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EUV Sources and Transients Detected by the Alexis Satellite

Published online by Cambridge University Press:  25 May 2016

D. Roussel-Dupré ,
T. Pfafman ,
J. Bloch  and
J. Theiler
D. Roussel-Dupré
Affiliation:
Los Alamos National Laboratory
T. Pfafman
Affiliation:
Stanford University
J. Bloch
Affiliation:
Los Alamos National Laboratory
J. Theiler
Affiliation:
Los Alamos National Laboratory

Extract

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Because ALEXIS is a spinning satellite, it is an ideal platform with which to study the time variability of the EUV cosmos. The main thrusts of this effort are to 1) detect EUV sources at known and unknown locations, 2) provide notification of transients in near real time to enable immediate follow-up from other observatories, and 3) create a time history of observed sources for comparison with previously published catalogs to aid in determining long duration variability from EUV sources.

Type
Part 2. Survey Projects
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 144 - 146
Copyright
Copyright © Kluwer 1998