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'4 =  H  h@hP@D`Xp,x X$ t < h \ p @ 0\ Pp 088T0P@pTh0Pp  0 ( D @H ` ,  0 @P`(@L`0@ @zRx $pFJ w?;*3$"Dȹ8\BxtL@&BED D(DP (D ABBF Y (C ABBG zRx P$P0$;BDA D@y  DABA zRx @$*@п BDG@ ABJ _ CBE  ABA zRx @ JlD h E T A  \D R A zRx  h0|sBFL DP  AABA zRx P$(D ` D (<P<dxD h E g A lxlD b A 8,BMN DHVPMHA@_  DBBA zRx @$74vBBA y BBE jBBzRx  $M40uBBA y BBE iBB,| BAA R ABA zRx  $X0L~BNA DP  AABD zRx P$uHdrAS A \zRx  BD0 A zRx 0 $0ZD P A L`H`BBB B(A0D8D`1 8D0A(B BBBA zRx `(1L BBH D(M0 (A BBBJ  (D BBBA zRx 0$ʳ= hdAQP AA L0BEB B(A0A8Gg 8D0A(B BBBH $zRx ,W  jAQ` AA zRx ` l  < 8D h E m A  D@ A zRx @qD AAQP  AA zRx P aP |ZD P A 4E  HF0V T k x0 ADD0u AAE FCA @ <$ 88 4 L 0b03 A NW0p  1AI  EE zRx    t pD@ A  4$ @`D@vHNPPHA@ A xy \ WpWqqqq#8H 0 PnМ؜o`  s (h!p ooo<o60F0V0f0v00000000011&161F1V1f1v11111111122&262F2V2f2v22222222233&363F3V3f3v333This module provides access to the mathematical functions defined by the C standard.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.asinh($module, x, /) -- Return the inverse hyperbolic sine of x.asin($module, x, /) -- Return the arc sine (measured in radians) of x.acosh($module, x, /) -- Return the inverse hyperbolic cosine of x.acos($module, x, /) -- Return the arc cosine (measured in radians) of x.isclose($module, /, a, b, *, rel_tol=1e-09, abs_tol=0.0) -- Determine whether two floating point numbers are close in value. rel_tol maximum difference for being considered "close", relative to the magnitude of the input values abs_tol maximum difference for being considered "close", regardless of the magnitude of the input values Return True if a is close in value to b, and False otherwise. For the values to be considered close, the difference between them must be smaller than at least one of the tolerances. -inf, inf and NaN behave similarly to the IEEE 754 Standard. That is, NaN is not close to anything, even itself. inf and -inf are only close to themselves.isinf($module, x, /) -- Return True if x is a positive or negative infinity, and False otherwise.isnan($module, x, /) -- Return True if x is a NaN (not a number), and False otherwise.isfinite($module, x, /) -- Return True if x is neither an infinity nor a NaN, and False otherwise.radians($module, x, /) -- Convert angle x from degrees to radians.degrees($module, x, /) -- Convert angle x from radians to degrees.pow($module, x, y, /) -- Return x**y (x to the power of y).hypot($module, x, y, /) -- Return the Euclidean distance, sqrt(x*x + y*y).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!. Raise a ValueError if x is negative or non-integral.fsum($module, seq, /) -- Return an accurate floating point sum of values in the iterable seq. Assumes IEEE-754 floating point arithmetic.floor($module, x, /) -- Return the floor of x as an Integral. This is the largest integer <= x.ceil($module, x, /) -- Return the ceiling of x as an Integral. This is the smallest integer >= x.gcd($module, x, y, /) -- greatest common divisor of x and ypq q/q9q>qXCq[IqX Nq[TqX`YpZYq[`_q0A9p=?q @@DqYwp[dqbhqbdpX@mqlsq@\@xqFqAp`\jpE pPNqhUp`@p]`'ql@Lp ZDp?3p=bpBqc-p9q^q Y qPS`pS@p_ p`b`pTJq@@OqY@q9UqYZqZ`q0BGCC: (Debian 10.2.1-6) 10.2.1 20210110.shstrtab.note.gnu.build-id.gnu.hash.dynsym.dynstr.gnu.version.gnu.version_r.rela.dyn.rela.plt.init.plt.got.text.fini.rodata.eh_frame_hdr.eh_frame.init_array.fini_array.data.rel.ro.dynamic.got.plt.data.bss.comment 88$o``(( @0 s8o<<EoTpp^Bh!h!(h00c 0 0n338w33p:}PnPn pp vvyyp МЌ؜،( r 0'Ǯ