169 citations
- Pennsylvania State UniversityUS11 papers
- California Institute of TechnologyUS3 papers
- Chinese Academy of SciencesCN3 papers
- National Astronomical ObservatoriesCN3 papers
- California State Polytechnic UniversityUS2 papers
- Center for Astrophysics Harvard & SmithsonianUS2 papers
- Jet Propulsion LaboratoryUS2 papers
- Max Planck Institute for Extraterrestrial PhysicsDE2 papers
- Nanjing UniversityCN2 papers
- Pontificia Universidad Católica de ChileCL2 papers
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5 papers · 1 filter
Sensitive Chandra coverage of a representative sample of weak-line quasars: revealing the full range of X-ray properties
Q. Ni, W. N. Brandt, B. Luo +8
We present deeper Chandra observations for weak-line quasars (WLQs) in a representative sample that previously had limited X-ray constraints, and perform X-ray photometric analyses…
X-ray properties of dust-obscured galaxies with broad optical/UV emission lines
Fan Zou, William N. Brandt, Fabio Vito +4
Dust-obscured galaxies (DOGs) with extreme infrared luminosities may represent a key phase in the co-evolution of galaxies and supermassive black holes. We select 12 DOGs at $0.3\l…
Gaia Stellar Kinematics in the Head of the Orion A Cloud: Runaway Stellar Groups and Gravitational Infall
K. V. Getman, E. D. Feigelson, M. A. Kuhn +1
This work extends previous kinematic studies of young stars in the Head of the Orion A cloud (OMC-1/2/3/4/5). It is based on large samples of infrared, optical, and X-ray selected…
Heavy X-ray obscuration in the most-luminous galaxies discovered by WISE
F. Vito, W. N. Brandt, D. Stern +11
Hot Dust-Obscured Galaxies (Hot DOGs) are hyperluminous () infrared galaxies with extremely high (up to hundreds of K) dust tempe…
X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?
B. Luo, W. N. Brandt, P. B. Hall +9
We present an X-ray and multiwavelength study of 33 weak emission-line quasars (WLQs) and 18 quasars that are analogs of the extreme WLQ, PHL 1811, at z ~ 0.5-2.9. New Chandra 1.5-…