Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.54

MLA

Yoshii, Yuzuru, et al. Potential Signature of Population III Pair-Instability Supernova Ejecta in the BLR Gas of the Most Distant Quasar at z = 7.54. 2022. EBSCOhost, https://doi.org/10.3847/1538-4357/ac8163.

APA

Yoshii, Y., Sameshima, H., Tsujimoto, T., Shigeyama, T., Beers, T. C., & Peterson, B. A. (2022). Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.54. https://doi.org/10.3847/1538-4357/ac8163

Chicago

Yoshii, Yuzuru, Hiroaki Sameshima, Takuji Tsujimoto, Toshikazu Shigeyama, Timothy C. Beers, and Bruce A. Peterson. 2022. “Potential Signature of Population III Pair-Instability Supernova Ejecta in the BLR Gas of the Most Distant Quasar at z = 7.54.” doi:10.3847/1538-4357/ac8163.