Closed arjunsavel closed 3 years ago
This is due to the convention in pulsating variable star studies to call peak-to-peak magnitude difference the amplitude. What is the convention in the exoplanet community?
Pretty sure we use half peak-to-peak magnitude! It'd be fine to keep this magnitude implementation in, though, so long as it's documented as such.
In tossing a simple sine wave through the amplitude spectrum function, it seems as though it returns twice the amplitude at the given period. Potential bug, or have I missed something?