Abstract:
The Ultra Violet Imaging Telescope on ASTROSAT Satellite mission is a suite of Far Ultra Violet (FUV: 130 – 180
nm), Near Ultra Violet (NUV: 200 – 300 nm) and Visible band (VIS: 320–550nm) imagers. ASTROSAT is the multiwavelength
mission of ISRO. UVIT will image the sky simultaneously in three channels with a field of view diameter of
~ 28 arcminutes and an angular resolution < 1.8”. Two identical co-aligned telescopes (T1, T2) of Ritchey-Chretien
configuration (Primary mirror of ~375 mm diameter) collect the celestial radiation and feed the detector systems via a
selectable filter on a filter wheel mechanism; gratings are available in the filter wheels of FUV and NUV channels for
slitless low-resolution spectroscopy. The photon-counting detector system for each of the 3 channels is generically
identical. One of the telescopes images in the FUV channel, while the other images in NUV and VIS channels via a
beamsplitter. Images from the VIS channel are principally used for measuring drift, used in construction of images on the
ground by shift and add, and to reconstruct absolute aspect of the images. Adequate baffling has been provided for
reducing the scattered background from the Sun, earth albedo and other bright objects. The one-time opening mechanical
cover on each telescope also works as a Sun-shield after deployment.
We will present the overall (mechanical, optical and electrical) design of the payload.
