9–12 Oct 2018
Royal Observatory of Belgium
UTC timezone
<br>2nd BINA Workshop<br><br>BINA as an expanding international collaboration<P><img src="https://events.oma.be/indico/event/48/picture/0.jpg" width="279" height="75">

The High Resolution Spectrograph of the Aryabhatta Research Institute of Observational Sciences

9 Oct 2018, 16:30
40m
Meridian Room (Royal Observatory of Belgium)

Meridian Room

Royal Observatory of Belgium

Ringlaan 3, 1180 Brussels, Belgium
Invited Review 1. Instrumentation of the Indo-Belgian telescopes 1. Instrumentation of the Indo-Belgian Telescopes

Speaker

Dr Jeewan Pandey (Aryabhatta Research Institute of Observational Sciences)

Description

A high resolution spectrograph for recently installed 3.6-m Devasthal Optical Telescope (DOT) of the Aryabhatta Research Institute of Observational Sciences (ARIES) is envisaged as a key instrument to meet the spectroscopic requirements of the telescope. A committee of national and international experts recommended the key science program that can be taken up with the proposed instrument as asteroseisomology, Doppler imaging of spotted stars, abundances studies, spectroscopy and ground-based follow-up of exoplanets, and supernovae. The committee recommends the technical specification of the proposed instrument as follows: two mode of spectral resolution (40k and 80k), spectral coverage of 380-900 nm, and high throughput of ~20%. Further, the spectrograph should be able to record simultaneously the spectra of an object and/or sky. The spectrograph would be mounted on a vibration isolation table in a temperature controlled environment. The instrument has a fixed configuration with no moving parts ensuring a robust operation and easy maintenance. I aim to present current status of the proposed spectrograph during the talk.

Primary author

Dr Jeewan Pandey (Aryabhatta Research Institute of Observational Sciences)

Co-author

Dr Yogesh Joshi (Scientist ARIES)

Presentation materials