Open jradavenport opened 8 years ago
Progress has been made, my only problem is computing the cumulative flare energy distribution. Also, there is an issue with current rate calculation.
What's going on with the current rate calculation?
You get the (reverse) cumulative distribution by adding up the number of flares from smallest to biggest. Let's talk this week about this!
Here's the end-goal figure I want you to shoot for:
The "Flare Frequency Diagram" for your star with 2 sets of data plotted: the (newest) results from Appaloosa, and your by-hand FBEYE results.
The X-axis is the flare energy
The Y-axis is the cumulative flare rate (in number per day)
To make this figure in Python you'll need to do these steps (and probably more)
np.loadtxt
or similarThere is much more complication to this if we have long and short cadence data to combine...