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The Ultra Fast Flash Observatory pathfinder – UFFO-p GRBimaging and location with its coded mask X-ray imager UBAT

Published online by Cambridge University Press:  22 July 2013

P.H. Connell ,
V. Reglero  and
on behalf of the UFFO collaboration
P.H. Connell
Affiliation:
University of Valencia, Spain
V. Reglero
Affiliation:
University of Valencia, Spain
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Abstract

The UFFO pathfinder mission will attempt to locate the optical afterglow of a GRB withinseconds of its detection and location by a wide field X-ray imager. It will be mounted onthe Lomonosov spacecraft for launch in 2013 and consists of a coded mask X-ray imager UBATto detect a GRB and estimate a direction vector which will be passed to the SMT opticalsystem which will rotate a moveable mirror to lock onto the GRB and direct the opticalafterglow to a camera with a  ~17′ wide aperture. We present the design geometry ofthe UBAT instrument only, with results of simulations for a range of GRB types to showprobable photon integration times to be expected to extract a significant FOV imagereconstruction and GRB location.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 61: Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe , 2013 , pp. 517 - 523
Copyright
© EAS, EDP Sciences 2013

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References

Jung, A., Ahamad, A.S., Barrillon, P., et al., 2012, Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory, Proceedings GRB 2012 Symposium (Marbella, Spain, Oct. 2012)