Two Remarkably Luminous Galaxy Candidates at z ≈ 10–12 Revealed by JWSTRohan P. Naidu, Andrea Weibel, D. Magee et al.|The Astrophysical Journal Letters|2022Cited by 429
DIRECT MEASUREMENTS OF DUST ATTENUATION IN<i>z</i>∼ 1.5 STAR-FORMING GALAXIES FROM 3D-HST: IMPLICATIONS FOR DUST GEOMETRY AND STAR FORMATION RATESSedona H. Price, Stijn Wuyts, Mariska Kriek et al.|The Astrophysical Journal|2014Cited by 204
The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with KMOS<sup>3D</sup> <sup>∗</sup>Hannah Übler, Stijn Wuyts, R. Genzel et al.|The Astrophysical Journal|2019Cited by 169
(untitled)N. M. Förster Schreiber, Hannah Übler, R. Genzel et al.|Research at the University of Copenhagen (University of Copenhagen)|0Cited by 152
The KMOS<sup>3D</sup> Survey: Data Release and Final Survey Paper*Emily Wisnioski, Eva Wuyts, N. M. Förster Schreiber et al.|The Astrophysical Journal|2019Cited by 146