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most citedMetallicity of the intergalactic medium using pixel statistics. II. The distribution of metals as traced by C IV

391 citations · 1.1k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2020★ 102 cited

The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies

Andreea S. Font, Ian G. McCarthy, Robert Poole-Mckenzie +6

We introduce the ARTEMIS simulations, a new set of 42 zoomed-in, high-resolution (baryon particle mass of ~ 2x10^4 Msun/h), hydrodynamical simulations of galaxies residing in haloe…

astro-ph.GA2016★ 77 cited

The properties of "dark" ΛCDM halos in the Local Group

Alejandro Benítez-Llambay, Julio F. Navarro, Carlos S. Frenk +7

We examine the baryon content of low-mass ΛCDM halos using the APOSTLE cosmological hydrodynamical simulations. Most of these systems…

astro-ph.CO2013★ 286 cited

The impact of angular momentum on black hole accretion rates in simulations of galaxy formation

Y. M. Rosas-Guevara, R. G. Bower, J. Schaye +7

Feedback from energy liberated by gas accretion onto black holes (BHs) is an attractive mechanism to explain the exponential cut-off at the massive end of the galaxy stellar mass f…

astro-ph2003★ 391 cited

Metallicity of the intergalactic medium using pixel statistics. II. The distribution of metals as traced by C IV

Joop Schaye, Anthony Aguirre, Tae-Sun Kim +3

(Modified) We measure the distribution of carbon in the intergalactic medium as a function of redshift z and overdensity delta. Using a hydrodynamical simulation to link the H I ab…

astro-ph2002

Numerical simulations of the intergalactic medium

Tom Theuns

The intergalactic medium at redshifts 2--6 can be studied observationally through the absorption features it produces in the spectra of background quasars. Most of the UV-absorptio…

astro-ph2002★ 187 cited

Constraints on reionization from the thermal history of the intergalactic medium

Tom Theuns, Joop Schaye, Saleem Zaroubi +3

The temperature of the diffuse, photo-heated intergalactic medium (IGM) depends on its reionization history because the thermal time scales are long. The widths of the hydrogen Lym…