Search Results - "Feltre, A."
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Nuclear activity versus star formation: emission-line diagnostics at ultraviolet and optical wavelengths
Published in Monthly notices of the Royal Astronomical Society (01-03-2016)“…In the context of observations of the rest-frame ultraviolet and optical emission from distant galaxies, we explore the emission-line properties of…”
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Smooth and clumpy dust distributions in AGN: a direct comparison of two commonly explored infrared emission models
Published in Monthly notices of the Royal Astronomical Society (11-10-2012)“…Abstract The geometry of dust distribution within the inner regions of active galactic nuclei (AGN) is still a debated issue and relates directly to the AGN…”
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Constraints on the production and escape of ionizing radiation from the emission-line spectra of metal-poor star-forming galaxies
Published in Monthly notices of the Royal Astronomical Society (21-11-2019)“…ABSTRACT We explore the production and escape of ionizing photons in young galaxies by investigating the ultraviolet and optical emission-line properties of…”
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Chemical abundances in Seyfert galaxies – V. The discovery of shocked emission outside the AGN ionization axis
Published in Monthly notices of the Royal Astronomical Society. Letters (01-02-2021)“…ABSTRACT We present maps for the electron temperature in the inner kpc of three luminous Seyfert galaxies: Mrk 79, Mrk 348, and Mrk 607 obtained from Gemini…”
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beagle-agn I: simultaneous constraints on the properties of gas in star-forming and AGN narrow-line regions in galaxies
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT We present the addition of nebular emission from the narrow-line regions (NLR) surrounding active galactic nuclei (AGNs) to beagle (BayEsian Analysis…”
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Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel
Published in Monthly notices of the Royal Astronomical Society (11-04-2014)“…We study a sample of Herschel selected galaxies within the Great Observatories Origins Deep Survey-South and the Cosmic Evolution Survey fields in the…”
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Extreme star formation events in quasar hosts over 0.5 < z < 4
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)“…We explore the relationship between active galactic nuclei (AGN) and star formation in a sample of 513 optically luminous type 1 quasars up to redshifts of ∼4…”
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Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT For the first time, the sulphur abundance relative to hydrogen (S/H) in the narrow-line regions of a sample of Seyfert 2 nuclei (Sy 2s) has been…”
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Compton-thick AGN in the NuSTAR Era. VIII. A joint NuSTAR–XMM-Newton Monitoring of the Changing-look Compton-thick AGN NGC 1358
Published in The Astrophysical journal (01-08-2022)“…Abstract We present the multi-epoch monitoring with NuSTAR and XMM-Newton of NGC 1358, a nearby Seyfert 2 galaxy whose properties made it a promising candidate…”
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Differential attenuation in star-forming galaxies at 0.3 ≲ z ≲ 1.5 in the SHARDS/CANDELS field
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT We use a sample of 706 galaxies, selected as [O ii]λ3727 ([O ii]) emitters in the Survey for High-z Absorption Red and Dead Sources (SHARDS) on the…”
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The roles of star formation and AGN activity of IRS sources in the HerMES fields
Published in Monthly notices of the Royal Astronomical Society (21-09-2013)“…In this work, we explore the impact of the presence of an active galactic nucleus (AGN) on the mid- and far-infrared (IR) properties of galaxies as well as the…”
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The HerMES submillimetre local and low-redshift luminosity functions
Published in Monthly notices of the Royal Astronomical Society (21-02-2016)“…We used wide-area surveys over 39 deg2 by the HerMES (Herschel Multi-tiered Extragalactic Survey) collaboration, performed with the Herschel Observatory SPIRE…”
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The AGN content in luminous infrared galaxies at z∼ 2 from a global SED analysis including Herschel data
Published in Monthly notices of the Royal Astronomical Society (01-06-2012)“…We use Herschel-PACS far-infrared (IR) data, combined with previous multiband information and mid-IR spectra, to properly account for the presence of an active…”
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On the nature of the absorber in IRAS 09104+4109: the X-ray and mid-infrared view
Published in Monthly notices of the Royal Astronomical Society (01-09-2011)“…We present a long (≈76 ks) Chandra observation of IRAS 09104+4109, a hyperluminous galaxy, optically classified as a type 2 active galactic nuclei (AGN) hosted…”
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On the nature of the absorber in IRAS09104+4109: the X-ray and mid-infrared view
Published in Monthly notices of the Royal Astronomical Society (21-09-2011)“…ABSTRACT We present a long ([asymptotically =]76ks) Chandra observation of IRAS09104+4109, a hyperluminous galaxy, optically classified as a type 2 active…”
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A COMPLETE CENSUS OF SILICATE FEATURES IN THE MID-INFRARED SPECTRA OF ACTIVE GALAXIES
Published in The Astrophysical journal (20-04-2015)“…ABSTRACT We present a comprehensive study of the silicate features at 9.7 and 18 m of a sample of almost 800 active galactic nuclei (AGNs) with available…”
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The Herschel ⋆ Multi-tiered Extragalactic Survey: HerMES
Published in Monthly notices of the Royal Astronomical Society (11-08-2012)“…Abstract The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling ∼380 deg2. Fields range…”
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Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
Published in Monthly notices of the Royal Astronomical Society (02-03-2023)“…ABSTRACT For the first time, the sulphur abundance relative to hydrogen (S/H) in the narrow-line regions of a sample of Seyfert 2 nuclei (Sy 2s) has been…”
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A COMPLETE CENSUS OF SILICATE FEATURES IN THE MOD-INFRARED SPECTRA OF ACTIVE GALAXIES
Published in The Astrophysical journal (01-04-2015)“…We present a comprehensive study of the silicate features at 9.7 and 18 [mu]m of a sample of almost 800 active galactic nuclei (AGNs) with available spectra…”
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