1.4k citations · 8.5k across the 76 of their papers we have counts for
7 papers · 1 filter
The DESI Experiment Part II: Instrument Design
DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290
DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…
The DESI Experiment Part I: Science,Targeting, and Survey Design
DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…
The galaxy population in cold and warm dark matter cosmologies
Lan Wang, Violeta Gonzalez-Perez, Lizhi Xie +7
We use a pair of high resolution N-body simulations implementing two dark matter models, namely the standard cold dark matter (CDM) cosmogony and a warm dark matter (WDM) alternati…
Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
Mark R. Lovell, Violeta Gonzalez-Perez, Sownak Bose +4
N-body dark matter simulations of structure formation in the CDM model predict a population of subhalos within Galactic halos that have higher central densities than inferred fo…
On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
J. Fogasy, K. K. Knudsen, C. D. P. Lagos +2
(Abridged) In the last decade several massive molecular gas reservoirs were found <100 kpc distance from active galactic nuclei (AGNs), residing in gas-rich companion galaxies. The…
The evolution of the [OII], Hβ and [OIII] emission-line luminosity functions over the last nine billions years
Johan Comparat, Guangtun Zhu, Violeta Gonzalez-Perez +12
Emission line galaxies are one of the main tracers of the large-scale structure to be targeted by the next-generation dark energy surveys. To provide a better understanding of the…
Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
Sownak Bose, Wojciech A. Hellwing, Carlos S. Frenk +6
We use the Copernicus Complexio (COCO) high resolution -body simulations to investigate differences in the properties of small-scale structures in the standard cold dark matter…