van Leeuwen, I. F., Bouwens, R. J., van der Werf, P. P., Hodge, J. A., Schouws, S., Stefanon, M., . . . Schneider, R. (2024). Characterizing the contribution of dust-obscured star formation at $z \gtrsim$ 5 using 18 serendipitously identified [CII] emitters.
Chicago Style (17th ed.) Citationvan Leeuwen, I. F., et al. Characterizing the Contribution of Dust-obscured Star Formation at $z \gtrsim$ 5 Using 18 Serendipitously Identified [CII] Emitters. 2024.
MLA (9th ed.) Citationvan Leeuwen, I. F., et al. Characterizing the Contribution of Dust-obscured Star Formation at $z \gtrsim$ 5 Using 18 Serendipitously Identified [CII] Emitters. 2024.
Warning: These citations may not always be 100% accurate.