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Cited article:

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Binary black hole mergers from population III stars: uncertainties from star formation and binary star properties

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Population III X-ray binaries and their impact on the early universe

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129 I and 247 Cm in meteorites constrain the last astrophysical source of solar r-process elements

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Formation of binary black holes similar to GW190521 with a total mass of ∼150 M⊙ from Population III binary star evolution

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