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A decoding method of an n length binary BCH code through (n + 1)n length binary cyclic code
(2013-09-01)
For a given binary BCH code Cn of length n = 2s-1 generated by a polynomial g(x)e{open}F2[x] of degree r there is no binary BCH code of length (n + 1)n generated by a generalized polynomial g(x1/2)e{open}F2[x1/2ℤ ≥ 0] of ...
A decoding method of an n length binary BCH code through (n + 1)n length binary cyclic code
(2013-09-01)
For a given binary BCH code Cn of length n = 2s-1 generated by a polynomial g(x)e{open}F2[x] of degree r there is no binary BCH code of length (n + 1)n generated by a generalized polynomial g(x1/2)e{open}F2[x1/2ℤ ≥ 0] of ...
An investigation of low-mass-ratio EW systems from the Catalina Sky Survey
(SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, 2020)
We have conducted a survey of overcontact binary systems (EW) with mass ratio <= 0.25 from the Catalina Sky Survey (CSS) that are considered strong merger candidates and are probable progenitors of FK Com-type stars and ...
BINARIES AMONG DEBRIS DISK STARS
(2012-02-01)
We have gathered a sample of 112 main-sequence starswith known debris disks.We collected published information
and performed adaptive optics observations at Lick Observatory to determine if these debris disks are ...