The Space Telescope Imaging Spectrograph Design
| Autor: | S. Franka, J. B. Hutchings, Edward B. Jenkins, Chuck Bowers, D. Rose, Richard F. Green, Alan W. Delamere, M. Bottema, D. Hood, W. Meyer, Sara R. Heap, Morley M. Blouke, Charles L. Joseph, George F. Hartig, Fred L. Roesler, Lee Feinberg, Randy A. Kimble, Jeffrey L. Linsky, J. J. Loiacono, J. F. Grady, Albert Boggess, J. C. Hetlinger, David A. Dorn, H. Garner, Steven B. Kraemer, David Michika, Vic S. Argabright, C. Ludtke, B. E. Woodgate, Mark D. Brumfield, Theodore R. Gull, H. W. Moos, Anthony C. Danks, J. G. Timothy, C. VanHouten, Mary Elizabeth Kaiser, Donna Weistrop, R. Stocker, Robert A. Woodruff, D. J. Lindler, Stephen P. Maran, I. Becker, Richard L. Bybee, Joe H. Sullivan |
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| Rok vydání: | 1998 |
| Předmět: | |
| Zdroj: | Publications of the Astronomical Society of the Pacific. 110:1183-1204 |
| ISSN: | 1538-3873 0004-6280 |
| DOI: | 10.1086/316243 |
| Popis: | The Space Telescope Imaging Spectrograph (STIS) instrument was installed on the Hubble Space Telescope (HST) during the second servicing mission, in 1997 February. Four bands cover the wavelength range of 115–1000 nm, with spectral resolving powers between 26 and 200,000. Camera modes are used for target acquisition and deep imaging. Correction for HST's spherical aberration and astigmatism is included. The 115–170 nm range is covered by a CsI MAMA (Multianode Microchannel Array) detector and the 165–310 nm range by a Cs2Te MAMA, each with a format of \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}{\cy... |
| Databáze: | OpenAIRE |
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