1.7k citations
- Yale UniversityUS42 papers
- Center for Astrophysics Harvard & SmithsonianUS11 papers
- California Institute of TechnologyUS9 papers
- Université Bourgogne Franche-ComtéFR8 papers
- Max Planck Institute for Extraterrestrial PhysicsDE7 papers
- Space Telescope Science InstituteUS7 papers
- Centre National de la Recherche ScientifiqueFR6 papers
- University of California, BerkeleyUS6 papers
- University of Hawaii SystemUS6 papers
- Durham UniversityGB5 papers
- Max Planck Institute for AstronomyDE5 papers
- National Radio Astronomy ObservatoryUS5 papers
51 papers
Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
R. Genzel, N. M. Förster Schreiber, H. Übler +28
In cold dark matter cosmology, the baryonic components of galaxies are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter, which dominates the t…
Chemical Composition of Young Stars in the Leading Arm of the Magellanic System
Lan Zhang, Christian Moni Bidin, Dana I. Casetti-Dinescu +6
Chemical abundances of eight O- and B-type stars are determined from high-resolution spectra obtained with the MIKE instrument on the Magellan 6.5m Clay telescope. The sample is se…
Mass Constraints of the WASP-47 Planetary System from Radial Velocities
Evan Sinukoff, Andrew W. Howard, Erik A. Petigura +19
We report precise radial velocity (RV) measurements of WASP-47, a G star that hosts three transiting planets in close proximity (a hot Jupiter, a super-Earth and a Neptune-sized pl…
Obscured Active Galactic Nuclei triggered in compact star-forming galaxies
Yu-Yen Chang, Emeric Le Floc'h, Stéphanie Juneau +10
We present a structural study of 182 obscured Active Galactic Nuclei (AGNs) at z<=1.5, selected in the COSMOS field from their extreme infrared to X-ray luminosity ratio and their…
An Over-Massive Black Hole in a Typical Star-Forming Galaxy, 2 Billion Years After the Big Bang
Benny Trakhtenbrot, C. Megan Urry, Francesca Civano +6
Supermassive black holes (SMBHs) and their host galaxies are generally thought to coevolve, so that the SMBH achieves up to about 0.2 to 0.5% of the host galaxy mass in the present…
Assessing Colour-dependent Occupation Statistics Inferred from Galaxy Group Catalogues
Duncan Campbell, Frank C van den Bosch, Andrew Hearin +5
We investigate the ability of current implementations of galaxy group finders to recover colour-dependent halo occupation statistics. To test the fidelity of group catalogue inferr…