How do I calculate Allan Variance (maybe for pulsars)?
So, after some discussion and paper reading I learned of the sigma_z calculation in this paper by Matsakis, Taylor, and Eubanks. Several astronomers recommended this to me. I was also told to try out Stable32, although I'm not sure if that will work for pulsars. The code for a sigma_z calculation can be found here: sigma_z calculation. I believe this is the best method for doing what I asked.