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Fabienne A. Bastien

4 papers here

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

author position
  • sole author1
  • first author1
  • middle author1
  • last author1

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

fields
  • astro-ph.EP3
  • astro-ph.SR1
ORCID 0000-0002-7243-1921

identity via Semantic Scholar / OpenAlex

most citedDiscovery of a Transiting Planet Near the Snow-Line

37 citations · 56 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2014★ 1 cited

Convection in Cool Stars, as Seen Through Kepler's Eyes

Fabienne A. Bastien

Stellar surface processes represent a fundamental limit to the detection of extrasolar planets with the currently most heavily-used techniques. As such, considerable effort has gon…

astro-ph.EP2014★ 37 cited

Discovery of a Transiting Planet Near the Snow-Line

David M. Kipping, Guillermo Torres, Lars A. Buchhave +8

In most theories of planet formation, the snow-line represents a boundary between the emergence of the interior rocky planets and the exterior ice giants. The wide separation of th…

astro-ph.EP2014

Larger Planet Radii Inferred from Stellar "Flicker" Brightness Variations of Bright Planet Host Stars

Fabienne A. Bastien, Keivan G. Stassun, Joshua Pepper

Most extrasolar planets have been detected by their influence on their parent star, typically either gravitationally (the Doppler method) or by the small dip in brightness as the p…

astro-ph.EP2014★ 18 cited

Flicker as a tool for characterizing planets through Asterodensity Profiling

David M. Kipping, Fabienne A. Bastien, Keivan G. Stassun +3

Variability in the time series brightness of a star on a timescale of 8 hours, known as 'flicker', has been previously demonstrated to serve as a proxy for the surface gravity of a…

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