KMOS 3D Reveals Low-level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z

KMOS 3D Reveals Low-level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7

Published:2017-05-17 Issue:1 Volume:841 Page:L6
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Belli Sirio^ORCID,Genzel Reinhard^ORCID,Förster Schreiber Natascha M.,Wisnioski Emily,Wilman David J.^ORCID,Wuyts Stijn^ORCID,Mendel J. Trevor^ORCID,Beifiori Alessandra,Bender Ralf^ORCID,Brammer Gabriel B.^ORCID,Burkert Andreas^ORCID,Chan Jeffrey,Davies Rebecca L.,Davies Ric,Fabricius Maximilian,Fossati Matteo^ORCID,Galametz Audrey,Lang Philipp^ORCID,Lutz Dieter,Momcheva Ivelina G.^ORCID,Nelson Erica J.,Saglia Roberto P.^ORCID,Tacconi Linda J.^ORCID,Tadaki Ken-ichi^ORCID,Übler Hannah,van Dokkum Pieter^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aa70e5/pdf

Reference52 articles.

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3. STELLAR POPULATIONS FROM SPECTROSCOPY OF A LARGE SAMPLE OF QUIESCENT GALAXIES ATZ> 1: MEASURING THE CONTRIBUTION OF PROGENITOR BIAS TO EARLY SIZE GROWTH

4. MOSFIRE SPECTROSCOPY OF QUIESCENT GALAXIES AT 1.5

5. ONE PLANE FOR ALL: MASSIVE STAR-FORMING AND QUIESCENT GALAXIES LIE ON THE SAME MASS FUNDAMENTAL PLANE ATz∼ 0 ANDz∼ 0.7

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