Search Results - "Pierce, J. C. S"
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The radio properties of high-excitation radio galaxies with intermediate radio powers
Published in Monthly notices of the Royal Astronomical Society (11-05-2020)“…ABSTRACT In the past decade, high-sensitivity radio surveys have revealed that the local radio active galactic nucleus population is dominated by…”
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Do AGN triggering mechanisms vary with radio power? – I. Optical morphologies of radio-intermediate HERGs
Published in Monthly notices of the Royal Astronomical Society (21-08-2019)“…ABSTRACT Active galactic nuclei (AGNs) with intermediate radio powers are capable of driving multiphase outflows in galaxy bulges, and are also more common…”
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Galaxy interactions are the dominant trigger for local type 2 quasars
Published in Monthly notices of the Royal Astronomical Society (21-04-2023)“…ABSTRACT The triggering mechanism for the most luminous, quasar-like active galactic nuclei (AGN) remains a source of debate, with some studies favouring…”
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4
Accretion mode versus radio morphology in the LOFAR Deep Fields
Published in Monthly notices of the Royal Astronomical Society (18-02-2022)“…ABSTRACT Radio-loud active galaxies have two accretion modes [radiatively inefficient (RI) and radiatively efficient (RE)], with distinct optical and infrared…”
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5
Do AGN triggering mechanisms vary with radio power? – II. The importance of mergers as a function of radio power and optical luminosity
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT Investigation of the triggering mechanisms of radio active galactic nuclei (radio AGN) is important for improving our general understanding of galaxy…”
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The nature of compact radio-loud AGN: a systematic look at the LOFAR AGN population
Published in Monthly notices of the Royal Astronomical Society (06-03-2024)“…ABSTRACT We investigate the nature of low-luminosity radio-loud active galactic nuclei (RLAGN) selected from the LOFAR Two-metre Sky Survey (LoTSS) first data…”
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Quantifying the cool ISM in radio AGNs: evidence for late-time retriggering by galaxy mergers and interactions
Published in Monthly notices of the Royal Astronomical Society (12-03-2022)“…ABSTRACT We use deep Herschel observations of the complete 2Jy sample of powerful radio active galactic nuclei (AGNs) in the local Universe (0.05 < z < 0.7) to…”
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8
Galaxy interactions are the dominant trigger for local type 2 quasars
Published 27-03-2023“…The triggering mechanism for the most luminous, quasar-like active galactic nuclei (AGN) remains a source of debate, with some studies favouring triggering via…”
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Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions
Published 16-02-2022“…We use deep Herschel observations of the complete 2Jy sample of powerful radio AGNs in the local universe (0.05 < z < 0.7) to probe their cool interstellar…”
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10
Warm molecular and ionized gas kinematics in the Type-2 quasar J0945+1737
Published 30-06-2022“…A&A 665, A55 (2022) We analyze Near-Infrared Integral Field Spectrograph (NIFS) observations of the type-2 quasar (QSO2) SDSS J094521.33+173753.2 to…”
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The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA
Published 15-03-2022“…A&A 658, A155 (2022) We present CO(2-1) and adjacent continuum observations of 7 nearby radio-quiet type-2 quasars (QSO2s) obtained with ALMA at ~0.2"…”
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Do AGN triggering mechanisms vary with radio power? II. The importance of mergers as a function of radio power and optical luminosity
Published 04-11-2021“…Investigation of the triggering mechanisms of radio AGN is important for improving our general understanding of galaxy evolution. In the first paper in this…”
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The LOFAR Two-Metre Sky Survey (LoTSS): VI. Optical identifications for the second data release
Published 31-08-2023“…A&A 678, A151 (2023) The second data release of the LOFAR Two-Metre Sky Survey (LoTSS) covers 27% of the northern sky, with a total area of $\sim 5,700$…”
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14
Accretion mode versus radio morphology in the LOFAR Deep Fields
Published 17-02-2022“…Radio-loud active galaxies have two accretion modes [radiatively inefficient (RI) and radiatively efficient (RE)], with distinct optical and infrared…”
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Journal Article -
15
The nature of compact radio-loud AGN: a systematic look at the LOFAR AGN population
Published 29-02-2024“…We investigate the nature of low-luminosity radio-loud active galactic nuclei (RLAGN) selected from the LOFAR Two-metre Sky Survey (LoTSS) first data release…”
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