activity
20142022
most citedThe Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

205 citations · 822 across the 22 of their papers we have counts for

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21 papers · 1 filter

astro-ph.GA2022★ 49 cited

Systematically Measuring Ultra-Diffuse Galaxies (SMUDGes). III. The Southern SMUDGes Catalog

Dennis Zaritsky, Richard Donnerstein, Ananthan Karunakaran +5

We present a catalog of 5598 ultra-diffuse galaxy (UDG) candidates with effective radius arcsec distributed throughout the southern portion of the DESI Legacy Imaging S…

astro-ph.GA2021

A new method to detect globular clusters with the S-PLUS survey

Maria Luísa Buzzo, Arianna Cortesi, Duncan A. Forbes +17

In this paper, we describe a new method to select globular cluster (GC) candidates, including galaxy subtraction with unsharp masking, template fitting techniques and the inclusion…

astro-ph.GA2021★ 18 cited

Canis Major OB1 stellar groups contents revealed by Gaia

T. Santos-Silva, H. D. Perottoni, F. Almeida-Fernandes +15

Canis Major OB1 (CMa OB1) is a Galactic stellar association with a very intriguing star-formation scenario. There are more than two dozen known star clusters in its line of sight,…

astro-ph.GA2021★ 43 cited

On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2

L. Nakazono, C. Mendes de Oliveira, N. S. T. Hirata +25

This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that…

astro-ph.GA2021

Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images

C. G. Escudero, A. V. Smith Castelli, F. R. Faifer +4

Galaxy clusters are the largest gravitationally bound systems in the Universe and, as such, play an important role in cosmological studies. An important resource for studying their…

astro-ph.GA2021

The Fornax Cluster through S-PLUS

A. V. Smith Castelli, C. Mendes de Oliveira, F. Herpich +25

The Southern Photometric Local Universe Survey (S-PLUS) aims to map 9300 deg of the Southern sky using the Javalambre filter system of 12 optical bands, 5 Sloan-like…

astro-ph.GA2021★ 49 cited

The Photometric Metallicity and Carbon Distributions of the Milky Way's Halo and Solar Neighborhood from S-PLUS Observations of SDSS Stripe 82

Devin D. Whitten, Vinicius M. Placco, Timothy C. Beers +14

We report photometric estimates of effective temperature, , metallicity, [Fe/H], carbonicity, [C/Fe], and absolute carbon abundances, , for over 700,000 st…

astro-ph.GA2021★ 15 cited

Recovering the origins of the lenticular galaxy NGC 3115 using multi-band imaging

Maria Luisa Buzzo, Arianna Cortesi, Jose A. Hernandez-Jimenez +16

A detailed study of the morphology of lenticular galaxies is an important way to understand how this type of galaxy formed and evolves over time. Decomposing a galaxy into its comp…

astro-ph.GA2021★ 8 cited

Physical and kinematic conditions of the local merging galaxy NGC 1487

M. L. Buzzo, B. Ziegler, P. Amram +6

We present optical VLT/MUSE integral field spectroscopy data of the merging galaxy NGC 1487. We use fitting techniques to study the ionized gas emission of this merger and its main…

astro-ph.GA2020★ 29 cited

A preserved high-z compact progenitor in the heart of NGC3311 revealed with MUSE 2D stellar population analysis

C. E. Barbosa, C. Spiniello, M. Arnaboldi +3

Massive early-type galaxies are believed to be the end result of an extended mass accretion history. The stars formed in situ very early on in the initial phase of the assembly mig…

astro-ph.GA2020★ 38 cited

An environmental dependence of the physical and structural properties in the Hydra Cluster galaxies

Ciria Lima-Dias, Antonela Monachesi, Sergio Torres-Flores +20

The nearby Hydra Cluster (50 Mpc) is an ideal laboratory to understand, in detail, the influence of the environment on the morphology and quenching of galaxies in dense envir…

astro-ph.GA2020★ 50 cited

One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field

C. E. Barbosa, D. Zaritsky, R. Donnerstein +19

We present the first systematic study of the stellar populations of ultra-diffuse galaxies (UDGs) in the field, integrating the large area search and characterization of UDGs by th…

astro-ph.GA2019★ 16 cited

The S-PLUS: a star/galaxy classification based on a Machine Learning approach

M. V. Costa-Duarte, L. Sampedro, A. Molino +32

We present a star/galaxy classification for the Southern Photometric Local Universe Survey (S-PLUS), based on a Machine Learning approach: the Random Forest algorithm. We train the…

astro-ph.GA2019★ 27 cited

Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case

A. Molino, M. V. Costa-Duarte, L. Sampedro +42

In this paper we present a thorough discussion about the photometric redshift (photo-z) performance of the Southern Photometric Local Universe Survey (S-PLUS). This survey combines…

astro-ph.GA2019★ 205 cited

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

C. Mendes de Oliveira, T. Ribeiro, W. Schoenell +142

The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-So…

astro-ph.GA2018★ 29 cited

The Hydra I cluster core - II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311

M. Hilker, T. Richtler, C. E. Barbosa +3

NGC 3311, the central galaxy of the Hydra I cluster, shows signatures of recent infall of satellite galaxies from the cluster environment. Previous work has shown that the line-of-…

astro-ph.GA2017★ 37 cited

Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311

Carlos E. Barbosa, Magda Arnaboldi, Lodovico Coccato +4

Early-type galaxies show a strong size evolution with redshift. This evolution is explained by fast "in-situ" star formation at high- followed by a late mass assembly mostly dri…

astro-ph.GA2016★ 25 cited

The Hydra I cluster core. I. Stellar populations in the cD galaxy NGC 3311

Carlos Eduardo Barbosa, Magda Arnaboldi, Lodovico Coccato +3

(Abridged for arXiv) The history of the mass assembly of brightest cluster galaxies may be studied by the mapping the stellar populations at large radial distances from the galaxy…

astro-ph.GA2015★ 14 cited

GHASP: an H kinematic survey of spiral galaxies - X. Surface photometry, decompositions and the Tully-Fisher relation in the Rc-band

C. E. Barbosa, C. Mendes de Oliveira, P. Amram +6

We present Rc-band surface photometry for 170 of the 203 galaxies in GHASP, Gassendi H-Alpha survey of SPirals, a sample of late-type galaxies for which high-resolution Fabry-Perot…

astro-ph.GA2014

A 3D view of the Hydra I cluster core - II. Stellar populations

Carlos Eduardo Barbosa, Magda Arnaboldi, Michael Hilker +3

Several observations of the central region of the Hydra I galaxy cluster point to a multi-epoch assembly history. Using our novel FORS2/VLT spectroscopic data set, we were able to…

astro-ph.GA2014★ 2 cited

A 3D view of the Hydra I galaxy cluster core - I. Kinematic substructures

Michael Hilker, Carlos Eduardo Barbosa, Tom Richtler +3

We used FORS2 in MXU mode to mimic a coarse 'IFU' in order to measure the 3D large-scale kinematics around the central Hydra I cluster galaxy NGC 3311. Our data show that the veloc…