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Edit: /opt/imh-python/lib/python3.9/lib-dynload/math.cpython-39-x86_64-linux-gnu.so (81560B)
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C_If(L9~ZK|HGL9uGDsf./L$zuL$HL/L$DfT0f.p/ff.E„ulH~f.f1AH^Yf(X\Xf(XH9\.fXf.QYL;d$tLL$"L$f(#H$dH3 %(Hĸ[]A\A]A^A_f.H<IHD$ HD$M(8 N.L;d$s1L;d$tLHD$苪HD$nf\cT$L$rT$L$Hf(-fT t.f.r>ff/wdD$ɧD$f!f.z.u,).H@f.zf/*-w苧!m-HHGAWAVAUATUSHHdH%(H$1Ht!HֹH=M6L#H[ID$uD$$HCD$ tLkM9l$I MLt$0Lt$(HD$E11DH;P kf.N,HG,D$HD$H|HGH;.P @H;P 趩f.,H+HD$l$1\f(fT,f.A_D$HD$A I9I|HGH;O 5wt$WDJ<#IHD$0HD$(MXH}+%K+f.d$GA踨HD$(@蕨H\|$|$èfDGfDf(fT|+f.*Efۺf.E„uyI~s8*f1f.A ^L$YHf(X\Xf(XI9\)fXf.QYL$L$L;t$(tL膦t$$t I,$+L$ t H+ D$fHH$dH3 %(HHH[]A\A]A^A_L;t$(tLT$$tI,$uLjf.D$ t H+1fDLxD$$IHwfHXD$ HHp|$$tI,$uL%=)|$DHL谣HL H5'1H80H1~fft$kܣL$L$5fDH~H;=QL ATUHSHH5M HHHFHHCt>H@8HHt1111H1HHHnH+It(L[]A\DE111HHH+IuH腢L[]A\D#UE1fDHG`HHIHuHEH5&HPH}K H81蓥iff.UHSHHK H9FH5 L HӢHHt[&HHC H@8HH111H1HHHFH+H[]DHH*f.z&zuD$D$Hu`'f(&fTf.v3H,ff(%%fUf(H*fTXfVH[]l@H1[]HHD$ˠHD$H[]E111HH& H=K f.\%z uáHHpitaunextafterintermediate overflow in fsummath.fsum partials-inf + inf in fsumpermk must not exceed %lldcombmath domain errormath range errorremaindercopysignatan2fmodpow(dd)ldexp(di)OO:logdist__ceil____floor__rel_tolabs_tolisclose__trunc__startprodmathacosacoshasinasinhatanatanhceildegreeserferfcexpm1fabsfactorialfloorfrexpgcdhypotisfiniteisinfisnanisqrtlcmlgammalog1plog10log2modfradianstrunculp0pThis module provides access to the mathematical functions defined by the C standard.hypot(*coordinates) -> value Multidimensional Euclidean distance from the origin to a point. Roughly equivalent to: sqrt(sum(x**2 for x in coordinates)) For a two dimensional point (x, y), gives the hypotenuse using the Pythagorean theorem: sqrt(x*x + y*y). For example, the hypotenuse of a 3/4/5 right triangle is: >>> hypot(3.0, 4.0) 5.0 x_7a(s(;LXww0uw~Cs+|g!tanh($module, x, /) -- Return the hyperbolic tangent of x.tan($module, x, /) -- Return the tangent of x (measured in radians).sqrt($module, x, /) -- Return the square root of x.sinh($module, x, /) -- Return the hyperbolic sine of x.sin($module, x, /) -- Return the sine of x (measured in radians).remainder($module, x, y, /) -- Difference between x and the closest integer multiple of y. Return x - n*y where n*y is the closest integer multiple of y. In the case where x is exactly halfway between two multiples of y, the nearest even value of n is used. The result is always exact.log1p($module, x, /) -- Return the natural logarithm of 1+x (base e). The result is computed in a way which is accurate for x near zero.lgamma($module, x, /) -- Natural logarithm of absolute value of Gamma function at x.gamma($module, x, /) -- Gamma function at x.fabs($module, x, /) -- Return the absolute value of the float x.expm1($module, x, /) -- Return exp(x)-1. This function avoids the loss of precision involved in the direct evaluation of exp(x)-1 for small x.exp($module, x, /) -- Return e raised to the power of x.erfc($module, x, /) -- Complementary error function at x.erf($module, x, /) -- Error function at x.cosh($module, x, /) -- Return the hyperbolic cosine of x.cos($module, x, /) -- Return the cosine of x (measured in radians).copysign($module, x, y, /) -- Return a float with the magnitude (absolute value) of x but the sign of y. On platforms that support signed zeros, copysign(1.0, -0.0) returns -1.0. atanh($module, x, /) -- Return the inverse hyperbolic tangent of x.atan2($module, y, x, /) -- Return the arc tangent (measured in radians) of y/x. Unlike atan(y/x), the signs of both x and y are considered.atan($module, x, /) -- Return the arc tangent (measured in radians) of x. The result is between -pi/2 and pi/2.asinh($module, x, /) -- Return the inverse hyperbolic sine of x.asin($module, x, /) -- Return the arc sine (measured in radians) of x. The result is between -pi/2 and pi/2.acosh($module, x, /) -- Return the inverse hyperbolic cosine of x.acos($module, x, /) -- Return the arc cosine (measured in radians) of x. The result is between 0 and pi.lcm($module, *integers) -- Least Common Multiple.gcd($module, *integers) -- Greatest Common Divisor.??@@8@^@@@@&AKAAA2A(;L4BuwsBuwB7Bs6Ch0{CZAC Ƶ;(DlYaRwNDAiAApqAAqqiA{DAA@@P@?CQBWLup#B2 B&"B补A?tA*_{ A]v}ALPEA뇇BAX@R;{`Zj@' @ulp($module, x, /) -- Return the value of the least significant bit of the float x.nextafter($module, x, y, /) -- Return the next floating-point value after x towards y.comb($module, n, k, /) -- Number of ways to choose k items from n items without repetition and without order. Evaluates to n! / (k! * (n - k)!) when k <= n and evaluates to zero when k > n. Also called the binomial coefficient because it is equivalent to the coefficient of k-th term in polynomial expansion of the expression (1 + x)**n. Raises TypeError if either of the arguments are not integers. Raises ValueError if either of the arguments are negative.perm($module, n, k=None, /) -- Number of ways to choose k items from n items without repetition and with order. 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Roughly equivalent to: sqrt(sum((px - qx) ** 2.0 for px, qx in zip(p, q)))fmod($module, x, y, /) -- Return fmod(x, y), according to platform C. x % y may differ.log10($module, x, /) -- Return the base 10 logarithm of x.log2($module, x, /) -- Return the base 2 logarithm of x.log(x, [base=math.e]) Return the logarithm of x to the given base. If the base not specified, returns the natural logarithm (base e) of x.modf($module, x, /) -- Return the fractional and integer parts of x. Both results carry the sign of x and are floats.ldexp($module, x, i, /) -- Return x * (2**i). This is essentially the inverse of frexp().frexp($module, x, /) -- Return the mantissa and exponent of x, as pair (m, e). m is a float and e is an int, such that x = m * 2.**e. If x is 0, m and e are both 0. Else 0.5 <= abs(m) < 1.0.trunc($module, x, /) -- Truncates the Real x to the nearest Integral toward 0. Uses the __trunc__ magic method.factorial($module, x, /) -- Find x!. 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