Aims. This research note presents a full analysis of the CAFOS polarimeter mounted at the Calar Alto 2.2m telescope. It also provides future users of this mode with all necessary information to properly correct for instrumental effects in polarization data obtained with this instrument.
Methods. The standard stars BD+59d389 (polarized) and HD14069 (unpolarized) were observed with CAFOS in November, 2010, using 16 half-wave plate angles. The linear spectropolarimetric properties of CAFOS were studied using a Fourier Analysis of the resulting data.
Results. CAFOS shows a roughly constant instrumental polarization at the level of ~0.3% between 4000 and 8600 A. Below 4000 A the spurious polarization grows to reach ~0.7% at 3600 A. This instrumental effect is most likely produced by the telescope optics, and appears to be additive. The Wollaston prism presents a clear deviation from the ideal behavior. The problem is largely removed by the usage of at least 4 retarder plate angles. The chromatism of the half-wave plate causes a peak-to-peak oscillation of ~11 degrees in the polarization angle. This can be effectively corrected using the tabulated values presented in this paper. The Fourier analysis shows that the k!=0,4 harmonics are practically negligible between 3800 and 7400 A.
Conclusions. After correcting for instrumental polarization and retarder plate chromatism, with 4 half-wave plate angles CAFOS can reach an rms linear polarization accuracy of about 0.1%.
Solar Spectropolarimetry of Ca II $8542~Å$ Line: Polarimeter Development,Calibration and Preliminary Observations
色球磁场对于了解太阳大气中高能事件的动力学具有极其重要的意义。在科代卡纳尔太阳观测站,过去研制了几台偏振计,用于研究活动区的磁场。一台新的偏振计已经研制完成并安装在Kodaikanal塔-隧道望远镜上,用于研究Ca II $8542~Å$谱线中色球水平的活动区。仪器和旋光策略的设计方面进行了讨论。望远镜仪器的偏振已经被重新审视,并提出了减少偏振的可能方法。本文讨论了Zemax提出的用来检验分析仪器偏振模型的望远镜偏振模型。简要介绍了旋光仪控制单元和旋光仪操作软件。文中介绍了仪器的偏振定标、观测结果、仪器偏振改正和样品斯托克斯剖面。极化精度和灵敏度分别优于$3\times10^{-2}$和$3\times 10^{-3}$。
Hard X-Ray Focal-Plane Compton Spectro-Polarimeter: Detector Development and Sensitivity Evaluation
Physical Research Laboratory(物理研究实验室);INAF-IAPS(意大利国家天体物理研究所-空间天体物理研究所);Kavli Institute of Particle Astrophysics and Cosmology, Stanford University(斯坦福大学卡弗里粒子天体物理学与宇宙学研究所)
Development of ProtoPol: a medium resolution echelle spectro-polarimeter for PRL telescopes, Mt Abu, India -- Part I : the design, development and laboratory characterization
Physical Research Laboratory(物理研究实验室);Indian Institute of Technology, Gandhinagar(印度理工学院甘地纳加尔分校);I. Physikalisches Institut, Universität zu Köln(科隆大学第一物理研究所);Advanced Engineering Group, Azista Industries(阿齐斯塔工业公司先进工程组)
The Spectro-Polarimeter (SP) of the Andrei B. Severny Solar Tower Telescope (STT) at the Crimean Astrophysical Observatory: Optical Design and Implementation
Development of ProtoPol: a medium resolution echelle spectro-polarimeter for PRL telescopes, Mt Abu, India -- Part II : the data-reduction pipeline, on-sky characterization $\&$ performance verification and first science results
Astronomy and Astrophysics Division, Physical Research Laboratory(物理研究实验室天文与天体物理学部);Indian Institute of Technology, Gandhinagar(印度理工学院甘地纳加尔分校);I. Physikalisches Institut, Universität zu Köln(科隆大学第一物理研究所);Advanced Engineering Group, Azista Industries(Azista工业公司先进工程组)
Shaping SHAPE - A spectro-polarimeter onboard Chandrayaan-3 to observe Earth as an Exoplanet
ISRO Satellite Integration and Test Establishment (ISITE), U. R. Rao Satellite Centre (URSC), Indian Space Research Organisation (ISRO)(印度空间研究组织(ISRO)乌·拉·劳卫星中心(URSC)卫星集成与测试设施(ISITE))
The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III
National Astronomical Observatory of Japan(日本国立天文台);The Graduate University for Advanced Studies, SOKENDAI(高等研究院 (SOKENDAI));Department of Astronomy, Graduate School of Science, The University of Tokyo(东京大学大学院理学研究系天文学专攻)
Spectro-polarimetry of HAbitable Planet Earth (SHAPE) on Chandrayaan-3: Instrument characteristics, calibration and onboard performance
Space Astronomy Group, ISITE-Campus, U. R. Rao Satellite Centre(空间天文组,ISITE校园,U.R. Rao卫星中心);U. R. Rao Satellite Centre(U.R. Rao卫星中心);Laboratory for Electro-Optics Systems(光电系统实验室)