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Ultraviolet Imaging Telescope on AstroSat


Affiliations
1 Indian Institute of Astrophysics, Bengaluru 560 034, India
2 National Centre for Radio Astrophysics, Ganeshkhind, Pune 411 007, India
3 Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, B.C. V9E 2E7, Canada
 

The AstroSat satellite is designed for multi-wavelength astronomy for observations covering a spectral range from soft and hard X-rays to the ultraviolet. The Ultraviolet Imaging Telescope (UVIT) is the only non-X-ray telescope on AstroSat and it provides the long lever arm to the multi-wavelength observations. In addition to the simultaneous multi-wavelength studies in coordination with the X-ray telescopes on-board AstroSat, UVIT is used to study a large variety of objects with arcsecond-level spatial resolution. During the first year of observations, UVIT has obtained images in many filter bands in the wavelength range 130-300 nm over a field of ~28', which are being used to study a variety of hot stars, nebulae, stellar clusters and galaxies.

Keywords

Multi-Wavelength Astronomy, Ultraviolet Imaging Telescope, X-Ray Telescope.
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  • Morrissey, P. et al., The calibration and data products of Galex. ApJ. Suppl. Ser., 2007, 173, 682.

  • Tandon, S. N. et al., First results. J. Astrophys. Astron., 2017, 38, 28.

  • Srivastava, M. K., Prabhudesai, S. M. and Tandon, S. N., Studying the imaging characteristics of ultra violet imaging telescope (UVIT) through numerical simulations. Publ. Astron. Pacific, 2009, 121, 621.

  • Subramaniam, A. et al., A hot comparison to a blue straggler in NGC 188 as revealed by the ultra-violet imaging telescope (UVIT) on AstroSat. Astrophys. J. Lett., 2016, 833, L27.


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  • Ultraviolet Imaging Telescope on AstroSat

Abstract Views: 277  |  PDF Views: 97

Authors

S. N. Tandon
Indian Institute of Astrophysics, Bengaluru 560 034, India
S. K. Ghosh
National Centre for Radio Astrophysics, Ganeshkhind, Pune 411 007, India
J. Hutchings
Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, B.C. V9E 2E7, Canada
C. S. Stalin
Indian Institute of Astrophysics, Bengaluru 560 034, India
A. Subramaniam
Indian Institute of Astrophysics, Bengaluru 560 034, India

Abstract


The AstroSat satellite is designed for multi-wavelength astronomy for observations covering a spectral range from soft and hard X-rays to the ultraviolet. The Ultraviolet Imaging Telescope (UVIT) is the only non-X-ray telescope on AstroSat and it provides the long lever arm to the multi-wavelength observations. In addition to the simultaneous multi-wavelength studies in coordination with the X-ray telescopes on-board AstroSat, UVIT is used to study a large variety of objects with arcsecond-level spatial resolution. During the first year of observations, UVIT has obtained images in many filter bands in the wavelength range 130-300 nm over a field of ~28', which are being used to study a variety of hot stars, nebulae, stellar clusters and galaxies.

Keywords


Multi-Wavelength Astronomy, Ultraviolet Imaging Telescope, X-Ray Telescope.

References





DOI: https://doi.org/10.18520/cs%2Fv113%2Fi04%2F583-586