no code implementations • 3 Mar 2021 • Delaney A. Dunne, Tracy M. A. Webb, Allison Noble, Christopher Lidman, Heath Shipley, Adam Muzzin, Gillian Wilson, H. K. C. Yee
We find these galaxies have molecular gas masses of $0. 7-11. 0\times 10^{10}\ \mathrm{M}_\odot$, comparable to other BCGs in this redshift range, and specific star formation rates which trace the Elbaz et al. (2011) Main Sequence.
Astrophysics of Galaxies
no code implementations • 9 Nov 2020 • Paolo Saracco, Danilo Marchesini, Francesco La Barbera, Adriana Gargiulo, Marianna Annunziatella, Ben Forrest, Daniel J. Lange Vagle, Z. Cemile Marsan, Adam Muzzin, Mauro Stefanon, Gillian Wilson
The analysis of its spectrum shows that this galaxy, hosting an AGN, formed and assembled $\sim$2$\times$10$^{11}$ M$_\odot$ shaping its morphology within the $\sim$600 Myr preceding the observations, since $z$$\sim$4. 6.
Astrophysics of Galaxies
1 code implementation • 6 Feb 2015 • Henk Hoekstra, Ricardo Herbonnet, Adam Muzzin, Arif Babul, Andisheh Mahdavi, Massimo Viola, Marcello Cacciato
Nonetheless we find that the uncertainty in the determination of photometric redshifts is the largest source of systematic error for our mass estimates.
Cosmology and Nongalactic Astrophysics
