
Proceedings Paper
Infrared camera and spectrograph for the Subaru TelescopeFormat | Member Price | Non-Member Price |
---|---|---|
$14.40 | $18.00 |
![]() |
GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. | Check Access |
Paper Abstract
A 1-5 micrometers IR camera and spectrograph (IRCS) is described. The IRCS will be a facility instrument for the 8.2 m Subaru Telescope at Mauna Kea. It consists of two sections, a spectrograph and a camera section. The spectrograph is a cross-dispersed echelle that will provide a resolving power of 20,000 with a slit width of 0.15 arcsec and two-pixel sampling. The camera section serves as a slit viewer and as a camera with two pixel scales, 0.022 arcsec/pixel and 0.060 arcsec/pixel. Grisms providing 400-1400 resolving power will be available. Each section will utilize an ALADDIN II 1024 X 1024 InSb array. The instrument specifications are optimized for 2.2 micrometers using the adaptive optics and the tip-tilt secondary systems of the Subaru Telescope.
Paper Details
Date Published: 21 August 1998
PDF: 13 pages
Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); doi: 10.1117/12.317277
Published in SPIE Proceedings Vol. 3354:
Infrared Astronomical Instrumentation
Albert M. Fowler, Editor(s)
PDF: 13 pages
Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); doi: 10.1117/12.317277
Show Author Affiliations
Alan T. Tokunaga, Univ. of Hawaii/Manoa (United States)
Naoto Kobayashi, National Astronomical Observatory of Japan (United States)
James Bell, Univ. of Hawaii/Manoa (United States)
Gregory K. Ching, Univ. of Hawaii/Manoa (United States)
Klaus-Werner Hodapp, Univ. of Hawaii/Manoa (United States)
Joseph L. Hora, Univ. of Hawaii/Manoa and Harvard-Smithsonian Ctr. for Astrophysics (United States)
Doug Neill, Univ. of Hawaii/Manoa (United States)
Naoto Kobayashi, National Astronomical Observatory of Japan (United States)
James Bell, Univ. of Hawaii/Manoa (United States)
Gregory K. Ching, Univ. of Hawaii/Manoa (United States)
Klaus-Werner Hodapp, Univ. of Hawaii/Manoa (United States)
Joseph L. Hora, Univ. of Hawaii/Manoa and Harvard-Smithsonian Ctr. for Astrophysics (United States)
Doug Neill, Univ. of Hawaii/Manoa (United States)
Peter M. Onaka, Univ. of Hawaii/Manoa (United States)
John T. Rayner, Univ. of Hawaii/Manoa (United States)
Louis Robertson, Univ. of Hawaii/Manoa (United States)
David W. Warren, The Aerospace Corp. (United States)
Mark Weber, National Astronomical Observatory of Japan (United States)
Tony T. Young, Univ. of Hawaii/Manoa (United States)
John T. Rayner, Univ. of Hawaii/Manoa (United States)
Louis Robertson, Univ. of Hawaii/Manoa (United States)
David W. Warren, The Aerospace Corp. (United States)
Mark Weber, National Astronomical Observatory of Japan (United States)
Tony T. Young, Univ. of Hawaii/Manoa (United States)
Published in SPIE Proceedings Vol. 3354:
Infrared Astronomical Instrumentation
Albert M. Fowler, Editor(s)
© SPIE. Terms of Use
