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2020RAA....20...32W - Research in Astron. and astroph., 20, 32-32 (2020/March-0)

The Coude Echelle Spectrograph for the Lijiang 1.8 m telescope.

WANG X.-L., CHANG L., WANG L., JI H.-X., XIAN H., TANG Z., XIN Y.-X., WANG C.-J., HE S.-S., ZHANG J.-J., LUN B.-L., WEI K., LI X.-Q., JIANG X.-J., WANG H.-J., LI H.-B. and MAO J.-R.

Abstract (from CDS):

The Coude Echelle Spectrograph (CES) was originally mounted on Xinglong 2.16 m telescope in 1994. When the High Resolution Fiber-fed Spectrograph (HRS) was commissioned at Xinglong 2.16 m telescope, the red path of CES was moved to Lijiang 1.8 m telescope, following some redesign and reinstallation. The CES of Lijiang 1.8 m telescope has the spectral resolution (R = λ/[?]λ) ranging from 20000 to 50000 corresponding to different slit widths. With a 2kx2k PI CCD, CES has a wavelength coverage between 570 nm to 1030 nm. In particular, the resolution of 37000 at 0.5 mm slit corresponds to 1.3'' on the sky. The limiting magnitude is V = 11.5 with the use of the tip-tilt feedback system, and the S/N is about 40 for 1 hour exposure at 600 nm (R = 37000). During the installation of CES, the tip-tilt mirror technology had successfully fulfilled high precision guiding and tracking for high resolution spectral observation and significantly improved the observation efficiency.

Abstract Copyright: © 2020 National Astronomical Observatories

Journal keyword(s): Instrumentation: spectrographs - methods: observational - techniques: spectroscopic

Simbad objects: 12

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