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SIRPOL: a JHK_s-simultaneous imaging polarimeter for the IRSF 1.4-m telescope

机译:SIRPOL:用于IRSF 1.4-M望远镜的JHK_S-同时成像偏振仪

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We describe a polarimeter for the near-infrared camera SIRIUS mounted on the IRSF 1.4 m telescope in South Africa. The polarimeter, SIRPOL, consists of an achromatic (1 - 2.5 μm) wave plate rotator unit and a polarizer located upstream of the camera, both of which are at a room temperature. This minimizes the effect of the mirrors in the camera on instrumental polarization. The combination of the polarimeter with the SIRIUS camera enables a deep (J = 19.2 mag, 5σ in one hour) and wide-field (7.7' x 7.7') imaging polarimetry at JHK_s simultaneously. The three color near-infrared polarimetry is useful for understanding the properties of dust grains that cause scattering and absorption in various environments (e.g., star forming regions, late-type stars, and galaxies). Using IRSF and SIRPOL, wide-field near-infrared polarization surveys in various star-forming regions are being conducted, starting from 2006, which aim to study both reflection nebulae associated with young stars and interstellar polarizations of background stars. In this contribution, we describe the hardware and software of SIRPOL and report its first results on the telescope.
机译:我们描述了近红外摄像头Sirius的偏振仪,安装在南非的IRSF 1.4米望远镜上。偏振仪SiRPOL包括一个消色差(1-2.5μm)波片旋转器单元和位于照相机上游的偏振器,两者都在室温下。这最大限度地减少了仪器极化上相机中的镜子的效果。偏振仪与Sirius相机的组合使得能够在JHK_S同时在JHK_S上进行深度(J = 19.2mag,5σ)和宽场(7.7'x 7.7')偏振。三种颜色的近红外偏振物可用于理解导致各种环境中的散射和吸收的尘颗粒的性质(例如,星形成形区域,晚期型恒星和星系)。使用IRSF和SIRPOL,从2006年开始,正在进行各种恒星形成区域的广泛近红外极化调查,这旨在研究与幼颗星和背景星星偏振相关的反射星云。在这一贡献中,我们描述了Sirpol的硬件和软件,并在望远镜上报告其第一个结果。

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