Parameters: 
 x : 1D array or sequence
Array or sequence containing the data.
 Fs : scalar
The sampling frequency (samples per time unit). It is used
to calculate the Fourier frequencies, freqs, in cycles per time
unit. The default value is 2.
 window : callable or ndarray
A function or a vector of length NFFT. To create window vectors see
window_hanning , window_none , numpy.blackman , numpy.hamming ,
numpy.bartlett , scipy.signal , scipy.signal.get_window , etc. The
default is window_hanning . If a function is passed as the argument,
it must take a data segment as an argument and return the windowed
version of the segment.
 sides : {'default', 'onesided', 'twosided'}
Specifies which sides of the spectrum to return. Default gives the
default behavior, which returns onesided for real data and both
for complex data. 'onesided' forces the return of a onesided
spectrum, while 'twosided' forces twosided.
 pad_to : int
The number of points to which the data segment is padded when
performing the FFT. This can be different from NFFT, which
specifies the number of data points used. While not increasing
the actual resolution of the spectrum (the minimum distance between
resolvable peaks), this can give more points in the plot,
allowing for more detail. This corresponds to the n parameter
in the call to fft(). The default is None, which sets pad_to
equal to NFFT
 NFFT : int
The number of data points used in each block for the FFT.
A power 2 is most efficient. The default value is 256.
This should NOT be used to get zero padding, or the scaling of the
result will be incorrect. Use pad_to for this instead.
 detrend : {'none', 'mean', 'linear'} or callable, default 'none'
The function applied to each segment before ffting, designed to
remove the mean or linear trend. Unlike in MATLAB, where the
detrend parameter is a vector, in Matplotlib is it a function.
The mlab module defines detrend_none ,
detrend_mean , and detrend_linear , but you can use a custom
function as well. You can also use a string to choose one of the
functions: 'none' calls detrend_none . 'mean' calls detrend_mean .
'linear' calls detrend_linear .
 scale_by_freq : bool, optional
Specifies whether the resulting density values should be scaled
by the scaling frequency, which gives density in units of Hz^1.
This allows for integration over the returned frequency values.
The default is True for MATLAB compatibility.
 mode : {'default', 'psd', 'magnitude', 'angle', 'phase'}
What sort of spectrum to use. Default is 'psd', which takes the
power spectral density. 'magnitude' returns the magnitude
spectrum. 'angle' returns the phase spectrum without unwrapping.
'phase' returns the phase spectrum with unwrapping.
 noverlap : int
The number of points of overlap between blocks. The
default value is 128.
 scale : {'default', 'linear', 'dB'}
The scaling of the values in the spec. 'linear' is no scaling.
'dB' returns the values in dB scale. When mode is 'psd',
this is dB power (10 * log10). Otherwise this is dB amplitude
(20 * log10). 'default' is 'dB' if mode is 'psd' or
'magnitude' and 'linear' otherwise. This must be 'linear'
if mode is 'angle' or 'phase'.
 Fc : int
The center frequency of x (defaults to 0), which offsets
the x extents of the plot to reflect the frequency range used
when a signal is acquired and then filtered and downsampled to
baseband.
 cmap
A matplotlib.colors.Colormap instance; if None, use
default determined by rc
 xextent : None or (xmin, xmax)
The image extent along the xaxis. The default sets xmin to the
left border of the first bin (spectrum column) and xmax to the
right border of the last bin. Note that for noverlap>0 the width
of the bins is smaller than those of the segments.
 **kwargs
Additional keyword arguments are passed on to imshow which makes
the specgram image.
