We study the dynamical properties of massive quiescent galaxies at 1.4 < z < 2.1 using deep Hubble Space Telescope WFC3/F160W imaging and a combination of literature stellar velocity dispersion measurements and new...
We study the dynamical properties of massive quiescent galaxies at 1.4 < z < 2.1 using deep Hubble Space Telescope WFC3/F160W imaging and a combination of literature stellar velocity dispersion measurements and new...
We derive relations between the effective radii R eff of galaxies and the virial radii R 200c of their dark matter halos over the redshift range 0 <z <3. For galaxies, we use the measured sizes...
We present a comparison of the spatial distributions of Lyα emitters (LAEs) and massive star-forming and quiescent galaxies (SFGs and QGs) at 2 < z < 4.5. We use the photometric redshift catalog to select SFGs and QGs...
We derive relations between the effective radii R eff of galaxies and the virial radii R 200c of their dark matter halos over the redshift range 0 <z <3. For galaxies, we use the measured sizes...
We present a comparison of the spatial distributions of Lyα emitters (LAEs) and massive star-forming and quiescent galaxies (SFGs and QGs) at 2 < z < 4.5. We use the photometric redshift catalog to select SFGs and QGs...
We explore the Hα emission in the massive quiescent galaxies observed by the KMOS3D survey at 0.7 <z <2.7. The Hα line is robustly detected in 20 out of 120 UVJ-selected quiescent galaxies, and we classify...
We explore the Hα emission in the massive quiescent galaxies observed by the KMOS3D survey at 0.7 <z <2.7. The Hα line is robustly detected in 20 out of 120 UVJ-selected quiescent galaxies, and we classify...
The solid-gas phase photo-catalytic activities of rutile TiO₂ and TiO n (1 < n < 2) sub-oxide phases have been evaluated. Varying concentrations of Ti 3+ defects were introduced into the rutile polymorph of titanium...
The solid-gas phase photo-catalytic activities of rutile TiO₂ and TiO n (1 < n < 2) sub-oxide phases have been evaluated. Varying concentrations of Ti 3+ defects were introduced into the rutile polymorph of titanium...
We report on the host properties of five X-ray-luminous active galactic nuclei (AGN) identified at 3 < z < 5 in the first epoch of imaging from the Cosmic Evolution Early Release Science Survey. Each galaxy has been...
We report on the host properties of five X-ray-luminous active galactic nuclei (AGN) identified at 3 < z < 5 in the first epoch of imaging from the Cosmic Evolution Early Release Science Survey. Each galaxy has been...
We explore the dependence of the incidence of moderate-luminosity (L0.5-8 keV = 1041.9-43.7 erg s-1) active galactic nuclei (AGNs) and the distribution of their accretion rates on host color...
We explore the dependence of the incidence of moderate-luminosity (L0.5-8 keV = 1041.9-43.7 erg s-1) active galactic nuclei (AGNs) and the distribution of their accretion rates on host color...
Here, we report on the development of highly overmoded structure for a millimeter-wave (MMW) extended interaction klystron (EIK). To enhance electron beam loading, a new method for designing an oversized beam tunnel in a...
|< |
< |
1 |