no code implementations • 8 Oct 2019 • FangXia An, J. M. Simpson, Ian Smail, A. M. Swinbank, Cong Ma, Daizhong Liu, P. Lang, E. Schinnerer, A. Karim, B. Magnelli, S. Leslie, F. Bertoldi, Chian-Chou Chen, J. E. Geach, Y. Matsuda, S. M. Stach, J. L. Wardlow, B. Gullberg, R. J. Ivison, Y. Ao, R. T. Coogan, A. P. Thomson, S. C. Chapman, R. Wang, Wei-Hao Wang, Y. Yang, R. Asquith, N. Bourne, K. Coppin, N. K. Hine, L. C. Ho, H. S. Hwang, Y. Kato, K. Lacaille, A. J. R. Lewis, I. Oteo, J. Scholtz, M. Sawicki, D. Smith
We identify multi-wavelength counterparts to 1, 147 submillimeter sources from the S2COSMOS SCUBA-2 survey of the COSMOS field by employing a recently developed radio$+$machine-learning method trained on a large sample of ALMA-identified submillimeter galaxies (SMGs), including 260 SMGs identified in the AS2COSMOS pilot survey.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
1 code implementation • 14 Sep 2017 • C. Yang, A. Omont, A. Beelen, Y. Gao, P. van der Werf, R. Gavazzi, Z. -Y. Zhang, R. Ivison, M. Lehnert, D. Liu, I. Oteo, E. González-Alfonso, H. Dannerbauer, P. Cox, M. Krips, R. Neri, D. Riechers, A. J. Baker, M. J. Michałowski, A. Cooray, I. Smail
The ratio between CO line luminosity and the dust mass appears to be slowly increasing with redshift for the SMGs, which need to be further confirmed.
Astrophysics of Galaxies
