These are the directions, and the code I am working on currently.
- get timestamps, and average precision for each target.
- plot points, i.e.calculate the Keplerian orbit, f(t; P, e, om, Tp, msini), where msini is directly related to K, P, e and Mstar; see this
- plot another point some t later
- linear fit, save the slope (use this code)
- repeat 2) to 4) many times (in delta_v/delta_t array)
- multiply by sqrt(Nobs)/precision to get SN_simulated
- compare SN < SN_simulated for efficiency
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