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20062024
most citedOptimal Dark Hole Generation via Two Deformable Mirrors with Stroke Minimization

150 citations · 1.1k across the 54 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.EP2018★ 18 cited

Planet occurrence rate density models including stellar effective temperature

Daniel Garrett, Dmitry Savransky, Rus Belikov

We present planet occurrence rate density models fit to Kepler data as a function of semi-major axis, planetary radius, and stellar effective temperature. We find that occurrence r…

astro-ph.IM2018★ 2 cited

Exoplanet Terra Incognita

Svetlana V. Berdyugina, Jeff R. Kuhn, Ruslan Belikov +1

Exoplanet surface imaging, cartography and the search for exolife are the next frontiers of planetology and astrophysics. Here we present an over-view of ideas and techniques to re…

astro-ph.IM2018

TDEM final report: Enhanced direct imaging exoplanet detection with astrometry mass determination

Eduardo Bendek, Ruslan Belikov, Olivier Guyon +6

This Final Report (FR) presents the results of the Enhanced direct imaging exoplanet detection with astrometry mass determination project, which was executed in support of NASA's E…

astro-ph.IM2018

Using Ground-Based Telescopes to Mature Key Technologies and Advance Science for Future NASA Exoplanet Direct Imaging Missions

Thayne Currie, Ruslan Belikov, Olivier Guyon +8

Ground-based telescopes have been playing a leading role in exoplanet direct imaging science and technological development for the past two decades and will continue to have an ind…

astro-ph.IM2018

The value of astrometry for exoplanet science

Eduardo Bendek, Mark Marley, Michael Shao +3

Exoplanets mass measurements will be a critical next step to assess the habitability of Earth-like planets: a key aspect of the 2020 vision in the previous decadal survey and also…

astro-ph.EP2018

Exoplanet Diversity in the Era of Space-based Direct Imaging Missions

Ravi Kopparapu, Eric Hebrard, Rus Belikov +55

This whitepaper discusses the diversity of exoplanets that could be detected by future observations, so that comparative exoplanetology can be performed in the upcoming era of larg…