We argue that adding large apertures with adaptive optics to an optical interferometer improves the performance of the interferometer in two ways: it improves...
naval research lab washington dc optical sciences div, 2007
The optical interferometry community has discussed the possibility of using adaptive optics (AO) on apertures much larger than the atmospheric coherence length...
We have developed a method for performing long coherent integrations with the Navy Prototype Optical Interferometer (NPOI), which is based on fitting a model...
In this report we explore replacing the widely used optimal V2 estimator with a model-fitting approach. We show that it is possible to fit the fringe power...
naval research lab washington dc remote sensing div, 2009
We present the results of an experiment to image the interacting binary star Beta Lyrae with data from the Navy Prototype Optical Interferometer using a...
naval research lab washington dc remote sensing div, 2006
We determine the masses and magnitude difference of the components of the Hyades spectroscopic binary theta(2) Tauri. We find that both components appear to be...
state univ of new york at stony brook dept of physics and astronomy, 2006
We report the successful fitting of a Roche model, with a surface temperature gradient following the von Zeipel gravity darkening law, to observations of...
state univ of new york at stony brook dept of physics and astronomy, 2006
Vega, the second brightest star in the northern hemisphere, serves as a primary spectral type standard. Although its spectrum is dominated by broad hydrogen...
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