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(73 - 96 of 306)

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An EAGLE view of the missing baryons
The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
Revealing the impact of quasar luminosity on giant Ly α nebulae
SEAGLE - II. Constraints on feedback models in galaxy formation from massive early-type strong-lens galaxies
Morphological and rotation structures of circumgalactic Mg II gas in the EAGLE simulation and the dependence on galaxy properties
Revealing the impact of quasar luminosity on giant Ly α nebulae
The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
Detection capabilities of the Athena X-IFU for the warm-hot intergalactic medium using gamma-ray burst X-ray afterglows
Erratum: MUSEQuBES: calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles
The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly emitters at z > 3
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray and UV line absorption
The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies
The BAHAMAS project: effects of dynamical dark energy on large-scale structure
The Cosmic Ultraviolet Baryon Survey (CUBS) - I. Overview and the diverse environments of Lyman limit systems at z < 1
The MUSE Hubble Ultra Deep Field Survey. XIV. Evolution of the Ly α emitter fraction from z = 3 to z = 6
O VII and O VIII in the CGM of simulated Milky Way mass galaxies
The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
MUSEQuBES: calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles
Simulating galaxy populations
Galaxy morphology and the stellar-halo mass relation
EAGLE and Illustris-TNG predictions for resolved eROSITA X-Ray observations of the circumgalactic medium around normal galaxies
Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters
Constraining the intergalactic medium at z≈9.1 using LOFAR Epoch of Reionization observations
Hot WHIM counterparts of FUV O VI absorbers: evidence in the line-of-sight towards quasar 3C 273

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