The adaptive optics Lorentzian point spread function
被引:23
作者:
Drummond, JD
论文数: 0引用数: 0
h-index: 0
机构:
USAF, Res Lab, Starfire Opt Range, Kirtland AFB, NM 87117 USAUSAF, Res Lab, Starfire Opt Range, Kirtland AFB, NM 87117 USA
Drummond, JD
[1
]
机构:
[1] USAF, Res Lab, Starfire Opt Range, Kirtland AFB, NM 87117 USA
来源:
ADAPTIVE OPTICAL SYSTEM TECHNOLOGIES, PARTS 1 AND 2
|
1998年
/
3353卷
关键词:
adaptive optics;
point spread function;
image analysis;
asteroids;
vesta;
D O I:
10.1117/12.321648
中图分类号:
O43 [光学];
学科分类号:
070207 ;
0803 ;
摘要:
A Lorentzian shaped point spread function (PSF) for adaptive optics is demonstrated. In some cases, a Lorentz atop an Airy pattern is a better description of the PSF. If the object can also be described with an analytic function, then Parametric Blind Deconvolution can be applied as a self referencing method to extract information about both the object and PSF simultaneously. The technique is used to derive the triaxial shape and rotational pole of the asteroid Vesta from observations made on the night of October 18, 1997, marking the first time the high order loop was closed for science with the Starfire Optical Range's 3.5m telescope.