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researcher

P. Santos

4 papers hereh-index 13 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • P. Santos — 44 papers, h 32
  • P. Santos — 8 papers, h 12
  • P. Santos — 5 papers, h 14
  • P. Santos — 4 papers, h 10
  • P. Santos — 4 papers, h 12
  • P. Santos — 4 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2025

Metallicity of Active Galactic Nuclei from ultraviolet and optical emission lines-II. Revisiting the C43 metallicity calibration and its implications

O. L. Dors, C. B. Oliveira, M. V. Cardaci +7

In this study, a new semi-empirical calibration is proposed between ultraviolet emission lines (\ion{C}{iii}]λ1909, \ion{C}{iv}λ1549, \ion{He}{ii}]λ1640) of…

astro-ph.GA2025

Metallicity of Active Galactic Nuclei from ultraviolet and optical emission lines I: Carbon abundance dependence

O. L. Dors, C. B. Oliveira, M. V. Cardaci +9

Metallicity (Z) estimates based on ultraviolet (UV) emission lines from the narrow-line regions (NLRs) of active galactic nuclei (AGNs) have been found to differ from those deriv…

astro-ph.GA2024

Semi-empirical calibration of the oxygen abundance for LINER galaxies based on SDSS-IV MaNGA -- The case for strong and weak AGN

C. B. Oliveira, O. L. Dors, I. A. Zinchenko +5

In this paper, we present a semi-empirical calibration between the oxygen abundance and the N2 emission-line ratio for Low Ionization Nuclear Emission Regions (LINERs). This rela…

astro-ph.GA2024

Empirical calibration for helium abundance determinations in Active Galactic Nuclei

O. L. Dors, G. C. Almeida, C. B. Oliveira +10

For the first time, a calibration between the HeI λ5876/Hβ emission line ratio and the helium abundance y=12+log(He/H) for Narrow line regions (NLRs) of Seyfert~2 Activ…

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