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20092026
most citedGASP I: Gas stripping phenomena in galaxies with MUSE

346 citations · 11.1k across the 299 of their papers we have counts for

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Showing 2014Show all

8 papers · 1 filter

astro-ph.GA2014★ 39 cited

Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories

Louis E. Abramson, Michael D. Gladders, Alan Dressler +3

We show that a model consisting of individual, log-normal star formation histories for a volume-limited sample of galaxies reproduces the evolution of the total and qui…

astro-ph.GA2014★ 23 cited

Understanding the Unique Assembly History of Central Group Galaxies

Benedetta Vulcani, Kevin Bundy, Claire Lackner +7

Central Galaxies (CGs) in massive halos live in unique environments with formation histories closely linked to that of the host halo. In local clusters they have larger sizes ($R_e…

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…

astro-ph.GA2014★ 27 cited

What do simulations predict for the galaxy stellar mass function and its evolution in different environments?

B. Vulcani, G. De Lucia, B. M. Poggianti +3

We present a comparison between the observed galaxy stellar mass function and the one predicted from the De Lucia & Blaizot (2007) semi-analytic model applied to the Millennium Sim…

astro-ph.GA2014★ 84 cited

WINGS Data Release: a database of galaxies in nearby clusters

A. Moretti, B. M. Poggianti, G. Fasano +15

[Abridged] To effectively investigate galaxy formation and evolution, it is of paramount importance to exploit homogeneous data for large samples of galaxies in different environme…

astro-ph.GA2014★ 119 cited

The Mass-Independence of Specific Star Formation Rates in Galactic Disks

Louis E. Abramson, Daniel D. Kelson, Alan Dressler +4

The slope of the star formation rate/stellar mass relation (the SFR "Main Sequence"; ) is not quite unity: specific star formation rates are weakly…