Provide a name for this calculation
Stellar temperature
Stellar metallicity
Stellar log g
Magnitude of Stellar Target
Stellar Radius
Planet Radius
For phase curves, will derive duration of phase from input file.
Column 1: wavelength Column 2: flux, no header
Temperature (K)
Select Chemistry Type
Clouds or Scattering
Planet Mass
Column 1: wave or time Column 2: Model, no header
Primary or Secondary
Needed for secondary eclipse only
Define length of out of transit observing time
Or number of phase observations
Recommended to compute optimal groups per integration first (type "optimize"). But, you can also input any number from 2-65536.
Percent fullwell or number of electrons.
Column 1: wavelength Column 2: Noise Floor (ppm)
Constant Minimum Noise
