Author/Authors :
Soffitta، نويسنده , , P. and Baldini، نويسنده , , L. and Bellazzini، نويسنده , , R. and Brez، نويسنده , , A. and Costa، نويسنده , , E. and Di Persio، نويسنده , , G. and Latronico، نويسنده , , L. and Omodei، نويسنده , , N. and Pacciani، نويسنده , , L. and Spandre، نويسنده , , G.، نويسنده ,
Abstract :
Polarimeters flown so far were based on the Thomson scattering and Bragg diffraction with intrinsically limited sensitivity. In the present paper, we review the experiments based on those techniques and discuss possible optimization and implementation for X-ray astronomy.
Keywords :
?-Ray , Polarimeters in astronomy , X-Ray , Detectors
