activity
19942026
most citedExtending the Butcher--Oemler effect up to z~0.7

35 citations · 222 across the 25 of their papers we have counts for

collaborators

26 papers

astro-ph.CO2026

S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known clusters and groups in DR5 and a pilot study of Abell 4038

C. Mendes de Oliveira, N. M. Cardoso, P. A. A. Lopes +26

Within the framework of the Southern Photometric Local Universe Survey (S-PLUS), we introduce -PLUS lusters nd arge-scale nvironments (…

astro-ph.GA2022★ 6 cited

An investigation of the star-forming main sequence considering the nebular continuum emission at low-z

Henrique Miranda, Ciro Pappalardo, Polychronis Papaderos +7

The code FADO is the first publicly available population spectral synthesis tool that treats the contribution from ionised gas to the observed emission self-consistently. We study…

astro-ph.CO2022★ 4 cited

Ram pressure stripping in the z~0.5 galaxy cluster MS 0451.6-0305

Florence Durret, Lucie Degott, Catarina. Lobo +3

The pressure exerted by the ambient hot X-ray gas on cluster galaxies can lead to the presence of ram pressure stripped (RPS) galaxies, characterized by asymmetric shapes, and, in…

astro-ph.GA2021★ 35 cited

Jellyfish galaxy candidates in MACS J0717.5+3745 and thirty-nine other clusters of the DAFT/FADA and CLASH surveys

Florence Durret, Simon Chiche, Catarina Lobo +1

Galaxies in clusters undergo several phenomena such as ram pressure stripping and tidal interactions, that can trigger or quench their star formation and, in some cases, lead to ga…

astro-ph.GA2019★ 11 cited

Structural analysis of massive galaxies using HST deep imaging at z < 0.5

Sandra N. dos Reis, Fernando Buitrago, Polychronis Papaderos +11

Taking advantage of HST CANDELS data, we analyze the lowest redshift (z<0.5) massive galaxies in order to disentangle their structural constituents and study possible faint non-axi…

astro-ph.GA2015★ 13 cited

Red galaxies with pseudo-bulges in the SDSS: closer to disk galaxies or to classical bulges?

B. Ribeiro, C. Lobo, S. Antón +2

Pseudo-bulges are expected to markedly differ from classical, quasi-monolithically forming bulges in their star formation history (SFH) and chemical abundance patterns. To test thi…