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Type la supernovae (SNe Ia) are explosions of C+O WDs triggered by the accretion of material from a companion. After many years of SN research, we are fairly certain of the nature of the exploding object, but very little is still known about the companion star. In fact, it has been from long noticed that the companion does not leave its imprint on the explosion in a way which could allow us to identify the progenitor system. It is hoped that in the near future the various observational tests discussed along this conference will shed light into the identification issue.

SNe Ia: On the Binary Progenitors and Expected Statistics