Search Results - "Procopio, P"
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wsclean: an implementation of a fast, generic wide-field imager for radio astronomy
Published in Monthly notices of the Royal Astronomical Society (11-10-2014)“…Astronomical wide-field imaging of interferometric radio data is computationally expensive, especially for the large data volumes created by modern…”
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2
Extragalactic Peaked-spectrum Radio Sources at Low Frequencies
Published in The Astrophysical journal (20-02-2017)“…We present a sample of 1483 sources that display spectral peaks between 72 MHz and 1.4 GHz, selected from the GaLactic and Extragalactic All-sky Murchison…”
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3
CHIPS: THE COSMOLOGICAL H i POWER SPECTRUM ESTIMATOR
Published in The Astrophysical journal (20-02-2016)“…ABSTRACT Detection of the cosmological neutral hydrogen signal from the Epoch of Reionization (EoR) and estimation of its basic physical parameters are…”
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Characterization of the ionosphere above the Murchison Radio Observatory using the Murchison Widefield Array
Published in Monthly notices of the Royal Astronomical Society (11-11-2017)“…Abstract We detail new techniques for analysing ionospheric activity, using Epoch of Reionization data sets obtained with the Murchison Widefield Array,…”
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5
FIRST SEASON MWA EOR POWER SPECTRUM RESULTS AT REDSHIFT 7
Published in The Astrophysical journal (10-12-2016)“…ABSTRACT The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data and now faces the challenge of overcoming…”
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A search for long-time-scale, low-frequency radio transients
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…We present a search for transient and highly variable sources at low radio frequencies (150-200 MHz) that explores long time-scales of 1-3 yr. We conducted…”
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7
A multifrequency radio continuum study of the Magellanic Clouds – I. Overall structure and star formation rates
Published in Monthly notices of the Royal Astronomical Society (01-10-2018)Get full text
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8
First limits on the 21 cm power spectrum during the Epoch of X-ray heating
Published in Monthly notices of the Royal Astronomical Society (21-08-2016)“…We present first results from radio observations with the Murchison Widefield Array seeking to constrain the power spectrum of 21 cm brightness temperature…”
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9
The jet/wind outflow in Centaurus A: a local laboratory for AGN feedback
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…Abstract We present new radio and optical images of the nearest radio galaxy Centaurus A and its host galaxy NGC 5128. We focus our investigation on the…”
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THE MURCHISON WIDEFIELD ARRAY 21 cm POWER SPECTRUM ANALYSIS METHODOLOGY
Published in The Astrophysical journal (10-07-2016)“…ABSTRACT We present the 21 cm power spectrum analysis approach of the Murchison Widefield Array Epoch of Reionization project. In this paper, we compare the…”
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11
LOW-FREQUENCY OBSERVATIONS OF LINEARLY POLARIZED STRUCTURES IN THE INTERSTELLAR MEDIUM NEAR THE SOUTH GALACTIC POLE
Published in The Astrophysical journal (10-10-2016)“…ABSTRACT We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), covering 625 deg2 centered on = 0hand δ = −27°. The…”
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Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA
Published in The Astrophysical journal (20-08-2018)“…Interferometric arrays seeking to measure the 21 cm signal from the epoch of reionization (EOR) must contend with overwhelmingly bright emission from…”
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13
The First Murchison Widefield Array low-frequency radio observations of cluster scale non-thermal emission: the case of Abell 3667
Published in Monthly notices of the Royal Astronomical Society (21-11-2014)“…We present the first Murchison Widefield Array observations of the well-known cluster of galaxies Abell 3667 (A3667) between 105 and 241 MHz. A3667 is one of…”
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Parametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Array
Published in Monthly notices of the Royal Astronomical Society (01-05-2016)“…Experiments that pursue detection of signals from the Epoch of Reionization (EoR) are relying on spectral smoothness of source spectra at low frequencies. This…”
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15
The spectral energy distribution of powerful starburst galaxies – I. Modelling the radio continuum
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract We have acquired radio-continuum data between 70 MHz and 48 GHz for a sample of 19 southern starburst galaxies at moderate redshifts…”
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Searching for dark matter signals from local dwarf spheroidal galaxies at low radio frequencies in the GLEAM survey
Published in Monthly notices of the Royal Astronomical Society (01-05-2020)“…ABSTRACT The search for emission from weakly interacting massive particle (WIMP) dark matter annihilation and decay has become a multipronged area of research…”
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Modelling of the spectral energy distribution of Fornax A: leptonic and hadronic production of high-energy emission from the radio lobes
Published in Monthly notices of the Royal Astronomical Society (01-02-2015)“…We present new low-frequency observations of the nearby radio galaxy Fornax A at 154 MHz with the Murchison Widefield Array, microwave flux-density…”
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Spectral Energy Distribution and Radio Halo of NGC 253 at Low Radio Frequencies
Published in The Astrophysical journal (20-03-2017)“…We present new radio continuum observations of NGC 253 from the Murchison Widefield Array at frequencies between 76 and 227 MHz. We model the broadband radio…”
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A high reliability survey of discrete Epoch of Reionization foreground sources in the MWA EoR0 field
Published in Monthly notices of the Royal Astronomical Society (01-10-2016)“…Detection of the epoch of reionization H I signal requires a precise understanding of the intervening galaxies and AGN, both for instrumental calibration and…”
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An analysis of the halo and relic radio emission from Abell 3376 from Murchison Widefield Array observations
Published in Monthly notices of the Royal Astronomical Society (21-08-2015)“…We have carried out multiwavelength observations of the nearby (z = 0.046) rich, merging galaxy cluster Abell 3376 with the Murchison Widefield Array (MWA). As…”
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