activity
20172022
most citedInvestigating the Relation between Galaxy Properties and the Gaussianity of the Velocity Distribution of Groups and Clusters

35 citations · 97 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.SR202220 cited

Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid

R. Razera, B. Barbuy, T. C. Moura +19

The central part of the Galaxy host a multitude of stellar populations, including the spheroidal bulge stars, stars moved to the bulge through secular evolution of the bar, inner h…

astro-ph.SR202111 cited

Gemini/Phoenix H-band analysis of the globular cluster AL3

B. Barbuy, H. Ernandes, S. O. Souza +9

The globular cluster AL~3 is old and located in the inner bulge. Three individual stars were observed with the Phoenix spectrograph at the Gemini South telescope. The wavelength re…

astro-ph.GA20205 cited

Stellar Population Properties of ETGs in Compact Groups of Galaxies

Tatiana C. Moura, Reinaldo R. de Carvalho, Sandro B. Rembold +6

We present results on the study of the stellar population in Early-Type galaxies (ETGs) belonging to 151 Compact Groups (CGs). We also selected a field sample composed of 846 ETGs…

astro-ph.SR20198 cited

Integrated Spectra of Milky Way Globular Cluster

Tatiana Coelho de Moura, Marina Trevisan, Beatriz Barbuy +1

Integrated spectra of Milky Way globular clusters (GCs) are reproduced by computing synthetic spectra taking into account individual element abundances. Five clusters were selected…

astro-ph.GA20197 cited

The Mass Density Profile and Star Formation History of Gaussian and Non-Gaussian Clusters

R. R. de Carvalho, A. P. Costa, T. C. Moura +1

This paper is the third of a series in which we investigate the discrimination between Gaussian (G) and Non-Gaussian (NG) clusters, based on the velocity distribution of the member…

astro-ph.IM2019

Machine and Deep Learning Applied to Galaxy Morphology -- A Comparative Study

P. H. Barchi, R. R. de Carvalho, R. R. Rosa +7

Morphological classification is a key piece of information to define samples of galaxies aiming to study the large-scale structure of the universe. In essence, the challenge is to…