Search Results - "POPESSO, Paola"

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    A new empirical method to estimate the molecular gas mass in galaxies by Concas, Alice, Popesso, Paola

    “…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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    Journal Article
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    The baryon census and the mass-density of stars, neutral gas, and hot gas as a function of halo mass by Dev, Ajay, Driver, Simon P, Meyer, Martin, Robotham, Aaron, Obreschkow, Danail, Popesso, Paola, Comparat, Johan

    “…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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    GOODS- HERSCHEL : SEPARATING HIGH-REDSHIFT ACTIVE GALACTIC NUCLEI AND STAR-FORMING GALAXIES USING INFRARED COLOR DIAGNOSTICS by Kirkpatrick, Allison, Pope, Alexandra, Charmandaris, Vassilis, Daddi, Emmanuele, Elbaz, David, Hwang, Ho Seong, Pannella, Maurilio, Scott, Douglas, Altieri, Bruno, Aussel, Herve

    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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    PHOTOMETRIC REDSHIFTS OF SUBMILLIMETER GALAXIES by Chakrabarti, Sukanya, Magnelli, Benjamin, McKee, Christopher F, Lutz, Dieter, Berta, Stefano, POPESSO, PAOLA, Pozzi, Francesca

    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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    A new empirical method to estimate the molecular gas mass in galaxies by Concas, Alice, Popesso, Paola

    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…”
    Get full text
    Journal Article
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    The baryon census and the mass-density of stars, neutral gas, and hot gas as a function of halo mass by Dev, Ajay, Driver, Simon P, Meyer, Martin, Robotham, Aaron, Obreschkow, Danail, Popesso, Paola, Comparat, Johan

    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…”
    Get full text
    Journal Article
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    Quantifying Observational Projection Effects with a Simulation-based hot CGM model by Shreeram, Soumya, Comparat, Johan, Merloni, Andrea, Zhang, Yi, Ponti, Gabriele, Nandra, Kirpal, ZuHone, John, Marini, Ilaria, Vladutescu-Zopp, Stephan, Popesso, Paola, Pakmor, Ruediger, Seppi, Riccardo, Peroux, Celine, Sorini, Daniele

    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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    A census of radio-selected AGN on the COSMOS field and of their FIR properties by Magliocchetti, Manuela, Popesso, Paola, Brusa, Marcella, Salvato, Mara

    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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    Spatial distribution of stellar mass and star formation activity at 0.2<z<1.2 across and along the Main Sequence by Morselli, Laura, Popesso, Paola, Cibinel, Anna, Oesch, Pascal A, Montes, Mireia, Atek, Hakim, Illingworth, Garth D, Holden, Bradford

    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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    The PEP Survey: evidence for intense star-forming activity in the majority of radio-selected AGN at z>~1 by Magliocchetti, Manuela, Lutz, Dieter, Santini, Paola, Salvato, Mara, Popesso, Paola, Berta, Stefano, Pozzi, Francesca

    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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