首页> 外文会议>Conference on Ground-based and Airborne Instrumentation for Astronomy >WALOP-South: A wide-field one-shot linear optical polarimeter for PASIPHAE survey
【24h】

WALOP-South: A wide-field one-shot linear optical polarimeter for PASIPHAE survey

机译:沃阿普南:帕斯皮亚调查的广泛单次线性光学偏振镜

获取原文

摘要

WALOP (Wide-Area Linear Optical Polarimetcr)-South, to be mounted on the 1m SAAO telescope in South Africa, is first of the two WALOP instruments currently under development for carrying out the PASIPHAE survey. Scheduled for commissioning in the year 2021, the WALOP instruments will be used to measure the linear polarization of around 106 stars in the SDSS-r broadband with 0.1 % polarimetric accuracy, covering 4000 square degrees in the Galactic polar regions. The combined capabilities of one-shot linear polarimetry, high polarimetric accuracy (< 0.1 %) and polarimetric sensitivity (< 0.05 %), and a large field of view (FOV) of 35 x 35 arcminutes make WALOP-South a unique astronomical instrument,. In a single exposure, it is designed to measure the Stokes parameters I, q and u in the SDSS-r broadband and narrowband filters between 500-700 nm. During each measurement, four images of the full field corresponding to the polarization angles of 0°, 45°, 90° and 135° will be imaged on four detectors and carrying out differential photometry on these images will yield the Stokes parameters. Major challenges in designing WALOP-South instrument include- (a) in the optical design, correcting for the spectral dispersion introduced by large split angle Wollaston Prisms used as polarization analyzers as well as aberrations from the wide field, and (b) making an optomechanical design adherent to the tolerances required to obtain good imaging and polarimetric performance under all temperature conditions as well as telescope pointing positions. We present the optical and optomechanical design for WALOP-South which overcomes these challenges.
机译:沃尔普(广域线性光学偏光极偏振电流)-South,安装在南非的1M萨安望远镜上,是目前正在开发的两个沃尔普仪器中的第一个开发,用于执行帕斯皮亚调查。预定在2021年的调试中,瓦片仪器将用于测量SDSS-R宽带中大约106颗恒星的线性极化,极化精度为0.1%,覆盖了银河极地区域的4000平方度。单次线性偏振物的组合能力,高偏振精度(<0.1%)和极化灵敏度(<0.05%),以及35 x 35 Arcminutes的大视野(FOV),使Walop-South是独特的天文仪器, 。在一次曝光中,它旨在测量SDSS-R宽带和窄带滤波器中的Stokes参数I,Q和U之间的速度。在每次测量期间,将在四个检测器上对应于0°,45°,90°和135°的偏振角对应的四个完整场的图像,并在这些图像上进行差分光度法将产生斯托克斯参数。在光学设计中设计的沃尔多 - 南风仪器包括 - (a)在光学设计中,校正由大型分角沃斯顿棱镜引入的光谱分子,用作偏振分析仪以及来自宽场的像差,(b)制造光学力学设计粘附在所有温度条件下获得良好的成像和偏振性能所需的公差以及望远镜指向位置。我们呈现了沃尔沃南的光学和光学力学设计,克服了这些挑战。

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