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Anzahl der Publikationen: 3
Zeitschriftenartikel
Wilman, David J.; Fossati, Matteo; Mendel, J. Trevor; Saglia, Roberto; Wisnioski, Emily; Wuyts, Stijn; Schreiber, Natascha Foerster; Beifiori, Alessandra; Bender, Ralf; Belli, Sirio; Uebler, Hannah; Lang, Philipp; Chan, Jeffrey C. C.; Davies, Rebecca L.; Nelson, Erica J.; Genzel, Reinhard; Tacconi, Linda J.; Galametz, Audrey; Davies, Richard I.; Lutz, Dieter; Price, Sedona; Burkert, Andreas; Tadaki, Ken-ichi; Herrera-Camus, Rodrigo; Brammer, Gabriel; Momcheva, Ivelina und Dokkum, Pieter van
(2020):
The Regulation of Galaxy Growth along the Size-Mass Relation by Star Formation, as Traced by H alpha in KMOS3D Galaxies at 0.7 less than or similar to z less than or similar to 2.7.
In: Astrophysical Journal, Bd. 892, Nr. 1, 1
Belli, Sirio; Genzel, Reinhard; Förster Schreiber, Natascha M.; Wisnioski, Emily; Wilman, David J.; Wuyts, Stijn; Mendel, J. Trevor; Beifiori, Alessandra; Bender, Ralf; Brammer, Gabriel B.; Burkert, Andreas; Chan, Jeffrey; Davies, Rebecca L.; Davies, Ric; Fabricius, Maximilian; Fossati, Matteo; Galametz, Audrey; Lang, Philipp; Lutz, Dieter; Momcheva, Ivelina G.; Nelson, Erica J.; Saglia, Roberto P.; Tacconi, Linda J.; Tadaki, Ken-ichi; Übler, Hannah und Dokkum, Pieter van
(2017):
KMOS3D Reveals Low-level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7.
In: Astrophysical Journal Letters, Bd. 841, Nr. 1, L6
Wuyts, Eva; Wisnioski, Emily; Fossati, Matteo; Schreiber, Natascha M. Foerster; Genzel, Reinhard; Davies, Ric; Mendel, J. Trevor; Naab, Thorsten; Roettgers, Bernhard; Wilman, David J.; Wuyts, Stijn; Bandara, Kaushala; Beifiori, Alessandra; Belli, Sirio; Bender, Ralf; Brammer, Gabriel B.; Burkert, Andreas; Chan, Jeffrey; Galametz, Audrey; Kulkarni, Sandesh K.; Lang, Philipp; Lutz, Dieter; Momcheva, Ivelina G.; Nelson, Erica J.; Rosario, David; Saglia, Roberto P.; Seitz, Stella; Tacconi, Linda J.; Tadaki, Ken-ichi; Uebler, Hannah und Dokkum, Pieter van
(2016):
The evolution of metallicity and metallicity gradients from z=2.7 TO 0.6 with KMOS3D.
In: Astrophysical Journal, Bd. 827, Nr. 1, 74