Point spread function deconvolution of an Atmospheric Cherenkov Telescope

被引：0

作者：

Kenny, G. E. ^{[1
]}

Gillanders, G. H. ^{[1
]}

Lang, M. J. ^{[1
]}

机构：

[1] Natl Univ Ireland Univ Coll Galway, Dept Phys, Galway, Ireland

来源：

Proceedings of the 29th International Cosmic Ray Conference, Vol 5: OG 2.5, 2.6 & 2.7 | 2005年

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The effect of iteratively deconvolving Imaging Atmospheric Cherenkov Telescope (IACT) images is investigated here with the aim of exploiting the full resolution of an IACT photomultipher tube camera. The Richardson-Lucy method of de-blurring images was chosen for the study as it functions effectively in the presence of noise. After the Richardson-Lucy algorithm was integrated into the analysis software, the procedure was tested using Crab Nebula data collected with the Whipple 10m IACT. Using the measured Point Spread Function (PSF) of the instrument with the Richardson-Lucy subroutine, Cherenkov images were iteratively deconvolved. Following this, a full re-optimisation of picture and boundary thresholds and image selection parameters was carried out in an attempt to enhance the detected signal. The improvement in signal using this method was not statistically significant.

引用

页码：279 / 282

页数：4

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