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R. D. da Silva

4 papers hereh-index 12 citations2 works total

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

author position
  • first author1
  • middle author3

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

fields
  • astro-ph.GA1
  • astro-ph.SR1
  • cs.FL1
  • cs.LG1
same name
  • R. D. Da Silva — 7 papers, h 1
  • R. D. da Silva — 1 paper, h 0
  • R. D. da Silva — 1 paper, h 2
  • R. D. da Silva — 1 paper, h 0
  • R. D. da Silva — 1 paper, h 2

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

most citedOxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk

32 citations · 37 across the 3 of their papers we have counts for

collaborators

4 papers

cs.FL2023★ 5 cited

Conflict-Aware Active Automata Learning

Tiago Ferreira, Léo Henry, Raquel Fernandes da Silva +1

Active automata learning algorithms cannot easily handle conflict in the observation data (different outputs observed for the same inputs). This inherent inability to recover after…

cs.LG2023

Conflict-Aware Active Automata Learning (Extended Version)

Tiago Ferreira, Léo Henry, Raquel Fernandes da Silva +1

Active automata learning algorithms cannot easily handle conflict in the observation data (different outputs observed for the same inputs). This inherent inability to recover after…

astro-ph.GA2023★ 32 cited

Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk

R. da Silva, V. D'Orazi, M. Palla +25

Classical Cepheids (CCs) are solid distance indicators and tracers of young stellar populations. Our aim is to provide iron, oxygen, and sulfur abundances for the largest and most…

astro-ph.SR2023

Effective temperatures of classical Cepheids from line-depth ratios in the H-band

V. Kovtyukh, B. Lemasle, N. Nardetto +6

The technique of line depth ratios (LDR) is one of the methods to determine the effective temperature of a star. They are crucial in the spectroscopic studies of variable stars lik…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.