output
19942026
Showing 2009 · astro-ph.COShow all

43 papers · 2 filters

astro-ph.CO2009★ 8 cited

Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?

J. E. Forero-Romero, G. Yepes, S. Gottloeber +4

We discuss the rest-frame UV emission between 5< z < 7 from the MareNostrum High-z Universe, a SPH simulation done with more than 2 billion particles. Cosmological simulations of g…

astro-ph.CO2009★ 92 cited

Rest-frame ultraviolet spectrum of the gravitationally lensed galaxy `the 8 o'clock arc': stellar and interstellar medium properties

M. Dessauges-Zavadsky, S. D'Odorico, D. Schaerer +3

We present the first detailed analysis of the rest-frame UV spectrum of the gravitationally lensed Lyman break galaxy (LBG), the `8 o'clock arc'. The spectrum of the 8 o'clock arc…

astro-ph.CO2009★ 55 cited

The XMM-Newton Wide Angle Survey (XWAS): the X-ray spectrum of type-1 AGN

S. Mateos, F. J. Carrera, M. J. Page +7

We discuss the broad band X-ray properties of one of the largest samples of X-ray selected type-1 AGN to date (487 objects in total), drawn from the XMM-Newton Wide Angle Survey. T…

astro-ph.CO2009★ 15 cited

Investigating the influence of magnetic fields upon structure formation with AMIGA - a C code for cosmological magnetohydrodynamics

Timur Doumler, Alexander Knebe

Despite greatly improved observational methods, the presence of magnetic fields at cosmological scales and their role in the process of large-scale structure formation still remain…

astro-ph.CO2009★ 196 cited

The Coyote Universe III: Simulation Suite and Precision Emulator for the Nonlinear Matter Power Spectrum

Earl Lawrence, Katrin Heitmann, Martin White +4

Many of the most exciting questions in astrophysics and cosmology, including the majority of observational probes of dark energy, rely on an understanding of the nonlinear regime o…

astro-ph.CO2009★ 52 cited

Fake star formation bursts: blue horizontal branch stars masquerade as young stars in optical integrated light spectroscopy

P. Ocvirk

Model color magnitude diagrams of low-metallicity globular clusters usually show a deficit of hot evolved stars with respect to observations. We investigate quantitatively the impa…