New initiatives in optical astronomy at ARIES

Sagar, R. ; Kumar, Brijesh ; Omar, A. ; Pandey, A. K. (2010) New initiatives in optical astronomy at ARIES Interstellar Matter and Star Formation: A Multi-wavelength Perspective, ASI Conference Series, 1 . pp. 203-210.

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Official URL: http://www.ncra.tifr.res.in/~basi/asics_vol001

Abstract

The Institute is establishing a 3.6-m new technology modern optical telescope at Devasthal. This telescope will have instruments providing high resolution spectral and seeing-limited imaging capabilities at visible and near-infrared bands. In addition to optical studies of a wide variety of astronomical topics, it will be used for follow-up studies of sources identified in the radio region by GMRT and UV/X-ray by ASTROSAT. A few other facilities with very specific goals are also being established. These are 1.3-m optical telescope to monitor optically variable sources, a 0.5-m wide field (25 square degrees) Baker-Nunn Schmidt telescope to produce a digital map of the Northern sky at optical bands, and a 4-m liquid mirror telescope for deep sky survey of transient sources. These optical facilities with specialized back-end instruments are expected to become operational within the next few years. All the telescopes, except the 0.5-m Schmidt, will be located at Devasthal, Nainital in the central Himalayas.

Item Type:Article
Source:Copyright of this article belongs to Interstellar Matter and Star Formation: A Multi-wavelength Perspective, ASI Conference Series.
Keywords:Telescope; Optical: Instrumentation
ID Code:91960
Deposited On:25 May 2012 11:38
Last Modified:19 May 2016 05:34

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