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An Imaging Polarimeter(IMPOL) for multi-wavelength observations

机译:成像偏振计(IMPOL)用于多波长观测

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摘要

Taking advantage of the advances in array detector technology, an imaging polarimeter (IMPOL) has been constructed for measuring linear polarization in the wavelength band from 400-800~nm. It makes use of a Wollaston prism as the analyser to measure simultaneously the two orthogonal polarization components that define a Stoke's parameter. An achromatic half-wave plate is used to rotate the plane of polarization with respect to the axis of the analyser so that the second Stoke's parameter also can be determined. With a field of view correponding to about $30\times30 mm^2$ for a \diameter 1.2 m, f/13 telescope, a sensitive, liquid-N_2 cooled CCD camera as the detector and a built-in acquisition and guidance unit, the instrument can be used for studying stellar fields or extended objects with an angular resolution of $\sim 2 arcsec$. The instrumental polarization is less than 0.05% and the accuracies of measurement are primarily limited by photon noise for typical observations.
机译:利用阵列检测器技术的进步,构建了成像偏振计(IMPOL),用于测量400-800〜nm波段的线性偏振。它使用沃拉斯顿棱镜作为分析仪,同时测量定义斯托克参数的两个正交偏振分量。消色差半波片用于相对于检偏器的轴旋转偏振面,从而也可以确定第二斯托克参数。对于直径为1.2 m,f / 13的望远镜,对应的视场约为$ 30 \乘以30 mm ^ 2 $,一台灵敏的液态N_2冷却CCD照相机作为检测器,并内置了采集和制导单元,该仪器可用于研究恒星场或角度分辨率为\\ sim 2 arcsec $的扩展对象。仪器的偏振度小于0.05%,典型观测的测量精度主要受到光子噪声的限制。

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