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arxiv: 1901.08948 · v1 · pith:YLBCG2UAnew · submitted 2019-01-25 · 🌌 astro-ph.IM

Gamma-ray burst localisation strategies for the SPHiNX hard X-ray polarimeter

classification 🌌 astro-ph.IM
keywords sphinxlocalisationburstgamma-raypolarimeterpolarisationsensitivityuncertainty
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SPHiNX is a proposed gamma-ray burst (GRB) polarimeter mission operating in the energy range 50-600 keV with the aim of studying the prompt emission phase. The polarisation sensitivity of SPHiNX reduces as the uncertainty on the GRB sky position increases. The stand-alone ability of the SPHiNX design to localise GRB positions is explored via Geant4 simulations. Localisation at the level of a few degrees is possible using three different routines. This results in a large fraction (> 80%) of observed GRBs having a negligible (< 5%) reduction in polarisation sensitivity due to the uncertainty in localisation.

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