activity
19982023
most citedLSST Science Book, Version 2.0

924 citations · 4.5k across the 99 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 170 cited

Angular momentum evolution of galaxies in EAGLE

Claudia del P. Lagos, Tom Theuns, Adam R. H. Stevens +5

We use the EAGLE cosmological hydrodynamic simulation suite to study the specific angular momentum of galaxies, , with the aims of (i) investigating the physical causes behind t…

astro-ph.GA2016★ 62 cited

How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE

Adam R. H. Stevens, Claudia del P. Lagos, Sergio Contreras +5

We use the hydrodynamic, cosmological EAGLE simulations to investigate how hot gas in haloes condenses to form and grow galaxies. We select haloes from the simulations that are act…

astro-ph.HE2016★ 20 cited

GW150914: First search for the electromagnetic counterpart of a gravitational-wave event by the TOROS collaboration

Mario C. Díaz, Martín Beroiz, Tania Peñuela +31

We present the results of the optical follow-up conducted by the TOROS collaboration of the first gravitational-wave event GW150914. We conducted unfiltered CCD observations (0.35-…

astro-ph.GA2016★ 30 cited

The evolution of the galaxy content of dark matter haloes

S. Contreras, I. Zehavi, C. M. Baugh +2

We use the halo occupation distribution (HOD) framework to characterise the predictions from two independent galaxy formation models for the galactic content of dark matter haloes…

astro-ph.CO2016★ 28 cited

Testing LSST Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics

Humna Awan, Eric Gawiser, Peter Kurczynski +7

The Large Synoptic Survey Telescope (LSST) will survey the southern sky from 2022--2032 with unprecedented detail. Since the observing strategy can lead to artifacts in the data, w…

astro-ph.CO2016★ 24 cited

Subhalo accretion through filaments

Roberto E. Gonzalez, Nelson D. Padilla

We track subhalo orbits of galaxy and group sized halos in cosmological simulations. We identify filamentary structures around halos and we use these to define a sample of subhalos…