A New Spectropolarimeter at the Dodaira Observatory
| Autor: | Koji S. Kawabata, Seiji Masuda, Ryuko Hirata, Masahiro Kondoh, Akira Okazaki, H. Akitaya, M. Seki, Nobuyuki Hirakata, Y. Ikeda |
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| Rok vydání: | 1999 |
| Předmět: | |
| Zdroj: | Publications of the Astronomical Society of the Pacific. 111:898-908 |
| ISSN: | 1538-3873 0004-6280 |
| DOI: | 10.1086/316387 |
| Popis: | We report a newly developed spectropolarimeter with a low‐dispersion resolution ( \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $R=40{\mbox{--}} 200$ \end{document} ) and a wide coverage in wavelength (400–900 nm). It is mainly used along with the 0.91 m telescope at the Dodaira Observatory of the National Astronomical Observatory, Japan. This instrument and the related reduction software are described briefly. The present polarimetric accuracy (rms) is estimated to be \documentclass{aastex} \usepackage{amsbsy} \usepac... |
| Databáze: | OpenAIRE |
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