activity
20082026
most citedThe Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V

282 citations · 2.8k across the 80 of their papers we have counts for

collaborators
Showing 2020Show all

7 papers · 1 filter

astro-ph.EP2020★ 104 cited

A New Window into Planet Formation and Migration: Refractory-to-Volatile Elemental Ratios in Ultra-hot Jupiters

Joshua D. Lothringer, Zafar Rustamkulov, David K. Sing +3

A primary goal of exoplanet characterization is to use a planet's current composition to understand how that planet formed. For example, the C/O ratio has long been recognized as c…

astro-ph.SR2020★ 37 cited

The non-monotonic, strong metallicity dependence of the wide-binary fraction

Hsiang-Chih Hwang, Yuan-Sen Ting, Kevin C. Schlaufman +2

The metallicity dependence of the wide-binary fraction in stellar populations plays a critical role in resolving the open question of wide binary formation. In this paper, we inves…

astro-ph.EP2020★ 31 cited

An Increase in Small-planet Occurrence with Metallicity for Late-type Dwarf Stars in the Kepler Field and Its Implications for Planet Formation

Cicero X. Lu, Kevin C. Schlaufman, Sihao Cheng

While it is well established that giant-planet occurrence rises rapidly with host star metallicity, it is not yet clear if small-planet occurrence around late-type dwarf stars depe…

astro-ph.SR2020★ 22 cited

The Most Metal-poor Stars in the Inner Bulge

Henrique Reggiani, Kevin C. Schlaufman, Andrew R. Casey +1

The bulge is the oldest component of the Milky Way. Since numerous simulations of Milky Way formation have predicted that the oldest stars at a given metallicity are found on tight…

astro-ph.EP2020★ 36 cited

Ultra-short-period Planets are Stable Against Tidal Inspiral

Jacob H. Hamer, Kevin C. Schlaufman

It has been unambiguously shown in both individual systems and at the population level that hot Jupiters experience tidal inspiral before the end of their host stars' main sequence…

astro-ph.EP2020★ 24 cited

Very wide companion fraction from Gaia DR2: a weak or no enhancement for hot jupiter hosts, and a strong enhancement for contact binaries

Hsiang-Chih Hwang, Jacob H. Hamer, Nadia L. Zakamska +1

There is an ongoing debate on whether hot jupiter hosts are more likely to be found in wide binaries with separations of AU. In this paper, we search for comoving, ve…