sb2sep

Separate Stellar Component Spectra and Calculate Radial Velocities in SB2 Binary Systems

View the Project on GitHub jsinkbaek/sb2sep

Evaluating output

Note: The plots shown are slightly out-dated as of version 1.2.6. Currently, the RV routine shifts the template with the best RV guess to improve the quality of the calculated broadening function. As such, new plots will show all broadening function peaks aligning close to 0 if converged.

The evaluate_ssr_results module provides convenient ways to evaluate the raw data output from the spectral separation routine with similar plots to those provided during routine execution.

Load data

To load the raw data from the routine, the function load_routine_results can be used:

Input arguments:

Returns:

Plotting functions

plot_broadening_functions() input:

This function will create a single figure for each wavelength interval provided.

Example broadening function plot: Broadening function plot

plot_rv_and_separated_spectra() input:

Returns: fig, ax1, ax2, ax3

Example rv plot: RV plot

Next Page: Preparing spectra