activity
20162025
most citedThe role of quenching time in the evolution of the mass-size relation of passive galaxies from the WISP survey

16 citations · 52 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

Ram-pressure stripping caught in action in a young cluster at

Ke Xu, Tao Wang, Emanuele Daddi +16

Galaxy clusters in the local Universe are dominated by massive quiescent galaxies with old ages, formed at high redshifts. Whether their quenching is driven by internal processes o…

astro-ph.GA2025★ 1 cited

The Parallel Ionizing Emissivity Survey (PIE). I. Survey design and selection of candidate Lyman Continuum leakers at 3.1<z<3.5

Alexander Beckett, Marc Rafelski, Claudia Scarlata +18

We present the survey design and initial results from the Parallel Ionizing Emissivity (PIE) survey. PIE is a large HST survey designed to detect Lyman continuum (LyC) emitting gal…

astro-ph.GA2025★ 3 cited

Clump formation in ram-pressure stripped galaxies: evidence from mass function

Eric Giunchi, Claudia Scarlata, Ariel Werle +8

The mass function (MF) of young ( Myr) stellar clumps is an indicator of the mechanism driving the collapse of the interstellar medium (ISM) into giant mo…

astro-ph.GA2023

The history of star-forming regions in the tails of 6 GASP jellyfish galaxies observed with the Hubble Space Telescope

A. Werle, E. Giunchi, B. Poggianti +12

Using images collected with the WFC3 camera on board of the Hubble Space Telescope, we detect stellar clumps in continuum-subtracted and ultraviolet (F275W filter), such clump…

astro-ph.GA2023

Morphology of star-forming clumps in ram-pressure stripped galaxies as seen by HST

Giunchi, E, Poggianti +18

We characterize the morphological properties of a statistically relevant sample of H and UV young star-forming clumps and optical complexes, observed with the \textit{Hubble Spa…

astro-ph.GA2016★ 16 cited

The role of quenching time in the evolution of the mass-size relation of passive galaxies from the WISP survey

A. Zanella, C. Scarlata, E. M. Corsini +13

We analyze how passive galaxies at z 1.5 populate the mass-size plane as a function of their stellar age, to understand if the observed size growth with time can be explaine…