SeBa is a package of semi-analytical formulae which covers all phases of evolution from the zero-age main-sequence up to and including remnant phases. It is valid for masses in the range 0.01-1000 Msun with variable metallicity. SeBa includes prescriptions for mass loss by stellar winds, supernova and supports binary evolution.

See the following publications:

• Portegies Zwart S.F. & Verbunt F., 1996, A&A, 309, 179: "Population synthesis of high-mass binaries"
• Toonen, S., Nelemans, G., Portegies Zwart S.F., 2012, A&A, 546A, 70T: "Supernova Type Ia progenitors from merging double white dwarfs. Using a new population synthesis model"