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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(462), p. 3591-3601

DOI: 10.1093/mnras/stw1882

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A new statistical model for Population III supernova rates: discriminating between ΛCDM and WDM cosmologies

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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