activity
20172026
most citedThe Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

205 citations · 807 across the 37 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

27 papers · 1 filter

astro-ph.GA2026

Evidence for the Typhon Stellar Stream as the Remnant of a Recently-disrupted Dwarf Galaxy

João V. Nogueira-Santos, Guilherme Limberg, Silvia Rossi +4

In the hierarchical model of galaxy formation, the Milky Way's stellar halo assembles through the successive accretion of dwarf galaxies. While many resulting substructures have be…

astro-ph.GA2026

The S-PLUS Fifth Data-Release: Over 4500 square degrees of the Southern Sky and a multicolor view of the Hydra and Antlia galaxy clusters

Erik Vinicius Rodrigues de Lima, Gustavo Bernhard Oliveira Schwarz, Fábio Rafael Herpich +55

We present the 5th data release (DR5) of the Southern Photometric Local Universe Survey (S-PLUS), covering 4592 square degrees across 2491 fields. Observations were conducted with…

astro-ph.GA2026

The Low- Splash Population in the Milky Way

Lais Borbolato, João A. S. Amarante, Hélio D. Perottoni +5

The Milky Way in-situ halo, also known as the Splash, consists of old (age 10 Gyr), metal-rich ([Fe/H] ), high- stars, i.e., thick disk-like chemistry, on halo-like…

astro-ph.GA2026

The Metallicity Gradient of Sagittarius Dwarf Spheroidal Galaxy Prior to Infall Constrained by S-PLUS Observations of its Tidal Stream

Felipe Almeida-Fernandes, Guilherme Limberg, Hélio D. Perottoni +16

We study the metallicity distribution along the Sagittarius (Sgr) stream using photometric metallicities from S-PLUS DR4, combined with Gaia DR3 kinematics and APOGEE DR17 spectros…

astro-ph.GA2026

Characterizing the velocity anisotropy of the Milky Way's stellar halo

F. O. Barbosa, A. Pérez-Villegas, S. Rossi +6

Modeling the Milky Way stellar halo requires well-determined density and velocity anisotropy profiles. However, it has been challenging to gather a large sample of stars with six-d…

astro-ph.GA2025★ 1 cited

GASTRO library II: Exploring Chemical Bimodalities in Disk Galaxies with GSE-like Mergers and Massive Star-forming Clumps

João A. S. Amarante, Chervin F. P. Laporte, Victor P. Debattista +10

We use several smoothed particle hydrodynamics+N-body models as part of the GASTRO library to study the role of high-density star-forming clumpy regions and a single merger on the…

astro-ph.GA2025

Early Co-formation of the Milky Way's Thin and Thick Disks at Redshift z > 2

Lais Borbolato, Silvia Rossi, Hélio D. Perottoni +8

The Milky Way serves as a template for understanding the formation and evolution of late-type massive disk galaxies since we can obtain detailed chemical and kinematic information…

astro-ph.GA2024★ 8 cited

Stellar atmospheric parameters and chemical abundances of about 5 million stars from S-PLUS multi-band photometry

C. E. Ferreira Lopes, L. A. Gutiérrez-Soto, V. S. Ferreira Alberice +30

Context. Spectroscopic surveys like APOGEE, GALAH, and LAMOST have significantly advanced our understanding of the Milky Way by providing extensive stellar parameters and chemical…

astro-ph.GA2024

The Fourth S-PLUS Data Release: 12-filter photometry covering square degrees in the southern hemisphere

Fabio R. Herpich, Felipe Almeida-Fernandes, Gustavo B. Oliveira Schwarz +68

The Southern Photometric Local Universe Survey (S-PLUS) is a project to map sq deg of the sky using twelve bands (seven narrow and five broadbands). Observations are per…

astro-ph.GA2023★ 2 cited

Ages and metallicities of stellar clusters using S-PLUS narrow-band integrated photometry: the Small Magellanic Cloud

Gabriel Fabiano de Souza, Pieter Westera, Felipe Almeida-Fernandes +14

The Magellanic Clouds are the most massive and closest satellite galaxies of the Milky Way, with stars covering ages from a few Myr up to 13 Gyr. This makes them important for vali…

astro-ph.GA2023

All-sky Kinematics and Chemistry of Monoceros Stellar Overdensity

Lais Borbolato, Hélio D. Perottoni, Silvia Rossi +7

We explore the kinematic and chemical properties of Monoceros stellar overdensity by combining data from 2MASS, WISE, APOGEE, and . Monoceros is a structure located to…

astro-ph.GA2023★ 4 cited

The Chemodynamical Nature of the Triangulum-Andromeda Overdensity

Yuri Abuchaim, Hélio D. Perottoni, Silvia Rossi +7

We present a chemodynamical study of the Triangulum-Andromeda overdensity (TriAnd) employing a sample of 31 candidate stars observed with the GRACES high-resolution (=40,000) sp…

astro-ph.GA2023★ 67 cited

Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc

F. Anders, P. Gispert, B. Ratcliffe +12

Over the last few years, many studies have found an empirical relationship between the abundance of a star and its age. Here we estimate spectroscopic stellar ages for 178 825 red-…

astro-ph.GA2022★ 26 cited

Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor () Regime

Guilherme Limberg, Anna B. A. Queiroz, Hélio D. Perottoni +6

In this work, we study the phase-space and chemical properties of Sagittarius (Sgr) stream, the tidal tails produced by the ongoing destruction of Sgr dwarf spheroidal (dSph) galax…

astro-ph.GA2022★ 90 cited

Reconstructing the Disrupted Dwarf Galaxy -Sausage/Enceladus Using its Stars and Globular Clusters

Guilherme Limberg, Stefano O. Souza, Angeles Pérez-Villegas +3

We combine spectroscopic, photometric, and astrometric information from APOGEE data release 17 and early data release 3 to perform a self-consistent characterization of $Gai…

astro-ph.GA2022★ 26 cited

The Unmixed Debris of Gaia-Sausage/Enceladus in the Form of a Pair of Halo Stellar Overdensities

Hélio D. Perottoni, Guilherme Limberg, João A. S. Amarante +5

In the first billion years after its formation, the Galaxy underwent several mergers with dwarf satellites of various masses. The debris of Gaia-Sausage/Enceladus (GSE), the galaxy…

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★ 29 cited

Abundance Patterns of and Neutron-capture Elements in the Helmi Stream

Guilherme Limberg, Rafael M. Santucci, Silvia Rossi +6

We identified 8 additional stars as members of the Helmi stream (HStr) in the combined GALAH+ DR3 and EDR3 catalog. By consistently reevaluating claimed members from the lit…

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★ 26 cited

Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy

Guilherme Limberg, Rafael M. Santucci, Silvia Rossi +7

We present the results of spectroscopic follow-up for 1897 low-metallicity star candidates, selected from the Best & Brightest (B&B) Survey, carried out with the GMOS-N/S (Gemini N…

astro-ph.GA2020★ 65 cited

Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys

Guilherme Limberg, Silvia Rossi, Timothy C. Beers +13

We analyze the dynamical properties of 1500 very metal-poor (VMP; [Fe/H] ) halo stars, based primarily on medium-resolution spectroscopic data from the HK and…

astro-ph.GA2020

The Abundance Pattern of elements in the Triangulum-Andromeda Overdensity

J. V. Sales Silva, K. Cunha, H. D. Perottoni +5

The close relationship between the nature of the Triangulum-Andromeda (TriAnd) overdensity and the Galactic disk has become increasingly evident in recent years. However, the chemi…

astro-ph.GA2019★ 5 cited

Triangulum-Andromeda overdensity: a region with a complex stellar population

J. V. Sales Silva, H. D. Perottoni, K. Cunha +4

The Triangulum--Andromeda (TriAnd) overdensity is a distant structure of the Milky Way located in the second Galactic quadrant well below the Galactic plane. Since its discovery, i…

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…