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Conference on Ground-based Instrumentation for Astronomy Glasgow, SCOTLAND, JUN 21-25, 2004, Date: 2004/06/21 - 2004/06/25, Location: SCOTLAND, Glasgow

Publication date: 2004-01-01
Volume: 5492 Pages: 322 - 330
ISSN: 0-8194-5424-9
Publisher: Spie-int soc optical engineering; 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA

Ground-based instrumentation for astronomy, pts 1-3

Author:

Raskin, Gert
Van Winckel, Hans ; Davignon, Geert ; Moorwood, AFM ; Masanori, I

Keywords:

astronomical instrumentation, optical design, echelle spectrograph, optical fiber, extra-solar planets, Science & Technology, Technology, Physical Sciences, Engineering, Aerospace, Instruments & Instrumentation, Optics, Imaging Science & Photographic Technology, Spectroscopy, Engineering, EXTRA-SOLAR PLANETS, 4006 Communications engineering, 4009 Electronics, sensors and digital hardware, 5102 Atomic, molecular and optical physics

Abstract:

Hermes, a high-resolution fiber-fed echelle spectrograph is currently under development for the 1.2-meter Mercator Telescope at the Roque De Los Muchachos Observatory on La Palma. The optical design is based on a large R2.6 echelle grating, operating in quasi-Littrow and white-pupil configuration, and a double-prism cross-disperser. This instrument records the complete optical spectrum from 380 to 875 nm in one single exposure on a 2k x 4k CCD. Order separation is sufficiently large to record two interleaved spectra simultaneously through two 60-mum core fibers: one spectrum of the object and one of the nearby sky or, alternatively.. of a wavelength calibration lamp for high-precision radial velocity measurements. This type of observations also benefits from the high instrumental stability, owing to bench-mounting the spectrograph with a fixed configuration in a precisely temperature and humidity controlled chamber. Modest telescope size calls for high detection efficiency and great efforts in the design of both the fiber link and the spectrograph itself go in that direction. We aim at a peak-efficiency larger than 25% for the complete system. With a large fiber aperture of 2.3 arcsec. the resolving power lamda/deltalamda is 50000, a value that can be increased to 90000 with an adjustable slit at the fiber exit. This instrument mounted on a flexible telescope has a wide astronomical scope, going from asteroseismology to binary star research and chemical studies of stars and circumstellar material. We present the spectrograph design and we report on the project status.