activity
20052008
most citedMasses, Luminosities, and Orbital Coplanarities of the mu Orionis Quadruple Star System from PHASES Differential Astrometry

56 citations · 183 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph200841 cited

A High Precision, Optical Polarimeter to Measure Inclinations of High Mass X-Ray Binaries

Sloane J. Wiktorowicz, Keith Matthews

We present commissioning data for the POLISH instrument obtained on the Hale 5-m telescope. The goal of this high precision polarimeter is to constrain orbital inclination of high…

astro-ph200756 cited

Masses, Luminosities, and Orbital Coplanarities of the mu Orionis Quadruple Star System from PHASES Differential Astrometry

Matthew W. Muterspaugh, Benjamin F. Lane, Francis C. Fekel +6

mu Orionis was identified by spectroscopic studies as a quadruple star system. Seventeen high precision differential astrometry measurements of mu Ori have been collected by the Pa…

astro-ph200635 cited

Liquid Water Oceans in Ice Giants

Sloane J. Wiktorowicz, Andrew P. Ingersoll

Aptly named, ice giants such as Uranus and Neptune contain significant amounts of water. While this water cannot be present near the cloud tops, it must be abundant in the deep int…

astro-ph200651 cited

Masses of Astrometrically-Discovered and Imaged Binaries: G 78-28AB and GJ 231.1BC

Steven H. Pravdo, Stuart B. Shaklan, Sloane J. Wiktorowicz +5

The Stellar Planet Survey (STEPS) is an ongoing astrometric search for giant planets and brown dwarfs around a sample of ~30 M-dwarfs. We have discovered several low-mass companion…

astro-ph2005

A Spitzer Search for Infrared Excesses around Massive Young White Dwarfs

Brad M. S. Hansen, Shri Kulkarni, Sloane Wiktorowicz

We examine 14 hot white dwarfs for signs of infrared excess using the Spitzer Space Telescope. Twelve of the objects are massive white dwarfs which have been suggested to be the re…

astro-ph2005

PHASES Differential Astrometry and Iodine Cell Radial Velocities of the kappa Pegasi Triple Star System

Matthew W. Muterspaugh, Benjamin F. Lane, Maciej Konacki +5

kappa Pegasi is a well-known, nearby triple star system. It consists of a ``wide'' pair with semi-major axis 235 milli-arcseconds, one component of which is a single-line spectrosc…