Wang, X., Cheng, C., Ge, J., Meng, X., Daddi, E., Yan, H., . . . Zhang, S. (2022). A strong He II $λ$1640 emitter with extremely blue UV spectral slope at $z=8.16$: Presence of Pop III stars?
Chicago Style (17th ed.) CitationWang, Xin, et al. A Strong He II $λ$1640 Emitter with Extremely Blue UV Spectral Slope at $z=8.16$: Presence of Pop III Stars? 2022.
MLA (9th ed.) CitationWang, Xin, et al. A Strong He II $λ$1640 Emitter with Extremely Blue UV Spectral Slope at $z=8.16$: Presence of Pop III Stars? 2022.
Warning: These citations may not always be 100% accurate.