Here is the code for calculating Quasi-Periodicity (Q) and Flux-Asymmetry (M) that we used in our work investigating the variability of young stellar objects in the North American Nebula. The interesting code/calculations of Q/M/etc. are in the ./results directory. We thank John Bredall for sharing an initial version of the code for Q that we modified for this work.
Misc. Notes:
- In our paper we adopted Q boundaries of
[0.45, 0.87]and M boundaries of[-0.25, 0.25].
