Analytical vs Physical Scaling#
When ForMoSA evaluates the likelihood, it compares a transformed model spectrum to the observed flux. Part of that transformation is a scaling step that brings the model to the same flux level as the data. ForMoSA offers two approaches.
Physical scaling: r + d#
Physical scaling applies the inverse-square law:
where r is the companion radius in Jupiter radii and d is the distance in
parsecs. This scaling is physically motivated and lets you retrieve the radius
as a free parameter.
from ForMoSA.config.global_config import ConfigParameters
config_parameters = ConfigParameters(
par1 = ["uniform", "800", "2000"], # Teff
par2 = ["uniform", "3.0", "5.5"], # log g
r = ["uniform", "0.5", "3.0"], # radius (R_Jup) — free
d = ["constant", "27.7"], # distance fixed to Gaia value (pc)
)
Use physical scaling when:
Your flux calibration is reliable (flux-calibrated spectrum or photometry).
You want to constrain the companion’s physical radius.
You can fix the distance (e.g. from Gaia parallax).
Analytical scaling: alpha#
Analytical scaling multiplies the model by a constant factor:
This is a pure nuisance parameter: it absorbs any flux-level offset without making any physical claim about the radius or distance.
from ForMoSA.config.global_config import ConfigParameters
config_parameters = ConfigParameters(
par1 = ["uniform", "800", "2000"],
par2 = ["uniform", "3.0", "5.5"],
alpha = ["uniform", "0.0", "10.0"], # free scaling factor
# r and d are NOT set
)
Use analytical scaling when:
The absolute flux calibration of your data is uncertain.
You are fitting contrast spectra (e.g. from integral-field unit observations) where the flux level is not physically meaningful.
You want a quick exploratory fit without committing to a radius prior.
Side-by-side comparison#
Physical ( |
Analytical ( |
|
|---|---|---|
Physical meaning |
Yes — retrieves radius |
No — nuisance parameter |
Requires distance |
Yes (can be fixed) |
No |
Requires flux calibration |
Yes |
No |
Adds free parameter? |
Yes ( |
Yes ( |
Recommended for |
Photometry, flux-calibrated spectra |
Contrast spectra, exploratory fits |
Combining both#
You can set both r+d and alpha simultaneously — in that case ForMoSA
applies the physical scaling first and then multiplies by alpha. This is
occasionally useful when testing for residual systematic offsets on top of a
physical model, but in most cases you should pick one or the other.