首页> 外文会议>Conference on adaptive optical systems technology >Analysis of off-axis Point Spread Function of Astronomical Adaptive Systems for the site of San Pedro Martir
【24h】

Analysis of off-axis Point Spread Function of Astronomical Adaptive Systems for the site of San Pedro Martir

机译:San Pedro Martir站点天文自适应系统的离轴点扩展功能分析

获取原文

摘要

A detailed analysis of anisotropy in the point spread function (PSF) associated with off-axis adaptive stronomical correction is presented. The results obtained are based on the experimental C_n~2 profile which has been recently measured at San Pedro Martir observatory (Mexico). It is found that the PSF has a complicated shpae that depends strongly on the wavelenght and on the separation between the guide and observed stars.
机译:提出了与轴外自适应天文校正相关的点扩展函数(PSF)中各向异性的详细分析。获得的结果基于最近在墨西哥圣佩德罗·马蒂尔天文台测量的实验C_n〜2剖面。发现PSF具有复杂的波形,这在很大程度上取决于波长和引导星与观测星之间的间隔。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号