farr/GalClusterFitting
Fits a cluster of galaxies plus background.
A code to compute the secular dynamics of systems dominated by a central body.
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Fits a cluster of galaxies plus background.
Code for fitting autoregressive (moving average, too!) models to unevenly sampled series.
Code to model foreground and background rates from trigger data sets in two LIGO-like IFO's.
Selection Effects Model in Kepler