Feldmann, R., Boylan-Kolchin, M., Bullock, J. S., Çatmabacak, O., Faucher-Giguère, C., Hayward, C. C., . . . Sun, G. (2024). Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency.
Chicago Style (17th ed.) CitationFeldmann, Robert, et al. Elevated UV Luminosity Density at Cosmic Dawn Explained by Non-evolving, Weakly Mass-dependent Star Formation Efficiency. 2024.
MLA (9th ed.) CitationFeldmann, Robert, et al. Elevated UV Luminosity Density at Cosmic Dawn Explained by Non-evolving, Weakly Mass-dependent Star Formation Efficiency. 2024.
Warning: These citations may not always be 100% accurate.