posted on 2017-11-21, 14:20authored byK. P. Singh, G. C. Dewangan, S. Chandra, S. Bhattacharayya, V. Chitnis, G. C. Stewart, N. J. Westergaard
The Soft X-ray focusing Telescope (SXT) is a moderate resolution
X-ray imaging spectrometer supplementing
the ultraviolet and hard X-ray payloads for broadband
studies of cosmic sources with AstroSat. Well
suited for observing bright X-ray sources, SXT observations
of nearby active galactic nuclei (AGN), binary
star systems with compact companions, active stars,
etc. are producing long soft X-ray light curves and
high-quality spectra. The strong X-ray variability and
multiple spectral components exhibited by SXT observations
of nearby Seyfert 1 galaxies show excellent
promise to probe accretion disks and central engines
in AGN through multi-band variability and spectroscopy.
History
Citation
Current Science, 2017, 113 (4), pp. 587-590 (4)
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Current Science
Publisher
Indian Academy of Sciences with Current Science Association