Modeling of the Lobster-ISS x-ray telescope in orbit

dc.contributor.authorPeele, Andrew G.en
dc.contributor.authorLyngsjo, Hakanen
dc.contributor.authorCrocker, Roland Murleyen
dc.contributor.authorMarkham, Johnen
dc.contributor.authorBannister, Nigelen
dc.contributor.authorNugent, Keith A.en
dc.contributor.conferenceUV and Gamma-ray Space Telescope Systems (2004 : Glasgow, Scotland)en
dc.contributor.schoolSchool of Chemistry and Physics : Physics and Mathematical Physicsen
dc.date.issued2004en
dc.description©2004 COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.en
dc.description.abstractThe Lobster-ISS instrument is an X-ray all sky monitor proposed as an attached payload on the zenith platform exposed payload facility of the European Space Agency (ESA) Columbus module of the International Space Station (ISS). The basic instrument consists of six microchannel plate X-ray telescopes, collectively providing wide-angle (22.5 x 162 sq.degree) astronomical X-ray imaging in the 0.1 - 3.5 keV energy band. In this paper we describe computer modeling software underway at the University of Melbourne to provide an accurate simulation of the operation of the Lobster-ISS in its low Earth orbit environment. We exhibit some preliminary exposure maps and examples of the X-ray images that the instrument should produce given our simulation of its operation.en
dc.description.statementofresponsibilityAndrew G. Peele, Hakan Lyngsjo, Roland M. Crocker, John Markham, Nigel Bannister, Keith A. Nugenten
dc.identifier.citationProceedings of SPIE - The International Society for Optical Engineering, 2004; 5488, (1):232-241en
dc.identifier.doi10.1117/12.550975en
dc.identifier.urihttp://hdl.handle.net/2440/37095
dc.language.isoenen
dc.publisherSPIE - The International Society for Optical Engineeringen
dc.titleModeling of the Lobster-ISS x-ray telescope in orbiten
dc.typeConference paperen

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