no code implementations • 11 Jan 2021 • A. Ellien, E. Slezak, N. Martinet, F. Durret, C. Adami, R. Gavazzi, C. R. Rabaça, C. Da Rocha, D. N. Epitácio Pereira
Large amounts of deep optical images will be available in the near future, allowing statistically significant studies of low surface brightness structures such as intracluster light (ICL) in galaxy clusters.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
no code implementations • 1 Mar 2019 • C. Yang, R. Gavazzi, A. Beelen, P. Cox, A. Omont, M. D. Lehnert, Y. Gao, R. J. Ivison, A. M. Swinbank, L. Barcos-Muñoz, R. Neri, A. Cooray, S. Dye, S. Eales, H. Fu, E. González-Alfonso, E. Ibar, M. J. Michałowski, H. Nayyeri, M. Negrello, J. Nightingale, I. Pérez-Fournon, D. A. Riechers, I. Smail, P. van der Werf
The reconstructed dust emission in the source plane is dominated by a compact disk with an effective radius of 0. 7kpc plus an overlapping extended disk with a radius twice as large.
Astrophysics of Galaxies
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