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Observing GRBs with the LOFT Wide Field Monitor
Published online by Cambridge University Press: 22 July 2013
Abstract
LOFT (Large Observatory For X-ray Timing) is one of the four candidate missions currentlyunder assessment study for the M3 mission in ESAs Cosmic Vision program to be launched in2024. LOFT will carry two instruments with prime sensitivity in the 2–30 keV range: a 10m2 class large area detector (LAD) with a <1° collimated field of viewand a wide field monitor (WFM) instrument. The WFM is based on the coded mask principle,and 5 camera units will provide coverage of more than 1/3 of the sky. The prime goal ofthe WFM is to detect transient sources to be observed by the LAD. With its wide field ofview and good energy resolution of <500 eV, the WFM will be an excellent instrumentfor detecting and studying GRBs and X-ray flashes. The WFM will be able to detect~150 gamma ray bursts per year, and a burst alert system will enable thedistribution of ~100 GRB positions per year with a ~1 arcmin locationaccuracy within 30 s of the burst.
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- © EAS, EDP Sciences 2013