activity
20142023
most citedGASP I: Gas stripping phenomena in galaxies with MUSE

346 citations · 1.2k across the 11 of their papers we have counts for

collaborators

12 papers

hep-ex2023

Technical Design Report for the LUXE Experiment

H. Abramowicz, M. Almanza Soto, M. Altarelli +131

This Technical Design Report presents a detailed description of all aspects of the LUXE (Laser Und XFEL Experiment), an experiment that will combine the high-quality and high-energ…

astro-ph.IM2021★ 68 cited

Fermi Large Area Telescope Performance After 10 Years Of Operation

The Fermi LAT Collaboration, M. Ajello, W. B. Atwood +126

The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope,…

astro-ph.GA2018★ 47 cited

The strong correlation between post-starburst fraction and environment

A. Paccagnella, B. Vulcani, B. M. Poggianti +4

We examine a magnitude limited (M_B< -18.7) sample of post-starburst (PSB) galaxies at 0.03<z<0.11 in the different environments from the spectroscopic data set of the Padova Mille…

astro-ph.CO2017★ 81 cited

The concentration-mass relation of clusters of galaxies from the OmegaWINGS survey

A. Biviano, A. Moretti, A. Paccagnella +8

The relation between a cosmological halo concentration and its mass (cMr) is a powerful tool to constrain cosmological models of halo formation and evolution. On the scale of galax…

astro-ph.GA2017★ 346 cited

GASP I: Gas stripping phenomena in galaxies with MUSE

Bianca M. Poggianti, Alessia Moretti, Marco Gullieuszik +15

GASP (GAs Stripping Phenomena in galaxies with MUSE) is a new integral-field spectroscopic survey with MUSE at the VLT aiming at studying gas removal processes in galaxies. We pres…

astro-ph.GA2017★ 56 cited

OmegaWINGS: The first complete census of post starburst galaxies in clusters in the local universe

A. Paccagnella, B. Vulcani, B. M. Poggianti +10

Galaxies that abruptly interrupt their star formation in < 1.5 Gyr present recognizable features in their spectra (no emission and Hd in absorption) and are called post starburst (…

astro-ph.GA2017★ 86 cited

OmegaWINGS: spectroscopy in the outskirts of local clusters of galaxies

A. Moretti, M. Gullieuszik, B. Poggianti +9

Studies of the properties of low-redshift cluster galaxies suffer, in general, from small spatial coverage of the cluster area. WINGS, the most homogeneous and complete study of ga…

astro-ph.GA2015★ 90 cited

Slow quenching of star formation in OMEGAWINGS clusters: galaxies in transition in the local universe

Angela Paccagnella, Benedetta Vulcani, Bianca Maria Poggianti +8

The star formation quenching depends on environment, but a full understanding of what mechanisms drive it is still missing. Exploiting a sample of galaxies with masses $M_\ast>10^{…

astro-ph.GA2015★ 176 cited

Jellyfish galaxy candidates at low redshift

B. M. Poggianti, G. Fasano, A. Omizzolo +9

Galaxies that are being stripped of their gas can sometimes be recognized from their optical appearance. Extreme examples of stripped galaxies are the so-called ``jellyfish galaxie…

astro-ph.GA2015★ 71 cited

The star formation history of galaxies: the role of galaxy mass, morphology and environment

Valentina Guglielmo, Bianca M. Poggianti, Alessia Moretti +5

We analyze the star formation history (SFH) of galaxies as a function of present-day environment, galaxy stellar mass and morphology. The SFH is derived by means of a non-parametri…

astro-ph.GA2015★ 96 cited

OmegaWINGS: OmegaCAM@VST observations of WINGS galaxy clusters

M. Gullieuszik, B. Poggianti, G. Fasano +13

The Wide-field Nearby Galaxy-cluster Survey (WINGS) is a wide-field multi-wavelength survey of X-ray selected clusters at z =0.04-0.07. The original 34'x34' WINGS field-of- view ha…

astro-ph.GA2014★ 63 cited

From blue star-forming to red passive: galaxies in transition in different environments

Benedetta Vulcani, Bianca M. Poggianti, Jacopo Fritz +4

Exploiting a mass complete (M_*>10^(10.25)M_sun) sample at 0.03<z<0.11 drawn from the Padova Millennium Galaxy Group Catalog (PM2GC), we use the (U-B)_rf color and morphologies to…