Search Results - "O'SULLIVAN, S. P"
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Magnetic field strength and spectral distribution of six parsec-scale active galactic nuclei jets
Published in Monthly notices of the Royal Astronomical Society (21-11-2009)“…We use observations of six ‘blazars’ with the Very Long Baseline Array (VLBA), at eight frequencies (4.6, 5.1, 7.9, 8.9, 12.9, 15.4, 22.2 and 43.1 GHz), to…”
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Complex Faraday depth structure of active galactic nuclei as revealed by broad-band radio polarimetry
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…We present a detailed study of the Faraday depth structure of four bright (>1 Jy), strongly polarized, unresolved radio-loud quasars. The Australia Telescope…”
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3
Coherent radio emission from a quiescent red dwarf indicative of star–planet interaction
Published in Nature astronomy (01-06-2020)“…Low-frequency ( ν ≲ 150 MHz) stellar radio emission is expected to originate in the outer corona at heights comparable to and larger than the stellar radius…”
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Improving Graduate Education to Support a Branching Career Pipeline: Recommendations Based on a Survey of Doctoral Students in the Basic Biomedical Sciences
Published in CBE life sciences education (01-09-2011)“…Today's doctoral programs continue to prepare students for a traditional academic career path despite the inadequate supply of research-focused faculty…”
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FARADAY ROTATION FROM MAGNESIUM II ABSORBERS TOWARD POLARIZED BACKGROUND RADIO SOURCES
Published in The Astrophysical journal (01-11-2014)“…Strong singly ionized magnesium (Mg II) absorption lines in quasar spectra typically serve as a proxy for intervening galaxies along the line of sight…”
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Faraday rotation at low frequencies: magnetoionic material of the large FRII radio galaxy PKS J0636−2036
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)“…Abstract We present a low-frequency, broad-band polarization study of the FRII radio galaxy PKS J0636−2036 (z = 0.0551), using the Murchison Widefield Array…”
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The magnetic field strength of the Faraday screen surrounding the radio galaxy Coma A
Published in Monthly notices of the Royal Astronomical Society (01-02-2019)Get full text
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Three-dimensional magnetic field structure of six parsec-scale active galactic nuclei jets
Published in Monthly notices of the Royal Astronomical Society (21-02-2009)“…The parsec-scale Faraday rotation measure (RM) distribution of six ‘blazars’ (0954+658, 1156+295, 1418+546, 1749+096, 2007+777 and 2200+420) are investigated…”
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The parsec-scale distributions of intensity, linear polarization and Faraday rotation in the core and jet of Mrk 501 at 8.4–1.6 GHz
Published in Monthly notices of the Royal Astronomical Society (11-02-2010)“…Previous very long baseline interferometry (VLBI) observations of the nearby (z = 0.0337) active galactic nucleus (AGN) Mrk 501 have revealed a complex…”
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GIANT LOBES OF CENTAURUS A RADIO GALAXY OBSERVED WITH THE SUZAKU X-RAY SATELLITE
Published in The Astrophysical journal (20-03-2013)“…We report on Suzaku observations of selected regions within the southern giant lobe of the radio galaxy Centaurus A. In our analysis we focus on distinct X-ray…”
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Radio circular polarization produced in helical magnetic fields in eight active galactic nuclei
Published in Monthly notices of the Royal Astronomical Society (01-03-2008)“…Homan & Lister have recently published circular polarization (CP) detections for 34 objects in the MOJAVE sample – a set of bright, compact active galactic…”
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12
Multifrequency polarization properties of 10 quasars on decaparsec scales at z > 3
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…Global very long baseline interferometry (VLBI) (European VLBI Network + Very Long Baseline Array) polarization observations at 5 and 8.4 GHz of 10…”
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Broad-band, radio spectro-polarimetric study of 100 radiative-mode and jet-mode AGN
Published in Monthly notices of the Royal Astronomical Society (01-08-2017)“…Abstract We present the results from a broad-band (1 to 3 GHz), spectro-polarimetry study of the integrated emission from 100 extragalactic radio sources with…”
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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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Broadband Radio Polarimetry of Fornax A. I. Depolarized Patches Generated by Advected Thermal Material from NGC 1316
Published in The Astrophysical journal (01-03-2018)“…We present observations and analysis of the polarized radio emission from the nearby radio galaxy Fornax A over 1.28-3.1 GHz, using data from the Australia…”
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The Faraday Rotation Measure Grid of the LOFAR Two-metre Sky Survey: Data Release 2
Published in Monthly notices of the Royal Astronomical Society (01-03-2023)“…ABSTRACT A Faraday rotation measure (RM) catalogue, or RM Grid, is a valuable resource for the study of cosmic magnetism. Using the second data release (DR2)…”
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The radio to GeV picture of PSR B1259-63 during the 2021 periastron passage
Published in Monthly notices of the Royal Astronomical Society (01-03-2024)“…ABSTRACT PSR B1259-63 is a gamma-ray binary system with a radio pulsar orbiting an O9.5Ve star, LS 2883, with a period of ${\sim} 3.4$ yr. Close to the…”
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Blazar jet evolution revealed by multi-epoch broad-band radio polarimetry
Published in Monthly notices of the Royal Astronomical Society (21-05-2019)Get full text
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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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