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NameSizeModeActions
array.cpython-35m-x86_64-linux-gnu.so533280755editdlrm
audioop.cpython-35m-x86_64-linux-gnu.so326400755editdlrm
binascii.cpython-35m-x86_64-linux-gnu.so259840755editdlrm
cmath.cpython-35m-x86_64-linux-gnu.so497600755editdlrm
fcntl.cpython-35m-x86_64-linux-gnu.so150720755editdlrm
grp.cpython-35m-x86_64-linux-gnu.so126560755editdlrm
math.cpython-35m-x86_64-linux-gnu.so423360755editdlrm
mmap.cpython-35m-x86_64-linux-gnu.so259680755editdlrm
nis.cpython-35m-x86_64-linux-gnu.so126080755editdlrm
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readline.cpython-35m-x86_64-linux-gnu.so287360755editdlrm
resource.cpython-35m-x86_64-linux-gnu.so118240755editdlrm
select.cpython-35m-x86_64-linux-gnu.so256160755editdlrm
spwd.cpython-35m-x86_64-linux-gnu.so125440755editdlrm
syslog.cpython-35m-x86_64-linux-gnu.so92480755editdlrm
termios.cpython-35m-x86_64-linux-gnu.so255360755editdlrm
unicodedata.cpython-35m-x86_64-linux-gnu.so8604400755editdlrm
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Edit: /opt/alt/python35/lib64/python3.5/lib-dynload/math.cpython-35m-x86_64-linux-gnu.so (42336B)
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It provides access to the mathematical functions defined by the C standard.acos(x) Return the arc cosine (measured in radians) of x.acosh(x) Return the inverse hyperbolic cosine of x.asin(x) Return the arc sine (measured in radians) of x.asinh(x) Return the inverse hyperbolic sine of x.atan(x) Return the arc tangent (measured in radians) of x.atan2(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.atanh(x) Return the inverse hyperbolic tangent of x.ceil(x) Return the ceiling of x as an Integral. This is the smallest integer >= x.copysign(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. cos(x) Return the cosine of x (measured in radians).cosh(x) Return the hyperbolic cosine of x.degrees(x) Convert angle x from radians to degrees.erf(x) Error function at x.erfc(x) Complementary error function at x.exp(x) Return e raised to the power of x.expm1(x) Return exp(x)-1. This function avoids the loss of precision involved in the direct evaluation of exp(x)-1 for small x.fabs(x) Return the absolute value of the float x.factorial(x) -> Integral Find x!. Raise a ValueError if x is negative or non-integral.floor(x) Return the floor of x as an Integral. This is the largest integer <= x.fmod(x, y) Return fmod(x, y), according to platform C. x % y may differ.frexp(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.fsum(iterable) Return an accurate floating point sum of values in the iterable. Assumes IEEE-754 floating point arithmetic.gamma(x) Gamma function at x.gcd(x, y) -> int greatest common divisor of x and yhypot(x, y) Return the Euclidean distance, sqrt(x*x + y*y).isclose(a, b, *, rel_tol=1e-09, abs_tol=0.0) -> bool 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.isfinite(x) -> bool Return True if x is neither an infinity nor a NaN, and False otherwise.isinf(x) -> bool Return True if x is a positive or negative infinity, and False otherwise.isnan(x) -> bool Return True if x is a NaN (not a number), and False otherwise.ldexp(x, i) Return x * (2**i).lgamma(x) Natural logarithm of absolute value of Gamma function at x.log(x[, base]) Return the logarithm of x to the given base. If the base not specified, returns the natural logarithm (base e) of x.log1p(x) Return the natural logarithm of 1+x (base e). The result is computed in a way which is accurate for x near zero.log10(x) Return the base 10 logarithm of x.log2(x) Return the base 2 logarithm of x.modf(x) Return the fractional and integer parts of x. Both results carry the sign of x and are floats.pow(x, y) Return x**y (x to the power of y).radians(x) Convert angle x from degrees to radians.sin(x) Return the sine of x (measured in radians).sinh(x) Return the hyperbolic sine of x.sqrt(x) Return the square root of x.tan(x) Return the tangent of x (measured in radians).tanh(x) Return the hyperbolic tangent of x.trunc(x:Real) -> Integral Truncates x to the nearest Integral toward 0. Uses the __trunc__ magic method.h hihi iii$ip1 )iP1 /i01 4i1@ :i0 \hP5 ?i0@ Ei 2 Sh05 %i0 *i0 Ji`- Ri3` Vi3 hp0 [iP0 ai00 fi@[ pi1@ bhp5 vi0Y h0S ip3@ h0K` hPI hG |i`G iG iF hD i`3 {h>` i 0 uhp= phP= i0; gh@7 i- 0i0 5i/@ i/ ;i/ @i/ i`,@ math.cpython-35m-x86_64-linux-gnu.so.debug.shstrtab.note.gnu.build-id.gnu.hash.dynsym.dynstr.gnu.version.gnu.version_r.rela.dyn.rela.plt.init.text.fini.rodata.eh_frame_hdr.eh_frame.ctors.dtors.jcr.data.rel.ro.dynamic.got.got.plt.data.bss.gnu_debuglink $oP(  0  8oEoxx`Th^@!@! h&&c''n**<tffz g gp mm4oo    ( (0 0     0