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Diffraction-Limited Imaging II. Optical Aperture-Synthesis Imaging of Two Binary Stars

Nakajima, T. and Kulkarni, S. R. and Gorham, P. W. and Ghez, A. M. and Neugebauer, G. and Oke, J. B. and Prince, T. A. and Readhead, A. C. S. (1989) Diffraction-Limited Imaging II. Optical Aperture-Synthesis Imaging of Two Binary Stars. Astronomical Journal, 97 (5). pp. 1510-1521. ISSN 0004-6256. https://resolver.caltech.edu/CaltechAUTHORS:20140509-084903601

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Abstract

We have used the technique of nonredundant masking at the Hale 5 m telescope and radio VLBI imaging software are used to make optical aperture-synthesis maps of two binary stars, β Corona Borealis and σ Herculis. The dynamic range of the map of β CrB is about 50:1. For σ Her, we find a separation of 70 milliarcsec. These maps demonstrate the potential of the nonredundant masking technique for diffraction-limited imaging of astronomical objects with high dynamic range. We find that the optimal integration time for measuring the closure phase is found to be longer than that for measuring the fringe amplitude. There is not a close relationship between amplitude errors and phase errors, as is found in radio astronomy, and amplitude self-calibration is less effective at optical wavelengths than at radio wavelengths. The primary beam sensitivity correlation made in radio astronomy is not necessary in optical interferometry.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/115090DOIArticle
http://adsabs.harvard.edu/abs/1989AJ.....97.1510NADSArticle
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
Ghez, A. M.0000-0003-3230-5055
Prince, T. A.0000-0002-8850-3627
Readhead, A. C. S.0000-0001-9152-961X
Additional Information:Copyright 1989 American Astronomical Society. Received 17 January 1989; revised 7 February 1989. We would like to thank E. Emery, F. Harris, and R. Nadler for the professional engineering of the observing and data acquisition systems. We thank A. Lee and G. Smith for excellent programming for the peripherals of the data-acquisition system. We also thank the mountain staff at the Palomar Observatory for assistance with the setup and observations. We would like to thank T. Pearson for assistance with the VLBI software. We thank the W. M. Keck Foundation for financial support. P. W. G. and T. A. P. acknowledge support from Department of Energy grant no. DE-FG-03-85ER25009 and National Science Foundation grant no. AST8351736. T. N. thanks the Schlumberger Fellowship.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
W. M. Keck FoundationUNSPECIFIED
Department of Energy (DOE)DE-FG-03-85ER25009
NSFAST-8351736
Schlumberger FoundationUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1990-16
Issue or Number:5
Record Number:CaltechAUTHORS:20140509-084903601
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140509-084903601
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:45630
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:09 May 2014 19:34
Last Modified:04 Nov 2019 02:45

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