Hi,
I have masses and radii estimates of an eclipsing binary system using radial velocities and light curves.
I have my ini file (which I load to the BinaryStarModel) the following way:
mass_0 = 2.834,0.12
mass_1 = 2.612,0.1
radius_0 = 1.749,0.05
radius_1 = 1.805,0.05
B = 9.92,0.05
V = 9.6,0.05
J = 9.0,0.04
H = 8.88,0.04
K = 8.84,0.04
parallax= 3.2241, 0.02
After fitting for ages, when I try to do BinaryStarModel.corner_observed(), I only see the fluxes and parallax.
How can I check if my masses and radii are being used in the fitting procedure?
Hi, I have masses and radii estimates of an eclipsing binary system using radial velocities and light curves. I have my ini file (which I load to the
BinaryStarModel
) the following way:After fitting for ages, when I try to do
BinaryStarModel.corner_observed()
, I only see the fluxes and parallax.How can I check if my masses and radii are being used in the fitting procedure?
Thanks in advance.