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EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
MIGHTEE-H I : the M_HI – M* relation over the last billion years
Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C, and SAMI surveys
Different higher order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI, and LEGA-C surveys
Euclid preparation
Statistical strong lensing
Ultra diffuse galaxies in the MATLAS low-to-moderate density fields