Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confp..68p&link_type=abstract
"The First Year of MAXI: Monitoring Variable X-ray Sources", Poster Presentations, 4th International MAXI Workshop held November
Astronomy and Astrophysics
Astronomy
Scientific paper
We will describe a Thomson X-ray polarimeter developed for a small satellite mission. The instrument works in the 5-30 keV band and will be suitable for X-ray polarisation measurement in about 50 hard X-ray sources. The accretion powered X-ray pulsars, black hole X-ray binaries, rotation powered pulsars and non-thermal SNR will be the prime targets for this mission. In spite of its moderate sensitivity, this experiment can give us unique opportunity to expand the field of X-ray astronomy into a hitherto unexplored dimension.
Ateequlla C. M.
Cowsik Ramanath
Devasia Jincy
Duraichelvan R.
Gopalakrishna Rao M.
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