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No more active galactic nuclei in clumpy disks than in smooth galaxies at z ~ 2 in CANDELS/3D-HST

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Nandra,  Kirpal
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Rosario,  David J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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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., Lotz, J., Maseda, M., Mozena, M., Nandra, K., Rosario, D. J., & Zeimann, G. R. (2014). No more active galactic nuclei in clumpy disks than in smooth galaxies at z ~ 2 in CANDELS/3D-HST. The Astrophysical Journal, 793(2):. doi:10.1088/0004-637X/793/2/101.


引用: https://hdl.handle.net/11858/00-001M-0000-0024-022F-A
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