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Detecting galaxy-filament alignments in the Sloan Digital Sky Survey III

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Detecting galaxy-filament alignments in the Sloan Digital Sky Survey III

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The formation of the faintest galaxies in cosmological simulations: from the impact of primordial magnetic fields to the metal enrichment of present day dwarfs by first stars

A model for the infrared-radio correlation of main sequence galaxies at gigahertz frequencies and its variation with redshift and stellar mass

GOGREEN: A critical assessment of environmental trends in cosmological hydrodynamical simulations at z approximate to 1

Euclid preparation XXX. Performance assessment of the NISP red grism through spectroscopic simulations for the wide and deep surveys

The DESI One-Percent Survey: Constructing Galaxy-Halo Connections for ELGs and LRGs Using Auto and Cross Correlations

SEAGLE III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations

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

Does concentration drive the scatter in the stellar-to-halo mass relation of galaxy clusters?

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

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