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
1) There are separate calculations for the short and long wavelength channels even though these observations occur simultaneously. Take caution to use the same Instrument Setup and Detector Setup in both the SW Grism Time Series and LW Grism Time Series calculations for a given target to correctly evaluate expected SNR.
2) SW Filter wavelength ranges cited in the dropdown menu are only for guidance. The exact numbers dependt on the choice of LW filter (see JDOX Table 3)
Order to run calculation on. If optimizing number of groups, we recommend optimizing for Order 1 first, and using that optimum for the Order 2 calculations.
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
