activity
20152024
most citedHigh-Resolution Spectroscopic Detection of TiO and Stratosphere in the Day-side of WASP-33b

168 citations · 793 across the 17 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.EP2018

Larger mutual inclinations for the shortest-period planets

Fei Dai, Kento Masuda, Joshua N. Winn

The {\it Kepler} mission revealed a population of compact multiple-planet systems with orbital periods shorter than a year, and occasionally even shorter than a day. By analyzing a…

astro-ph.EP2018

Kepler-730b is probably a hot Jupiter with a small companion

Wei Zhu, Fei Dai, Kento Masuda

Here we draw attention to a candidate system with one hot Jupiter and one small, nearby companion, revealed by the recent Kepler data release (DR25). The hot Jupiter, Kepler-730b,…

astro-ph.HE2018

Prospects of Finding Detached Black Hole-Star Binaries with TESS

Kento Masuda, Kenta Hotokezaka

We discuss prospects of identifying and characterizing black hole (BH) companions to normal stars on tight but detached orbits, using photometric data from the Transiting Exoplanet…

astro-ph.CO2018

A Hubble constant measurement from superluminal motion of the jet in GW170817

Kenta Hotokezaka, Ehud Nakar, Ore Gottlieb +5

The Hubble constant () measures the current expansion rate of the Universe, and plays a fundamental role in cosmology. Tremendous effort has been dedicated over the past decad…

astro-ph.EP2018

Biases in Planet Occurrence Caused by Unresolved Binaries in Transit Surveys

L. G. Bouma, Kento Masuda, J. N. Winn

Wide-field surveys for transiting planets, such as the NASA Kepler and TESS missions, are usually conducted without knowing which stars have binary companions. Unresolved and unrec…

astro-ph.EP2018

Systematic Search for Rings around Kepler Planet Candidates: Constraints on Ring Size and Occurrence Rate

Masataka Aizawa, Kento Masuda, Hajime Kawahara +1

We perform a systematic search for rings around 168 Kepler planet candidates with sufficient signal-to-noise ratios that are selected from all the short-cadence data. We fit ringed…