activity
20122019
most citedKepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone

255 citations · 700 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2019114 cited

The Featureless Transmission Spectra of Two Super-Puff Planets

Jessica E. Libby-Roberts, Zachory K. Berta-Thompson, Jean-Michel Desert +9

The Kepler mission revealed a class of planets known as ''super-puffs,'' with masses only a few times larger than Earth's but radii larger than Neptune, giving them very low mean d…

astro-ph.EP2018

Stellar obliquities and magnetic activities of Planet-Hosting Stars and Eclipsing Binaries based on Transit Chord Correlation

Fei Dai, Joshua N. Winn, Zachory Berta-Thompson +2

The light curve of an eclipsing system shows anomalies whenever the eclipsing body passes in front of active regions on the eclipsed star. In some cases, the pattern of anomalies c…

astro-ph.EP2018

Kepler-78 and the Ultra-Short-Period Planets

Joshua N. Winn, Roberto Sanchis-Ojeda, Saul Rappaport

Compared to the Earth, the exoplanet Kepler-78b has a similar size (1.2 ) and an orbital period a thousand times shorter (8.5 hours). It is currently the smallest planet…

astro-ph.EP201617 cited

On the Detection of Non-Transiting Exoplanets with Dusty Tails

John DeVore, Saul Rappaport, Roberto Sanchis-Ojeda +2

We present a way of searching for non-transiting exoplanets with dusty tails. In the transiting case, the extinction by dust during the transit removes more light from the beam tha…

astro-ph.EP2016

Doppler Monitoring of five K2 Transiting Planetary Systems

Fei Dai, Joshua N. Winn, Simon Albrecht +21

In an effort to measure the masses of planets discovered by the NASA {\it K2} mission, we have conducted precise Doppler observations of five stars with transiting planets. We pres…

astro-ph.SR201540 cited

Time variation of Kepler transits induced by stellar spots - a way to distinguish between prograde and retrograde motion. II. Application to KOIs

Tomer Holczer, Avi Shporer, Tsevi Mazeh +8

Mazeh, Holczer, and Shporer (2015) have presented an approach that can, in principle, use the derived transit timing variation (TTV) of some transiting planets observed by the $Kep…