activity
20092020
most citedAn analysis of the composite stellar population in M32

49 citations · 107 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020

UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems

M. L. L. Dantas

Ultraviolet (UV) emission from galaxies is associated with hot components, whether from stellar sources or not. By making use of colour-colour diagrams, early-type galaxies (ETGs)…

astro-ph.GA2020★ 7 cited

UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample

M. L. L. Dantas, P. R. T. Coelho, P. Sánchez-Blázquez

The ultraviolet (UV) upturn is characterised by an unexpected up-rise of the UV flux in quiescent galaxies between the Lyman limit and 2500Å. By making use of colour-colour diagram…

astro-ph.GA2020★ 19 cited

Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry

Ariel Werle, Roberto Cid Fernandes, Natalia Vale Asari +10

Stellar population studies of early-type galaxies (ETGs) based on their optical stellar continuum suggest that these are quiescent systems. However, emission lines and ultraviolet…

astro-ph.GA2019★ 12 cited

UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?

M. L. L. Dantas, P. R. T. Coelho, R. S. de Souza +1

The so-called ultraviolet (UV) upturn of elliptical galaxies is a phenomenon characterised by the up-rise of their fluxes in bluer wavelengths, typically in the 1,200-2,500A range.…

astro-ph.IM2018★ 20 cited

Spatial field reconstruction with INLA: Application to IFU galaxy data

S. González-Gaitán, R. S. de Souza, A. Krone-Martins +4

Astronomical observations of extended sources, such as cubes of integral field spectroscopy (IFS), encode auto-correlated spatial structures that cannot be optimally exploited by s…

astro-ph.GA2009★ 49 cited

An analysis of the composite stellar population in M32

P. Coelho, C. Mendes de Oliveira, R. Cid Fernandes

We obtained long-slit spectra of high signal-to-noise ratio of the galaxy M32 with the GMOS spectrograph at the GEMINI North telescope. We analysed the integrated spectra by means…