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researcher

Sofia Covarrubias

3 papers hereh-index 212 citations3 works total

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

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP1
  • astro-ph.IM1
  • astro-ph.SR1

identity via Semantic Scholar / OpenAlex

most citedN-body Interactions will be Detectable in the HR-8799 System within 5 years with VLTI-GRAVITY

4 citations · 4 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.IM2024

orbitize! v3: Orbit fitting for the High-contrast Imaging Community

Sarah Blunt, Jason Jinfei Wang, Lea Hirsch +18

orbitize! is a package for Bayesian modeling of the orbital parameters of resolved binary objects from time series measurements. It was developed with the needs of the high-contras…

astro-ph.SR2024

Constraining Extra Mixing during the Main Sequence: What Depletes Lithium Does Not Touch Beryllium

Henrique Reggiani, Jhon Yana Galarza, Diego Lorenzo-Oliveira +4

Measurements of lithium abundances in solar-type stars have shown that standard models of stellar evolution are incapable of explaining the observed depletion as a function of stel…

astro-ph.EP2022★ 4 cited

N-body Interactions will be Detectable in the HR-8799 System within 5 years with VLTI-GRAVITY

Sofia Covarrubias, Sarah Blunt, Jason J. Wang

While Keplerian orbits account for the majority of the astrometric motion of directly-imaged planets, perturbations due to N-body interactions allow us to directly constrain exopla…

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