CANDELS z~2 galaxy properties

J. Trump (Creator)
G. Barro (Creator)
Stéphanie Juneau (Creator)
Benjamin J Weiner (Creator)
B. Luo (Creator)
Gabriel B. Brammer (Creator)
E. F. Bell (Creator)
W. N. Brandt (Creator)
Avishai Dekel (Creator)
Yicheng Guo (Creator)
Philip F. Hopkins (Creator)
D. C. Koo (Creator)
D. D. Kocevski (Creator)
D. H. McIntosh (Creator)
Ivelina Momcheva (Creator)
S. Faber (Creator)
H. C. Ferguson (Creator)
N. A. Grogin (Creator)
Jeyhan S. Kartaltepe (Creator)
A. M. Koekemoer (Creator)
J. Lotz (Creator)
Michael V. Maseda (Creator)
Mark Mozena (Creator)
K. Nandra (Creator)
David J. Rosario (Creator)
Gregory R. Zeimann (Creator)

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2014
No more active galactic nuclei in clumpy disks than in smooth galaxies at z ∼ 2 in candels/3D-HST
Trump, J. R., Barro, G., Juneau, S., Weiner, B. J., Luo, B., Brammer, G. B., Bell, E. F., Brandt, W. N., Dekel, A., Guo, Y., Hopkins, P. F., Koo, D. C., Kocevski, D. D., McIntosh, D. H., Momcheva, I., Faber, S. M., Ferguson, H. C., Grogin, N. A., Kartaltepe, J. & Koekemoer, A. M. & 6 others, Lotz, J., Maseda, M., Mozena, M., Nandra, K., Rosario, D. J. & Zeimann, G. R., Oct 1 2014, In: Astrophysical Journal. 793, 2, 101.
Research output: Contribution to journal › Article › peer-review

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