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20002019
most citedAstrophysical Quantities of Cepheid Variables Measured with the NPOI

230 citations · 1k across the 23 of their papers we have counts for

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astro-ph2008★ 2 cited

Solving the Imaging Problem with Coherently Integrated Multiwavelength Data

H. R. Schmitt, T. A. Pauls, J. T. Armstrong +7

Recovering images from optical interferometric observations is one of the major challenges in the field. Unlike the case of observations at radio wavelengths, in the optical the at…

astro-ph2008★ 3 cited

Measurements of binary stars with coherent integration of NPOI data

Anders M. Jorgensen, H. Schmitt, R. Hindsley +5

In this paper we use coherently integrated visibilities (see separate paper in these proceedings, Jorgensen et al. 2008) to measure the properties of binary stars. We use only the…

astro-ph2008★ 6 cited

Practical Coherent Integration with the NPOI

Anders M. Jorgensen, Dave Mozurkewich, Henrique Schmitt +4

In this paper we will discuss the current status of coherent integration with the Navy Prototype Optical Interferometer (NPOI) (Armstrong et al. 2008). Coherent integration relies…

astro-ph2008★ 25 cited

The effect of rotation on the spectrum of Vega

Jinmi Yoon, Deane M. Peterson, Robert J. Zagarello +2

The discovery that Vega is a rapidly rotating pole-on star has raised a number of questions about this fundamental standard, including such issues as its composition, and in turn i…

astro-ph2008★ 34 cited

Navy Prototype Optical Interferometer Imaging of Line Emission Regions of beta Lyrae Using Differential Phase Referencing

H. R. Schmitt, T. A. Pauls, C. Tycner +9

We present the results of an experiment to image the interacting binary star beta Lyrae with data from the Navy Prototype Optical Interferometer (NPOI), using a differential phase…

astro-ph2006★ 19 cited

Initial Results from the USNO Dispersed Fourier Transform Spectrograph

Arsen R. Hajian, Bradford B. Behr, Andrew T. Cenko +15

We have designed and constructed a ``dispersed Fourier Transform Spectrometer'' (dFTS), consisting of a conventional FTS followed by a grating spectrometer. By combining these two…