SIMBAD references

2009ApJ...692..924L - Astrophys. J., 692, 924-930 (2009/February-2)

Getting lucky with adaptive optics: fast adaptive optics image selection in the visible with a large telescope.

LAW N.M., MacKAY C.D., DEKANY R.G., IRELAND M., LLOYD J.P., MOORE A.M., ROBERTSON J.G., TUTHILL P. and WOODRUFF H.C.

Abstract (from CDS):

We describe the results from a new instrument which combines Lucky Imaging and adaptive optics (AO) to give the first routine direct diffraction-limited imaging in the visible on a 5 m telescope. With fast image selection and alignment behind the Palomar AO system we obtained Strehl ratios of 5%-20% at 700 nm in a typical range of seeing conditions, with a median Strehl of approximately 12% when 10% of the input frames are selected. At wavelengths around 700 nm the system gave diffraction-limited 35 mas full width at half-maxima (FWHMs). At 950 nm the output Strehl ratio was as high as 36% and at 500 nm the FWHM resolution was as small as 42 mas, with a low Strehl ratio but with resolution improved by a factor of ∼20 compared to the prevailing seeing. To obtain wider fields we also used multiple Lucky Imaging guide stars in a configuration similar to a ground layer AO system. With eight guide stars but very undersampled data we obtained 300 mas resolution across a 30'' x 30'' field of view in the i' band.

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Journal keyword(s): instrumentation: adaptive optics - instrumentation: high angular resolution - methods: data analysis - techniques: high angular resolution - techniques: image processing

Simbad objects: 3

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