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Fig. A.2.
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Ten Gyr time-integrated number of SNIa per unit stellar mass formed. Same as Fig. 2, but with an SNIa progenitor mass range from 3 to 8 M⊙ for the primary star and 1.5 to 8 M⊙ for the secondary star instead of 3 to 8 M⊙ for both stars.
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