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(1 - 20 of 22)

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Spectroscopic confirmation of four metal-poor galaxies at z = 10.3-13.2
The MAGPI Survey: impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
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
Galaxy And Mass Assembly (GAMA)
The velocity dispersion function for massive quiescent and star-forming galaxies at 0.6 < z <= 1.0
The mass scale of high-redshift galaxies
LEGA-C
The LEGA-C and SAMI galaxy surveys
Ubiquitous [O II] Emission in Quiescent Galaxies at z ≍ 0.85 from the LEGA-C Survey
Toward precise galaxy evolution
The Large Early Galaxy Astrophysics Census (LEGA-C) data release 3
The Fundamental Plane in the LEGA-C survey
The SAMI galaxy survey
The LEGA-C Survey of 4000 Galaxies at z 1
The LEGA-C survey completed
Dust attenuation curves at z ~ 0.8 from LEGA-C: precise constraints on the slope and 2175A bump strength
Tightly coupled morpho-kinematic evolution for massive star-forming and quiescent galaxies across 7 Gyr of cosmic time
Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
Stellar kinematics and environment at z ~ 0.8 in the LEGA-C survey: massive slow rotators are built first in overdense environments

Pages