activity
20082026
most citedThe Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

205 citations · 1.5k across the 63 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021

Photometric redshifts for the S-PLUS Survey: is machine learning up to the task?

E. V. R. Lima, L. Sodré, C. R. Bom +14

The Southern Photometric Local Universe Survey (S-PLUS) is a novel project that aims to map the Southern Hemisphere using a twelve filter system, comprising five broad-band SDSS-li…

astro-ph.GA2021★ 8 cited

Chemical abundances in Seyfert galaxies -- VIII. Argon abundance estimates

A. F. Monteiro, O. L. Dors

For the first time, the argon abundance relative to hydrogen abundance (Ar/H) in the narrow line region of a sample of Seyfert 2 nuclei has been derived. In view of this, optical n…

astro-ph.GA2021

Chemical abundances in Seyfert galaxies -- VII. Direct abundance determination of neon based on optical and infrared emission lines

Mark Armah, O. L. Dors, C. P. Aydar +6

For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfert~2 nuclei. In view of this, we compiled from the literature fluxes of optical…

astro-ph.GA2021★ 1 cited

Chemical abundances in Seyfert galaxies VI. Empirical abundance calibration

Dors, O. L

We derived a bi-dimensional calibration between the emission line ratios R23=([O II]3726+3729+[O II]4959+5007)/Hb, P=[([O II]4959+5007)/Hb]/R23 and the oxygen abundance relative to…

astro-ph.GA2021★ 13 cited

Electron temperature fluctuations in Seyfert galaxies

Rogemar A. Riffel, Oli L. Dors, Angela Krabbe +1

We use Gemini GMOS-IFU observations of three luminous nearby Seyfert galaxies (Mrk79, Mrk348 and Mrk607) to estimate the electron temperature () fluctuations in the inne…

astro-ph.GA2021★ 11 cited

Chemical Abundance of the LINER galaxy UGC 4805 with SDSS-IV MaNGA

A. C. Krabbe, C. B. Oliveira, I. A. Zinchenko +5

Chemical abundance determinations in Low-Ionization Nuclear Line Regions (LINERs) are especially complex and uncertain because the nature of the ionizing source of this kind of obj…