Search Results - "GARGIULO, A."
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The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3
Published in Monthly notices of the Royal Astronomical Society (21-11-2019)“…ABSTRACT We present a Bayesian full-spectral-fitting analysis of 75 massive ($M_* \gt 10^{10.3} \, \mathrm{M_\odot }$) UVJ-selected galaxies at redshifts of…”
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Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
Published in Monthly notices of the Royal Astronomical Society (21-07-2020)“…ABSTRACT We present a sample of 151 massive (M* > 1010 M⊙) quiescent galaxies at 2 < z < 5, based on a sophisticated Bayesian spectral energy distribution…”
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The VANDELS ESO public spectroscopic survey
Published in Monthly notices of the Royal Astronomical Society (01-09-2018)Get full text
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On the central stellar mass density and the inside-out growth of early-type galaxies
Published in Monthly notices of the Royal Astronomical Society (01-06-2012)“…Recent theoretical and observational studies on the assembly of early-type galaxies (ETGs) point towards an inside-out growth of their stellar mass…”
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Constraining the star formation and the assembly histories of normal and compact early-type galaxies at 1 < z < 2
Published in Monthly notices of the Royal Astronomical Society (01-04-2011)“…We present a study based on a sample of 62 early-type galaxies (ETGs) at 0.9 < z spec < 2 aimed at constraining their past star formation and mass assembly…”
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The Fundamental Plane of cluster spheroidal galaxies at z ∼ 1.3: evidence for mass-dependent evolution
Published in Monthly notices of the Royal Astronomical Society (11-01-2020)“…ABSTRACT We present spectroscopic observations obtained at the Large Binocular Telescope in the field of the cluster XLSSJ0223−0436 at z = 1.22. We confirm 12…”
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A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass, and age from z = 0.6 to z = 1.3
Published in Monthly notices of the Royal Astronomical Society (21-03-2022)“…ABSTRACT We study the relationships between stellar mass, size, and age within the quiescent population, using two mass-complete spectroscopic samples with…”
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sipgi: an interactive pipeline for spectroscopic data reduction
Published in Monthly notices of the Royal Astronomical Society (22-06-2022)“…ABSTRACT We present sipgi, a spectroscopic pipeline to reduce optical/near-infrared data from slit-based spectrographs. sipgi is a complete spectroscopic data…”
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The number density of superdense early-type galaxies at 1 < z < 2 and the local cluster galaxies
Published in Monthly notices of the Royal Astronomical Society. Letters (01-10-2010)“…Many of the early-type galaxies (ETGs) observed so far at z > 1 turned out to have smaller radii with respect to that of a typical present day ETG with…”
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The Smallest Scale of Hierarchy Survey (SSH) – II. Extended star formation and bar-like features in the dwarf galaxy NGC 3741: recent merger or ongoing gas accretion?
Published in Monthly notices of the Royal Astronomical Society (23-03-2022)“…ABSTRACT Using Large Binocular Telescope deep imaging data from the Smallest Scale of Hierarchy Survey (SSH) and archival Hubble Space Telescope data, we…”
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The space density of z > 4 blazars
Published in Monthly notices of the Royal Astronomical Society (21-03-2019)Get full text
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Age, metallicity, and star formation history of spheroidal galaxies in cluster at z ∼ 1.2
Published in Monthly notices of the Royal Astronomical Society (01-04-2019)Get full text
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The fraction of ionizing radiation from massive stars that escapes to the intergalactic medium
Published in Monthly notices of the Royal Astronomical Society (11-03-2019)“…Whether stars could have driven the reionization of the intergalactic medium depends critically on the proportion of ionizing radiation that escapes the…”
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The role of galaxy mass on AGN emission: a view from the VANDELS survey
Published in Monthly notices of the Royal Astronomical Society (01-04-2020)“…ABSTRACT We present a comparative analysis of the properties of active galactic nuclei (AGNs) emitting at radio and X-ray wavelengths. The study is performed…”
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End-colostomy parastomal hernia repair: a systematic review on laparoscopic and robotic approaches
Published in Hernia : the journal of hernias and abdominal wall surgery (01-06-2024)“…Introduction Parastomal hernia (PSH) is the most common and challenging complication after stoma creation, with an estimated 50% incidence 2 years after the…”
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Spectral detection of multiple stellar populations in z ∼ 1 early-type galaxies
Published in Monthly notices of the Royal Astronomical Society (01-11-2014)“…We present a spectroscopic analysis based on measurements of two mainly age-dependent spectrophotometric indices in the 4000 A rest-frame region, i.e. H+K(Ca…”
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Old age and supersolar metallicity in a massive z ∼ 1.4 early-type galaxy from VLT/X-Shooter spectroscopy
Published in Monthly notices of the Royal Astronomical Society (21-12-2015)“…We present the first estimate of age, stellar metallicity and chemical abundance ratios, for an individual early-type galaxy at high-redshift (z = 1.426) in…”
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Clinical Heterogeneity in ME/CFS. A Way to Understand Long-COVID19 Fatigue
Published in Frontiers in psychiatry (11-10-2021)“…The aim of present paper is to identify clinical phenotypes in a cohort of patients affected of Myalgic Encephalomyelitis/Chronic Fatigue Syndrome. Ninety-one…”
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The VANDELS Survey: new constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT We use VANDELS spectroscopic data overlapping with the ≃7 Ms Chandra Deep Field South survey to extend studies of high-mass X-ray binary systems…”
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IMPROVEMENT OF THE TECHNIQUES FOR THE COMPUTATION OF EVAPOTRANSPIRATION MAPS
Published in International archives of the photogrammetry, remote sensing and spatial information sciences. (30-05-2022)“…The definition of a methodology for estimating suitable areas for new renewable sources needs to identify possible indexes that describe the fields. One…”
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