Annotation
The distribution function of an absolute maximum of the correlated stationary Gaussian sequence has been calculated. The final formula includes the Owen functions $T(c,a)$ tabulated for a wide range of possible values of the arguments $c$ and $a$. The main results are specified for computing abnormal errors in the search for the "astro-gravitational correlation".
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
A.V. Gusev
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia