Add to ORKGWe present a comparison of stellar and dynamical masses for 63 UV-selected galaxies with spectroscopic redshifts at z ∼ 2. Stellar masses are determined by fitting SEDs to UGRJK photometry, with the addition of mid-IR data from the Spitzer Space Telescope in some cases. Dynamical masses are determined using the velocity dispersions from Hα spectra. We find a mean stellar mass of 7 × 10^(10) M_☉ and a mean dynamical mass of 6 × 10^(10) M_☉; we discuss the limitations of both mass estimators
Aims.The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We present an analysis of stellar mass estimates for a sample of 25000 galaxies from the COMBO-17 s...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...
We present a comparison of stellar and dynamical masses for 63 UV-selected galaxies with spectroscop...
We present analysis of the near-infrared spectra of 114 rest-frame UV-selected star-forming galaxies...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We determine the importance of redshift-dependent systematic effects in the determination of stellar...
We present analysis of the near-infrared spectra of 114 rest-frame UV-selected star-forming galaxies...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...
16Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, base...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
Aims.The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We present an analysis of stellar mass estimates for a sample of 25000 galaxies from the COMBO-17 s...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...
We present a comparison of stellar and dynamical masses for 63 UV-selected galaxies with spectroscop...
We present analysis of the near-infrared spectra of 114 rest-frame UV-selected star-forming galaxies...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We determine the importance of redshift-dependent systematic effects in the determination of stellar...
We present analysis of the near-infrared spectra of 114 rest-frame UV-selected star-forming galaxies...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...
16Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, base...
Aims. The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
Aims.The purpose of this study is to explore the relationship between galaxy stellar masses, based ...
We present an analysis of stellar mass estimates for a sample of 25000 galaxies from the COMBO-17 s...
We measured stellar velocity dispersions σ and derived dynamical masses of nine massive (M ≈ 1011 M ...