Computer Science
Scientific paper
Feb 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998nasa.reptv....j&link_type=abstract
Technical Report, NASA/CR-1998-206867; NAS 1.26:206867
Computer Science
Computerized Simulation, Kolmogorov-Smirnov Test, Frequencies, Research, Procedures, X Ray Sources, Variability, Unsteady Flow, Sensitivity, Cygnus Constellation, Calibrating, Galactic Cosmic Rays
Scientific paper
This final report describes the research of a single common portion of the above-named two projects, conducted by G. Jernigan, i.e., the theory for a new method, a variation of a Kolmogorov-Smirnov test, for determining the fastest variability present in an X-ray source. The current phase involves testing the newly developed code on real example sources (CYG X1). Unfortunately, there are no calibration sources for testing the code, which therefore required the development of an X-ray source simulation code. The goal is to evaluate the sensitivity of the code for the detection of a range of different types of variability (bursts, pulsations, etc.).
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