A high-resolution spectrograph for the 3.6-m Devasthal Optical Telescope of ARIES
Jeewan Chandra Pandey,
Aryabhatta Research Institute of Observational Sciences. Nainital, India 263001,
jeewan@aries.res.in
Jayshreekar Pant,
Aryabhatta Research Institute of Observational Sciences. Nainital, India 263001
Yogesh Chandra Joshi,
Aryabhatta Research Institute of Observational Sciences. Nainital, India 263001
Abstract
A high-resolution spectrograph for the 3.6-m Devasthal Optical Telescope (DOT) of Aryabhatta Reearch Institute of Observational Sciences (ARIES; Nainital, India) is envisaged to achieve the various science goals. The spectrograph will have two modes of spectral resolution (40 000 and 80 000) with a wavelength coverage of 380 - 900 nm. The design of the spectrograph will be similar to many contemporary high-resolution spectrometers in the world and will be based on a modern design using the white pupil concept. It will be a bench mounted fibre-fed spectrograph. In this article, we present the various science goals, technical specifications, and concept of design for the proposed spectrograph.
Keywords : spectrograph, optical band, high-resolution, echelle
Pour citer cet article
Jeewan Chandra Pandey, Jayshreekar Pant & Yogesh Chandra Joshi, «A high-resolution spectrograph for the 3.6-m Devasthal Optical Telescope of ARIES», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 88 - Année 2019, Actes de colloques, 2nd Belgo-Indian Network for Astronomy & Astrophysics (BINA) workshop - October 2018 - Brussels, Belgium, 43-54 URL : http://popups.ulg.be/0037-9565/index.php?id=8651.