The Small Satellite ``Tsubame'' for Polarimetry of GRBs

Details The Small Satellite ``Tsubame'' for Polarimetry of GRBs The Small Satellite ``Tsubame'' for Polarimetry of GRBs

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..355t&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 355-357

Astronomy and Astrophysics

Astrophysics

X-Ray Sources (Astronomical), Time Series, Satellites, Planetary, Mass, X-Ray Sources, X-Ray Bursts, Time Series Analysis, Time Variability, Satellite Orbits, Mass And Mass Distribution

Scientific paper

``Tsubame'' is a university-built small satellite mission that measures polarization of hard X-ray photons (30-100 keV) from gamma-ray bursts (GRB) using azimuthal angle anisotropy of Compton scattering. The satellite is intended for a piggy-back launch on the H-IIA rocket. It uses Control moment gyros to quickly orient itself to GRBs within 15 seconds from triggers. We are now developing the engineering model of the two detector systems on Tsubame, the polarimeter and the bust monitor. In this paper, we present an overview of the Tsubame mission, and detail of development of engineering model of our polarimeter and burst monitor.

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