Search Results - "BALDI, R"
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A population of galaxy-scale jets discovered using LOFAR
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT The effects of feedback from high luminosity radio-loud active galactic nuclei (AGN) have been extensively discussed in the literature, but feedback…”
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X-ray study of a sample of FR0 radio galaxies: unveiling the nature of the central engine
Published in Monthly notices of the Royal Astronomical Society (01-06-2018)Get full text
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The radio loudness of SDSS quasars from the LOFAR Two-metre Sky Survey: ubiquitous jet activity and constraints on star formation
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT We examine the distribution of radio emission from ∼42 000 quasars from the Sloan Digital Sky Survey, as measured in the LOFAR Two-metre Sky Survey…”
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The PG-RQS survey. Building the radio spectral distribution of radio-quiet quasars. I. The 45-GHz data
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT The origin of the radio emission in radio-quiet quasars (RQQs) remains unclear. Radio emission may be produced by a scaled-down version of the…”
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On the multiwavelength variability of Mrk 110: two components acting at different time-scales
Published in Monthly notices of the Royal Astronomical Society (01-07-2021)“…ABSTRACT We present the first intensive continuum reverberation mapping study of the high accretion-rate Seyfert galaxy Mrk 110. The source was monitored…”
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X-ray/UV/optical variability of NGC 4593 with Swift: reprocessing of X-rays by an extended reprocessor
Published in Monthly notices of the Royal Astronomical Society (01-11-2018)Get full text
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The host galaxy of the γ-ray-emitting narrow-line Seyfert 1 galaxy PKS 1502+036
Published in Monthly notices of the Royal Astronomical Society. Letters (01-07-2018)“…The detection of γ-ray emission from narrow-line Seyfert 1 galaxies (NLSy1) has challenged the idea that large black hole (BH) masses (≥108 M⊙) are needed to…”
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Hard-X-ray-selected active galactic nuclei – I. A radio view at high frequencies
Published in Monthly notices of the Royal Astronomical Society (11-07-2020)“…ABSTRACT A thorough study of radio emission in active galactic nuclei (AGNs) is of fundamental importance to understand the physical mechanisms responsible for…”
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Investigating the spectra and physical nature of galaxy scale jets
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT Previous studies have shown that physically small, low-luminosity radio galaxies, which we refer to as galaxy scale jets (GSJ), could potentially have…”
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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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The Multiwavelength Environment of Second Bologna Catalog Sources
Published in The Astrophysical journal. Supplement series (01-09-2023)“…We present the first results of the Chandra Cool Targets (CCT) survey of the Second Bologna Catalog (B2CAT) of powerful radio sources, aimed at investigating…”
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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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Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc
Published in Monthly notices of the Royal Astronomical Society (11-05-2020)“…ABSTRACT To answer major questions on supermassive black hole (SMBH) and galaxy evolution, a complete census of SMBH growth, i.e. active galactic nuclei (AGN),…”
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The new class of FR 0 radio galaxies
Published in Astronomische Nachrichten (01-02-2016)“…Are the FRI and FRII radio galaxies representative of the radio‐loud (RL) AGN population in the local Universe? Recent studies on the local low‐luminosity…”
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LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies through the [O iii] – radio connection
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT What determines the nuclear radio emission in local galaxies? To address this question, we combine optical [O iii] line emission, robust black hole…”
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Hard X-ray selected giant radio galaxies – III. The LOFAR view
Published in Monthly notices of the Royal Astronomical Society (01-06-2021)“…ABSTRACT Giant radio galaxies (GRGs), with extended structures reaching hundreds of kpc, are among the most spectacular examples of ejection of relativistic…”
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Radio jets in NGC 4151: where eMERLIN meets HST
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…Abstract We present high-sensitivity eMERLIN radio images of the Seyfert galaxy NGC 4151 at 1.51 GHz. We compare the new eMERLIN images to those from archival…”
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LeMMINGs – IV. The X-ray properties of a statistically complete sample of the nuclei in active and inactive galaxies from the Palomar sample
Published in Monthly notices of the Royal Astronomical Society (01-03-2022)“…ABSTRACT All 280 of the statistically complete Palomar sample of nearby (<120 Mpc) galaxies δ > 20° have been observed at 1.5 GHz as part of the LeMMINGs…”
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LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
Published in Monthly notices of the Royal Astronomical Society (02-05-2023)“…ABSTRACT Multiwavelength studies indicate that nuclear activity and bulge properties are closely related, but the details remain unclear. To study this…”
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LeMMINGs. Multiwavelength constraints on the co-existence of nuclear star clusters and AGN in nucleated galaxies
Published in Monthly notices of the Royal Astronomical Society (06-08-2024)“…ABSTRACT The relation between nuclear star clusters (NSCs) and the growth of the central supermassive black holes (SMBHs), as well as their connection to the…”
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