87 citations · 331 across the 13 of their papers we have counts for
13 papers
The PHASES Differential Astrometry Data Archive. V. Candidate Substellar Companions to Binary Systems
Matthew W. Muterspaugh, Benjamin F. Lane, S. R. Kulkarni +7
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbi…
The PHASES Differential Astrometry Data Archive IV: The Triple Star Systems 63 Gem A and HR 2896
Matthew W. Muterspaugh, Francis C. Fekel, Benjamin F. Lane +7
(Abridged) Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) are used to constrain the astrometric orbit of the…
The PHASES Differential Astrometry Data Archive. III. Limits to Tertiary Companions
Matthew W. Muterspaugh, Benjamin F. Lane, S. R. Kulkarni +4
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian pla…
The orbits of the quadruple star system 88 Tau A from PHASES differential astrometry and radial velocity
Benjamin F. Lane, Matthew W. Muterspaugh, Francis C. Fekel +7
We have used high precision differential astrometry from the Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) project and radial velocity measurements cover…
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…
Limits to Tertiary Astrometric Companions in Binary Systems
Matthew W. Muterspaugh, Benjamin F. Lane, S. R. Kulkarni +3
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) has monitored 37 sub-arcsecond binary systems to determine whether their Keplerian orbits are perturbed…