activity
20072021
most citedThe Transiting Circumbinary Planets Kepler-34 and Kepler-35

484 citations · 2.1k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2021★ 10 cited

Photodynamical Modeling of the Fascinating Eclipses in the Triple-Star System KOI-126

Mitchell E. Yenawine, William F. Welsh, Jerome A. Orosz +7

We explore the fascinating eclipses and dynamics of the compact hierarchical triple star system KOI-126 (KIC 5897826). This system is comprised of a pair of M-dwarf stars (KOI-126…

physics.ed-ph2021★ 1 cited

Developing Virtual Reality Activities for the Astro 101 Class and Lab

Gur Windmiller, Philip Blanco, William F. Welsh

We report on our ongoing efforts to develop, implement, and test VR activities for the introductory astronomy course and laboratory. Specifically, we developed immersive activities…

astro-ph.SR2020★ 1 cited

Fast Transit Computation Using Tabulated Stellar Intensities

Donald R. Short, Jerome A. Orosz, Gur Windmiller +1

Limb darkening laws are convenient parameterizations of the stellar intensity center-to-limb variation, and their use is ubiquitous in eclipse and transit modeling. But they are no…

astro-ph.SR2020★ 47 cited

Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary

Quentin J Socia, William F Welsh, Jerome A Orosz +7

We report the discovery of a Neptune-size (R_p = 3.87 +/- 0.06 R_Earth) transiting circumbinary planet, Kepler-1661 b, found in the Kepler photometry. The planet has a period of ~1…

physics.ed-ph2019★ 1 cited

Lessons Learned from Teaching Astronomy with Virtual Reality

Philip Blanco, Gur Windmiller, William Welsh +1

We report on the initial phase of an ongoing, multi-stage investigation of how to incorporate Virtual Reality (VR) technology in teaching introductory astronomy concepts. Our goal…

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…