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Galaxy formation and evolution

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Galaxy formation and evolution

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Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles

The GOGREEN survey: dependence of galaxy properties on halo mass a z > 1 and implications for environmental quenching

Towards Efficient and Accurate Numerical Simulations of Galaxies using Task-based Parallelism and Application to Dwarf Galaxies

The GOGREEN survey: transition galaxies and the evolution of environmental quenching

The infrared-radio correlation of star-forming galaxies is strongly M-star-dependent but nearly redshift-invariant since z similar to 4

The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body mock challenge for the eBOSS emission line galaxy sample

SEEDisCS: I. Molecular gas in galaxy clusters and their large-scale structure: The case of CL1411.1-1148 at z similar to 0.5

Virgo filaments I. Processing of gas in cosmological filaments around the Virgo cluster

The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulumii, and Coma Berenices UFDs

On the influence of halo mass accretion history on galaxy properties and assembly bias