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Table B.2

Multipliers to calculate self-bias correction for ISPH from the values of Table B.1.

f1 f1 f1 f4 f5 f6 f7 f8 f9
O32 1.007 1.003 1.003 1.0 0.999 0.999 0.996 0.996 0.995
O64 1.005 0.999 1.0 0.999 0.999 0.998 0.996 0.997 0.995
O128 1.004 0.998 0.999 0.999 0.998 0.996 0.995 0.997 0.996
O256 1.004 1.0 0.999 0.999 0.998 0.998 0.998 0.998 0.998
OI,32 1.019 0.979 0.992 0.970 0.886 0.803 0.714 0.341 0.088
OI,64 1.007 1.001 1.002 1.001 1.0 0.999 0.996 0.997 0.996
OI,128 1.005 1.0 1.0 1.0 1.0 1.041 0.996 0.997 0.996
OI,256 1.005 1.0 1.0 1.0 1.0 0.999 0.997 0.998 0.996
C2 1.005 0.996 0.995 0.994 0.988 0.998 0.998 0.996 0.997
C4 0.963 0.997 0.997 0.999 0.999 0.998 1.0 0.999 0.999
C6 0.973 0.997 0.998 1.0 1.0 1.0 1.0 1.0 1.0
C8 0.974 0.998 0.999 0.999 1.0 1.0 1.0 1.0 1.0
WU2 0.978 0.990 0.987 0.956 0.937 0.895 0.853 0.693 0.363
WU4 1.003 0.998 0.998 0.997 0.997 0.993 0.994 0.995 0.993
CM04 0.981 0.975 0.910 0.806 0.719 0.557 0.395 0.1 x
CM05 0.976 1.0 1.0 1.0 0.998 0.999 0.997 0.998 0.997
BUH 0.970 0.996 0.997 0.998 0.994 0.999 0.998 0.998 0.998

Notes. Correction to self-bias for ISPH is given by using (fici) instead of ci in Eq. B.2. In general the kernels with ISPH have very similar self-bias coefficients to that of GDSPH, but one can see that some kernels in ISPH become increasingly unstable as Nsmooth increases, such as CM04, WU2, and OI,32, and their behavior diverges from the others, which otherwise converges to roughly 1.

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