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In the paper of Israel and Stella, 1996, they write:
"V0332+53 is a 4.4 s X–ray pulsar accreting from a Be star in a transient X–ray binary. Its
light curves are characterised by a pronounced red–noise type variability. The 4.4 s pulsations have a small amplitude...
Can somewone help me with understanding what frequency bin is?
Many strophysical papers use this notation, but i do not understand why i need a frequency bin, i would just Fourier transfom the series and look at the powers and decide what frequency belongs to my signal...
Now, when talking...
I need to find a linear filter to eliminate the power law noise from the signal: y=x+u, where x is the signal and u is the correlated noise of the 1/f^\alpha type.
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