and ionosphere
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)Get full text
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Clustered calibration: an improvement to radio interferometric direction-dependent self-calibration
Published in Monthly notices of the Royal Astronomical Society (01-04-2013)“…The new generation of radio synthesis arrays, such as Low Frequency Array and Square Kilometre Array, have been designed to surpass existing arrays in terms of…”
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A novel radio imaging method for physical spectral index modelling
Published in Monthly notices of the Royal Astronomical Society (01-09-2023)“…ABSTRACT We present a new method, called ‘forced-spectrum fitting’, for physically based spectral modelling of radio sources during deconvolution. This…”
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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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Probing reionization with LOFAR using 21-cm redshift space distortions
Published in Monthly notices of the Royal Astronomical Society (11-10-2013)“…One of the most promising ways to study the epoch of reionization (EoR) is through radio observations of the redshifted 21-cm line emission from neutral…”
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Polarization leakage in epoch of reionization windows – II. Primary beam model and direction-dependent calibration
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)“…Leakage of diffuse polarized emission into Stokes I caused by the polarized primary beam of the instrument might mimic the spectral structure of the 21-cm…”
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Radio interferometric calibration via ordered-subsets algorithms: OS-LS and OS-SAGE calibrations
Published in Monthly notices of the Royal Astronomical Society (01-10-2013)“…The main objective of this work is to accelerate the maximum likelihood (ML) estimation procedure in radio interferometric calibration. We introduce the…”
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Imaging neutral hydrogen on large scales during the Epoch of Reionization with LOFAR
Published in Monthly notices of the Royal Astronomical Society (01-10-2012)“…ABSTRACT The first generation of redshifted 21 cm detection experiments, carried out with arrays like Low Frequency Array (LOFAR), Murchison Widefield Array…”
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LOFAR insights into the epoch of reionization from the cross-power spectrum of 21 cm emission and galaxies
Published in Monthly notices of the Royal Astronomical Society (01-07-2013)“…Using a combination of N-body simulations, semi-analytic models and radiative transfer calculations, we have estimated the theoretical cross-power spectrum…”
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