We study the carbon monoxide (CO) excitation, mean molecular gas density, and interstellar radiation field (ISRF) intensity in a comprehensive sample of 76...
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PublicationCO Excitation, Molecular Gas Density, and Interstellar Radiation Field in Local and High-redshift Galaxies
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PublicationCO in the ALMA Radio-source Catalogue (ARC): The molecular gas content of radio galaxies as a function of redshift
To evaluate the role of radio activity in galaxy evolution, we designed a large archival CO survey of radio galaxies (RGs) to determine their molecular gas...
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PublicationCO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
Context. Voids are the most under-dense large-scale regions in the Universe. Galaxies inhabiting voids are one of the keys for understanding the intrinsic...
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PublicationCO-CAVITY pilot survey: Molecular gas and star formation in void galaxies (Corrigendum)
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PublicationCoherent star formation in spiral galaxies.
A sample of spiral galaxies is examined, applying moments analysis to their broad-band azimuthal profiles, in order to search for evidence of coherent large...
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PublicationCoincidence between morphology and star formation activity through cosmic time: the impact of the bulge growth
The origin of the quenching in galaxies is still highly debated. Different scenarios and processes are proposed. We use multiband (400-1600 nm) bulge-disc...
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PublicationCold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey
We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore...
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PublicationColors and color gradients in bulges of galaxies
We have obtained surface photometry in U, B, R, and I for a complete optically selected sample of 45 early-type spiral galaxies, to investigate the colors and...
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PublicationColour and infall time distributions of satellite galaxies in simulated Milky-Way analogues
We use the Auriga simulations to probe different satellite quenching mechanisms operating at different mass scales ($10^5 \, \mathrm{M}_\odot \lesssim M_\star...