Stellar continuum plus diskwind flux

After solving the problem with the velocity projections onto the line of sight, the next step was to add the full diskwind contribution to the stellar flux. I had to solve some small problems in the code, but nothing worth of note here. After some debugging and coding, I got my first line profile calculated with the 'Flux' code that contains the stellar continuum and the diskwind contribution.


Comparing this plot with the last post's plot, we can see that the wind contribution is far superior than the stellar continuum, but still we have a blue-shifted absorption feature, that is expected.