Search Results - "POPESSO, Paola"
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GOODS-HERSCHEL: IMPACT OF ACTIVE GALACTIC NUCLEI AND STAR FORMATION ACTIVITY ON INFRARED SPECTRAL ENERGY DISTRIBUTIONS AT HIGH REDSHIFT
Published in The Astrophysical journal (10-11-2012)“…We explore the effects of active galactic nuclei (AGNs) and star formation activity on the infrared (0.3-1000 mu m) spectral energy distributions (SEDs) of…”
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A new empirical method to estimate the molecular gas mass in galaxies
Published in Monthly notices of the Royal Astronomical Society. Letters (01-06-2019)“…ABSTRACT We find a tight correlation between the dust extinction, traced by the Balmer Decrement (BD = H α/H β), the CO(1-0) line luminosity (LCO), and total…”
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The baryon census and the mass-density of stars, neutral gas, and hot gas as a function of halo mass
Published in Monthly notices of the Royal Astronomical Society (15-11-2024)“…ABSTRACT We study the stellar, neutral gas content within haloes over a halo mass range $10^{10} \text{ to } 10^{15.5} \text{M}_\odot$ and hot X-ray gas…”
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Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
Published in The Astrophysical journal (01-12-2011)“…We analyze the dependence of galaxy structure (size and Sersic index) and mode of star formation ( Delta *SSFR and SFRIR/SFRUV) on the position of galaxies in…”
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On Star Formation Rates and Star Formation Histories of Galaxies Out to z ~ 3
Published in The Astrophysical journal (01-09-2011)“…We compare multi-wavelength star formation rate (SFR) indicators out to z ~ 3 in the GOODS-South field. Our analysis uniquely combines U to 8 Delta *mm…”
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GOODS-HERSCHEL AND CANDELS: THE MORPHOLOGIES OF ULTRALUMINOUS INFRARED GALAXIES AT z ∼ 2
Published in The Astrophysical journal (20-09-2012)“…Using deep 100 and 160 [mu]m observations in GOODS-South from GOODS-Herschel, combined with high-resolution HST/WFC3 near-infrared imaging from CANDELS, we…”
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GOODS- HERSCHEL : SEPARATING HIGH-REDSHIFT ACTIVE GALACTIC NUCLEI AND STAR-FORMING GALAXIES USING INFRARED COLOR DIAGNOSTICS
Published in The Astrophysical journal (01-02-2013)“…We have compiled a large sample of 151 high-redshift (z = 0.5-4) galaxies selected at 24 mu m (S sub(24) > 100 mu Jy) in the GOODS-N and ECDFS fields for which…”
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EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION IN z ∼ 2 DUSTY GALAXIES FROM THE GOODS-HERSCHEL SURVEY
Published in The Astrophysical journal (01-11-2012)“…Dusty galaxies at z ~ 2 span a wide range of relative brightness between rest-frame mid-infrared (8 [mu]m) and ultraviolet wavelengths. We attempt to determine…”
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PHOTOMETRIC REDSHIFTS OF SUBMILLIMETER GALAXIES
Published in The Astrophysical journal (20-08-2013)“…We use the photometric redshift method of Chakrabarti & McKee to infer photometric redshifts of submillimeter galaxies with far-IR (FIR) Herschel data obtained…”
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EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION IN z similar to 2 DUSTY GALAXIES FROM THE GOODS-HERSCHEL SURVEY
Published in The Astrophysical journal (01-11-2012)“…Dusty galaxies at z similar to 2 span a wide range of relative brightness between rest-frame mid-infrared (8 mu m) and ultraviolet wavelengths. We attempt to…”
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A new empirical method to estimate the molecular gas mass in galaxies
Published 06-05-2019“…We find a tight correlation between the dust extinction, traced by the Balmer Decrement (BD$=$H$\alpha$/H$\beta$), the CO(1-0) line luminosity (L$_{CO}$) and…”
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The baryon census and the mass-density of stars, neutral gas, and hot gas as a function of halo mass
Published 01-11-2024“…We study the stellar, neutral gas content within halos over a halo mass range $10^{10} \text{ to } 10^{15.5} \text{M}_\odot$ and hot X-ray gas content over a…”
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Quantifying Observational Projection Effects with a Simulation-based hot CGM model
Published 16-09-2024“…The hot phase of the circumgalactic medium (CGM) allows us to probe the inflow and outflow of gas within a galaxy, which is responsible for dictating the…”
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The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
Published 18-08-2024“…A&A 690, A268 (2024) Understanding how the properties of galaxies relate to the properties of the hot circum-galactic medium (CGM) around them can constrain…”
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The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
Published 18-08-2024“…A&A 690, A267 (2024) The circumgalactic medium (CGM) provides the material needed for galaxy formation and influences galaxy evolution. The hot ($T>10^6K$) CGM…”
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A census of radio-selected AGN on the COSMOS field and of their FIR properties
Published 21-09-2017“…We use the new catalogue by Laigle et al. (2016) to provide a full census of VLA-COSMOS radio sources. We identify 90% of such sources and sub-divide them into…”
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The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3
Published 13-01-2022“…A&A 666, A156 (2022) We aim at characterizing the hot phase of the Circum-Galactic Medium in a large sample of galaxies. We stack X-ray events from the…”
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Spatial distribution of stellar mass and star formation activity at 0.2<z<1.2 across and along the Main Sequence
Published 20-12-2018“…A&A 626, A61 (2019) High-resolution multi-wavelength photometry is crucial to explore the spatial distribution of star formation in galaxies and understand how…”
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A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
Published 24-06-2020“…In the second work of this series, we analyse the connection between the availability of gas and the position of a region with respect to the spatially…”
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The PEP Survey: evidence for intense star-forming activity in the majority of radio-selected AGN at z>~1
Published 10-11-2015“…In order to investigate the FIR properties of radio-active AGN, we have considered three different fields where both radio and FIR observations are the deepest…”
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