activity
19982019
most citedThe Neptune-Sized Circumbinary Planet Kepler-38b

201 citations · 921 across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.SR2019★ 7 cited

Stellar Properties of KIC 8736245: An Eclipsing Binary with a Solar-type Star Leaving the Main Sequence

Tara Fetherolf, William F. Welsh, Jerome A. Orosz +5

There is a well-known stellar parameter discrepancy for late K and M dwarfs, in that the observed radii and temperatures are often respectively larger and cooler than predicted by…

astro-ph.SR2013★ 24 cited

Two New Long-Period Hot Subdwarf Binaries with Dwarf Companions

Brad N. Barlow, Sandra E. Liss, Richard A. Wade +1

Hot subdwarf stars with F-K main sequence binary companions have been known for decades, but the first orbital periods for such systems were published just recently. Current observ…

astro-ph.SR2012★ 38 cited

Kepler Studies of Low-Mass Eclipsing Binaries I. Parameters of the Long-Period Binary KIC 6131659

Gideon Bass, Jerome A. Orosz, William F. Welsh +5

KIC 6131659 is a long-period (17.5 days) eclipsing binary discovered by the Kepler mission. We analyzed six quarters of Kepler data along with supporting ground-based photometric a…

astro-ph.SR2012★ 201 cited

The Neptune-Sized Circumbinary Planet Kepler-38b

Jerome A. Orosz, William F. Welsh, Joshua A. Carter +28

We discuss the discovery and characterization of the circumbinary planet Kepler-38b. The stellar binary is single-lined, with a period of 18.8 days, and consists of a moderately ev…

astro-ph.SR2012★ 33 cited

A Radial Velocity Study of Composite-Spectra Hot Subdwarf Stars with the Hobby-Eberly Telescope

Brad N. Barlow, Richard A. Wade, Sandra E. Liss +2

Many hot subdwarf stars show composite spectral energy distributions indicative of cool main sequence companions. Binary population synthesis (BPS) models demonstrate such systems…

astro-ph.SR2012★ 57 cited

The Rømer Delay and Mass Ratio of the sdB+dM Binary 2M 1938+4603 from Kepler Eclipse Timings

Brad N. Barlow, Richard A. Wade, Sandra E. Liss

The eclipsing binary system 2M 1938+4603 consists of a pulsating hot subdwarf B star and a cool M dwarf companion in an effectively circular three-hour orbit. The light curve shows…