Characterizing the contribution of dust-obscured star formation at $z\gtrsim$ 5 using 18 serendipitously identified [CII] emitters

I. F. van Leeuwen, R. J. Bouwens, P. P. van der Werf +24

We present a new method to determine the star formation rate (SFR) density of the Universe at $z\gtrsim 5$ that includes the contribution of dust-obscured star formation. For this…