activity
20182026
most citedThe Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

205 citations · 860 across the 37 of their papers we have counts for

collaborators

38 papers

astro-ph.GA2026

Fishing for Jellyfish Galaxies: Exploring ram-pressure stripping with crowd science

C. Bellhouse, Y. L. Jaffé, J. P. Crossett +13

Aims: We present the first results of Fishing for Jellyfish Galaxies, a pilot citizen-science project using Zooniverse to identify galaxies undergoing ram-pressure stripping (RPS).…

astro-ph.GA2025

Investigating the clumpy star formation in an interacting dwarf irregular galaxy

Augusto E. Lassen, Ana L. Chies-Santos, Rogerio Riffel +9

Clumpy morphologies are more frequent in distant and low-mass star-forming galaxies. Therefore the less numerous nearby galaxies presenting kpc-sized clumps represent unique labora…

astro-ph.GA2025★ 1 cited

What goes around comes around: the fate of stars in stripped tails of gas

Nina Akerman, Stephanie Tonnesen, Bianca M. Poggianti +5

We conduct high-resolution wind-tunnel simulations to study in-situ star formation in the stripped tails of two massive () galaxies undergoing time-ev…

astro-ph.GA2025

Stripped and Enriched: The Role of Ram-Pressure in Shaping Chemical Enrichment of Galaxies at Intermediate Redshift

Amir H. Khoram, Bianca Poggianti, Alessia Moretti +11

The chemical evolution of galaxies is shaped by their star formation histories and the exchange of gas with their environments. Metallicity provides key insights into these process…

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.GA2024

Spatially resolved comparison of SFRs from UV and H in GASP gas-stripped galaxies

Neven Tomicic, Ariel Werle, Benedetta Vulcani +6

Star-formation rates (SFR) in galaxies offer a view of various physical processes across them and are measured using various tracers, such as H and UV. Different physical mechan…