Search Results - "Vernstrom, T."
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Differences in Faraday Rotation between Adjacent Extragalactic Radio Sources as a Probe of Cosmic Magnetic Fields
Published in The Astrophysical journal (20-06-2019)“…Faraday rotation measures (RMs) of extragalactic radio sources provide information on line-of-sight magnetic fields, including contributions from our Galaxy,…”
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Constraints on large-scale magnetic fields in the intergalactic medium using cross-correlation methods
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT Large-scale coherent magnetic fields in the intergalactic medium (IGM) are presumed to play a key role in the formation and evolution of the cosmic…”
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Discovery of magnetic fields along stacked cosmic filaments as revealed by radio and X-ray emission
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT Diffuse filaments connect galaxy clusters to form the cosmic web. Detecting these filaments could yield information on the magnetic field strength,…”
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New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations
Published in Monthly notices of the Royal Astronomical Society (01-07-2020)“…ABSTRACT Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation provides a means to understand the origin and…”
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Magnetic field strength in cosmic web filaments
Published in Monthly notices of the Royal Astronomical Society (17-03-2022)“…ABSTRACT We used the rotation measure (RM) catalogue derived from the LOFAR Two-metre Sky Survey Data Release 2 (LoTSS DR2) at 144 MHz to measure the evolution…”
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The redshift evolution of extragalactic magnetic fields
Published in Monthly notices of the Royal Astronomical Society (14-07-2022)“…ABSTRACT Faraday rotation studies of distant radio sources can constrain the evolution and the origin of cosmic magnetism. We use data from the LOFAR Two-Metre…”
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RESOLVING THE RADIO SOURCE BACKGROUND: DEEPER UNDERSTANDING THROUGH CONFUSION
Published in The Astrophysical journal (10-10-2012)“…We used the Karl G. Jansky Very Large Array to image one primary beam area at 3 GHz with 8" FWHM resolution and 1.0 mu Jy beam super(-1) rms noise near the…”
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Mysterious odd radio circle near the large magellanic cloud – an intergalactic supernova remnant?
Published in Monthly notices of the Royal Astronomical Society (15-03-2022)“…ABSTRACT We report the discovery of J0624–6948, a low-surface brightness radio ring, lying between the Galactic Plane and the large magellanic cloud (LMC). It…”
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A deep ALMA image of the Hubble Ultra Deep Field
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…Abstract We present the results of the first, deep Atacama Large Millimeter Array (ALMA) imaging covering the full ≃4.5 arcmin2 of the Hubble Ultra Deep Field…”
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Magnetic field evolution in cosmic filaments with LOFAR data
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT Measuring the magnetic field in cosmic filaments reveals how the Universe is magnetized and the process that magnetized it. Using the Rotation…”
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A MeerKAT-meets-LOFAR study of MS 1455.0 + 2232: a 590 kiloparsec ‘mini’-halo in a sloshing cool-core cluster
Published in Monthly notices of the Royal Astronomical Society (06-04-2022)“…ABSTRACT Radio mini-haloes are poorly understood, moderately extended diffuse radio sources that trace the presence of magnetic fields and relativistic…”
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Deep 3-GHz observations of the Lockman Hole North with the Very Large Array – II. Catalogue and μJy source properties
Published in Monthly notices of the Royal Astronomical Society (01-11-2016)“…This is the second of two papers describing the observations and source catalogues derived from sensitive 3-GHz images of the Lockman Hole North using the Karl…”
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The Angular Size Distribution of μJy Radio Sources
Published in The Astrophysical journal (20-03-2018)“…Abstract We made two new sensitive (rms noise μ Jy beam −1 ) high-resolution ( θ = 3.″0 and θ = 0.″66 FWHM) S-band (2 < ν < 4 GHz) images covering a single…”
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Radio fossils, relics, and haloes in Abell 3266: cluster archaeology with ASKAP-EMU and the ATCA
Published in Monthly notices of the Royal Astronomical Society (01-08-2022)“…ABSTRACT Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant substructure. We present new, highly sensitive radio continuum…”
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The deep diffuse extragalactic radio sky at 1.75 GHz
Published in Monthly notices of the Royal Astronomical Society (01-03-2015)“…We present a study of diffuse extragalactic radio emission at 1.75 GHz from part of the ELAIS-S1 (European Large Area Infrared Space Observatory Survey - South…”
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The cosmic radio background from 150 MHz to 8.4 GHz and its division into AGN and star-forming galaxy flux
Published in Monthly notices of the Royal Astronomical Society (02-03-2023)“…ABSTRACT We present a revised measurement of the extragalactic background light (EBL) at radio frequencies based on a near complete compendium of radio source…”
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Deep 3 GHz number counts from a P(D) fluctuation analysis
Published in Monthly notices of the Royal Astronomical Society (21-05-2014)“…Radio source counts constrain galaxy populations and evolution, as well as the global star formation history. However, there is considerable disagreement among…”
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Contribution to the diffuse radio background from extragalactic radio sources
Published in Monthly notices of the Royal Astronomical Society (21-08-2011)“…We examine the brightness of the cosmic radio background (CRB) by comparing the contribution from individual source counts to absolute measurements. We use a…”
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Ram-pressure stripped radio tails detected in the dynamically active environment of the Shapley Supercluster
Published in Monthly notices of the Royal Astronomical Society (01-09-2024)“…ABSTRACT We study the radio continuum emission of four galaxies experiencing ram-pressure stripping in four clusters of the Shapley Supercluster at redshift…”
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Radio polarization properties of quasars and active galaxies at high redshifts
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)Get full text
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