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19992022
most citedCoronagraphic Survey for Companions of Stars within 8 pc

95 citations · 559 across the 21 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 13 cited

Interferometric Studies of the extreme binary, Aurigae: Pre-eclipse Observations

R. Stencel, M. Creech-Eakman, A. Hart +3

We report new and archival K-band interferometric uniform disk diameters obtained with the Palomar Testbed Interferometer for the eclipsing binary star Aurigae, in advance of t…

astro-ph2008★ 19 cited

Milliarcsecond N-Band Observations of the Nova RS Ophiuchi: First Science with the Keck Interferometer Nuller

R. K. Barry, W. C. Danchi, W. A. Traub +38

We report observations of the nova RS Ophiuchi (RS Oph) using the Keck Interferometer Nuller (KIN), approximately 3.8 days following the most recent outburst that occurred on 2006…

astro-ph2007★ 60 cited

The Palomar Testbed Interferometer Calibrator Catalog

G. T. van Belle, G. van Belle, M. J. Creech-Eakman +7

The Palomar Testbed Interferometer (PTI) archive of observations between 1998 and 2005 is examined for objects appropriate for calibration of optical long-baseline interferometer o…

astro-ph2002★ 51 cited

Long baseline interferometric observations of Cepheids

B. F. Lane, M. Creech-Eakman, T. E. Nordgren

We present observations of the galactic cepheids eta Aql and zeta Gem. Our observations are able to resolve the diameter changes associated with pulsation. This allows us to determ…

astro-ph2001★ 95 cited

Coronagraphic Survey for Companions of Stars within 8 pc

B. R. Oppenheimer, D. A. Golimowski, S. R. Kulkarni +4

We present the technique and results of a survey of stars within 8 pc of the Sun with declinations $\bfδ> -35\arcdeg$ (J2000.00). The survey, designed to find without color bias fa…

astro-ph2000★ 52 cited

Infrared interferometric observations of young stellar objects

R. L. Akeson, D. R. Ciardi, G. T. van Belle +2

We present infrared observations of four young stellar objects using the Palomar Testbed Interferometer (PTI). For three of the sources, T Tau, MWC 147 and SU Aur, the 2.2 micron e…