Abstract
An algorithm is described that is intended for use in the analysis of data from the Extreme Ultraviolet Explorer (EUVE) satellite. An improved technique for detecting sources has been developed. This method is shown to be computationally simpler than non-linear methods and more sensitive to point sources than previous linear techniques, because it incorporates more information from the instrument point spread function. It is shown how simulated data help test this algorithm and are useful in the design of the satellite hardware.
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References
Bowyer, S., Malina, R. F., and Marshall, H. L. 1988, “The Extreme Ultraviolet Explorer Mission: Instrumentation and Science Goals,” in J.B.I.S. ,41, 357.
Cruddace, R. G., Hasinger, G. R., and Schmitt, J. H. M. M. 1988, “The Application of a Maximum Likelihood Analysis to Detection of Sources in the ROSAT Data Base,” in proceedings of the ESO conference on Astronomy from Large Databases, 177.
Marshall, H. L., Dobson, C.A., Malina, R. F., and Bowyer, S. 1987, “Analysis of Simulated Images from the Extreme Ultraviolet Explorer,” in proceedings of the International Topical Meeting on Image Detection and Quality ,ANRT and SPIE, 702, 275.
1988, “Plans for the Extreme Ultraviolet Explorer Data Base,” in proceedings of the ESO conference on Astronomy from Large Databases ,397.
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© 1989 Plenum Press, New York
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Marshall, H.L. (1989). Algorithms for the Analysis of Data from the Extreme Ultraviolet Explorer. In: Di Gesù, V., Scarsi, L., Crane, P., Friedman, J.H., Levialdi, S., Maccarone, M.C. (eds) Data Analysis in Astronomy III. Ettore Majorana International Science Series, vol 40. Springer, Boston, MA. https://doi.org/10.1007/978-1-4684-5646-2_19
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DOI: https://doi.org/10.1007/978-1-4684-5646-2_19
Publisher Name: Springer, Boston, MA
Print ISBN: 978-1-4684-5648-6
Online ISBN: 978-1-4684-5646-2
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