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Proceedings Paper

Analysis of K-band imaging of the wide binary system σ CrB with the Lick Observatory NGS AO system
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Paper Abstract

We present astronomical results from K-band adaptive optics (AO) observations of the wide binary system σ Corona Borealis with the Lick Observatory natural guide star adaptive optics system on 2004 August 27-29. Seeing conditions were excellent and the AO compensation was very good, with Strehl ratios reaching 50% at times. The stellar images were reduced using three different analysis techniques: (1) Parametric Blind Deconvolution, (2) Multi-Frame Blind Deconvolution, and (3) the MATPHOT stellar photometry code. The relative photometric and astrometric precision achievable with these three analysis methods are compared. Future directions that this research can go towards achieving the goal of routinely obtaining precise and accurate photometry and astrometry based on near-infrared AO observations are described.

Paper Details

Date Published: 27 June 2006
PDF: 6 pages
Proc. SPIE 6272, Advances in Adaptive Optics II, 62720I (27 June 2006); doi: 10.1117/12.670574
Show Author Affiliations
Kenneth J. Mighell, National Optical Astronomy Observatory (United States)
Julian C. Christou, Ctr. for Adaptive Optics, Univ. of California, Santa Cruz (United States)
Jack D. Drummond, Air Force Research Lab. (United States)


Published in SPIE Proceedings Vol. 6272:
Advances in Adaptive Optics II
Brent L. Ellerbroek; Domenico Bonaccini Calia, Editor(s)

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