I'd be curious to know how PACMAN combines the individual models (constant, model_ramp, transit etc) to give the the full model. There are different ways one can combine systematics and astrophysical models, so it'd be great to point out in the documentation how PACMAN does this.
I'd be curious to know how PACMAN combines the individual models (constant, model_ramp, transit etc) to give the the full model. There are different ways one can combine systematics and astrophysical models, so it'd be great to point out in the documentation how PACMAN does this.