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Initial scientific results from phase-referenced astrometry of sub-arcsecond binaries

Muterspaugh, Matthew W. and Lane, Benjamin F. and Burke, B. F. and Konacki, Maciej and Kulkarni, S. R. (2004) Initial scientific results from phase-referenced astrometry of sub-arcsecond binaries. In: New Frontiers in Stellar Interferometry. Proceedings of SPIE. No.5491. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, pp. 82-89. ISBN 9780819454232. https://resolver.caltech.edu/CaltechAUTHORS:20180910-131322294

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Abstract

The Palomar Testbed Interferometer has observed several binary star systems whose separations fall between the interferometric coherence length (a few hundredths of an arcsecond) and the typical atmospheric seeing limit of one arcsecond. Using phase-referencing techniques we measure the relative separations of the systems to precisions of a few tens of micro-arcseconds. We present the first scientific results of these observations, including the astrometric detection of the faint third stellar component of the kappa Pegasi system.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.551980DOIArticle
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
Additional Information:© 2004 Society of Photo-Optical Instrumentation Engineers (SPIE). The PHASES project is funded by the Astronomy Department at the California Institute of Technology. We thank the members of the PTI Collaboration for their contributions to the instrument construction, operation, maintenance, and continued improvements. We would like to thank M. Colavita, K. Rykoski, and N. Safizadeh for their contributions to this effort. Interferometer data was obtained at the Palomar Observatory using the NASA Palomar Testbed Interferometer, supported by NASA contracts to the Jet Propulsion Laboratory. We thank the staff of Palomar Observatory. M.W.M. acknowledges the support of the Michelson Graduate Fellowship program. B.F.L. acknowledges support from a Pappalardo Fellowship in Physics.
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
Michaelson Graduate FellowshipUNSPECIFIED
Pappalardo FellowshipUNSPECIFIED
Subject Keywords:Optical Interferometry, Phase-referencing, astrometry, PTI, binary star, kappa Pegasi, kappa Peg
Series Name:Proceedings of SPIE
Issue or Number:5491
DOI:10.1117/12.551980
Record Number:CaltechAUTHORS:20180910-131322294
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180910-131322294
Official Citation:Matthew W. Muterspaugh, Matthew W. Muterspaugh, Benjamin F. Lane, Benjamin F. Lane, Bernard F. Burke, Bernard F. Burke, Maciej Konacki, Maciej Konacki, Shri R. Kulkarni, Shri R. Kulkarni, } "Initial scientific results from phase-referenced astrometry of sub-arcsecond binaries", Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); doi: 10.1117/12.551980; https://doi.org/10.1117/12.551980
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89503
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:10 Sep 2018 20:42
Last Modified:16 Nov 2021 00:35

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