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Double-wedged Wollaston-type polarimeter design and integration to RTT150-TFOSC; initial tests, calibration, and characteristics

机译:双楔Wollaston型旋光仪设计并集成到RTT150-TFOSC;初始测试,校准和特性

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摘要

Photometric and spectroscopic observation capabilities of 1.5-m Russian-Turkish Telescope RTT150 has been broadened with the integration of presented polarimeter. The well-known double-wedged Wollaston-type dual-beam technique was preferred and applied to design and produce it. The designed polarimeter was integrated into the telescope detector TFOSC, and called TFOSC-WP. Its capabilities and limitations were attempted to be determined by a number of observation sets. Non-polarized and strongly polarized stars were observed to determine its limitations as well as its linearity. An instrumental intrinsic polarization was determined for the 1 x 5 arcmin field of view in equatorial coordinate system, the systematic error of polarization degree as 0.2 %, and position angle as 1.9(a similar to). These limitations and capabilities are denoted as good enough to satisfy telescopes' present and future astrophysical space missions related to GAIA and SRG projects.
机译:1.5毫米俄罗斯-土耳其望远镜RTT150的光度学和光谱观察功能已通过集成偏振计得到了扩展。众所周知的双楔Wollaston型双光束技术是首选,并应用于设计和生产。设计的旋光仪已集成到望远镜探测器TFOSC中,称为TFOSC-WP。它的能力和局限性试图通过许多观察集来确定。观察到非极化和强极化的恒星,以确定其局限性和线性。赤道坐标系中1 x 5 arcmin视场的仪器固有极化被确定,极化度的系统误差为0.2%,位置角为1.9(近似)。这些局限性和能力被认为足以满足望远镜当前和未来与GAIA和SRG项目相关的天体太空任务。

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