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O. Aguiar

170 papers hereh-index 8246.1k citations258 works total

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

author position
  • sole author2
  • middle author11
  • last author12

Across the 25 of 170 papers where every author was matched, so the position is known.

fields
  • gr-qc95
  • astro-ph.HE55
  • astro-ph.CO9
  • astro-ph.IM7
  • astro-ph4
same name
  • O. Aguiar — 19 papers, h 6
  • O. Aguiar — 10 papers, h 20

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

activity
19982026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 41.2k across the 167 of their papers we have counts for

collaborators
Showing 2005Show all

2 papers · 1 filter

astro-ph2005

Can black hole MACHO binaries be detected by the Brazilian spherical antenna?

J. C. N. de Araujo, O. D. Miranda, C. S. Castro +2

Different studies show that dark matter of non-baryonic origin might exist. There have been experimental evidences that at least one form of dark matter has been detected through m…

gr-qc2005★ 14 cited

Detectability of f-mode Unstable Neutron Stars by the Schenberg Spherical Antenna

J. C. N. de Araujo, O. D. Miranda, O. D. Aguiar

The Brazilian spherical antenna (Schenberg) is planned to detect high frequency gravitational waves (GWs) ranging from 3.0 kHz to 3.4 kHz. There is a host of astrophysical sources…

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