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The X-ray telescope on board ASCAThe Advanced Satellite for Cosmology and Astrophysics (ASCA) instrument uses identical conical foil X-ray mirrors for its four telescopes. One of the major advantages of ASCA's telescopes is the first time ever use of X-ray imaging over a broad energy band and high throughput for conducting astronomical spectroscopy. Nested thin foil reflectors make possible a large effective area up to 10 keV, even under the tight weight restriction of the ASCA spacecraft. The expected characteristics of the ASCA mirrors are summarized based on ray tracings and pre-flight calibrations. The total effective area of four telescopes at 1 and 7 keV are approximately 1200 and 600 sq cm, respectively. The image size (half power diameter: HPD) is about 3 min. The field of view is 24 min and 16 min full width at half maximum for 1 and 7 keV, respectively. Observations of several X-ray sources from space during the performance verification phase have confirmed those performances as well as the alignment of the optical systems.
Document ID
19950050105
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Serlemitsos, Peter J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Jalota, Lalit
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Soong, Yang
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kunieda, Hideyo
(Nagoya University Nagoya, Japan)
Tawara, Yuzuru
(Nagoya University Nagoya, Japan)
Tsusaka, Yoshiyuki
(Nagoya University Nagoya, Japan)
Suzuki, Hisanori
(Nagoya University Nagoya, Japan)
Sakima, Yasuhiro
(Nagoya University Nagoya, Japan)
Yamazaki, Takashi
(Nagoya University Nagoya, Japan)
Yoshioka, Hidenori
(Nagoya University Nagoya, Japan)
Date Acquired
August 16, 2013
Publication Date
January 1, 1995
Publication Information
Publication: PASJ: Publications of the Astronomical Society of Japan
Volume: 47
Issue: 1
ISSN: 0004-6264
Subject Category
Astronomy
Accession Number
95A81704
Distribution Limits
Public
Copyright
Other

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