An imperfectly passive nature: bright submillimeter emission from dust-obscured star formation in the z = 3.717 'passive' system, ZF 20115

Simpson, J. M., Smail, Ian, Wang, Wei-Hao, Riechers, D., Dunlop, J. S., Ao, Y., Bourne, N., Bunker, A., Chapman, S. C., Chen, Chian-Chou, Dannerbauer, H., Geach, J. E., Goto, T., Harrison, C. M., Hwang, H. S., Ivison, R. J., Kodama, Tadayuki, Lee, C.-H., Lee, H.-M., Lee, M., Lim, C.-F., Micha?owski, M. J., Rosario, D. J., Shim, H., Shu, X. W., Swinbank, A. M., Tee, W.-L., Toba, Y., Valiante, Elisabetta, Wang, Junxian and Zheng, X. Z. 2017. An imperfectly passive nature: bright submillimeter emission from dust-obscured star formation in the z = 3.717 'passive' system, ZF 20115. Astrophysical Journal Letters 844 (1) , L10. 10.3847/2041-8213/aa7cf2

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Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Schools > Physics and Astronomy
Publisher:	American Astronomical Society
ISSN:	2041-8213
Date of First Compliant Deposit:	14 September 2017
Date of Acceptance:	15 June 2017
Last Modified:	13 May 2023 17:30
URI:	https://orca.cardiff.ac.uk/id/eprint/104669

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