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On the equivalent width of the Fe K$\alpha$ line produced by a dusty absorber in active galactic nuclei
Free accessArXiv | 2015| -
Pairing of Massive Black Holes in Merger Galaxies Driven by Dynamical Friction
Free accessArXiv | 2020| -
The Pairing Probability of Massive Black Holes in Merger Galaxies in the Presence of Radiative Feedback
Free accessArXiv | 2020| -
Massive Black Hole Binaries from the TNG50-3 Simulation: I. Coalescence and LISA Detection Rates
Free accessArXiv | 2022| -
CO Line Emission from Compact Nuclear Starburst Disks Around Active Galactic Nuclei
Free accessArXiv | 2012| -
IRON Ka EMISSION FROM X-RAY REFLECTION: PREDICTIONS FOR GAMMA-RAY BURST MODELS
Online Contents | 2001| -
The Merger-Triggered Active Galactic Nuclei Contribution to the Ultraluminous Infrared Galaxy Population
Free accessArXiv | 2012| -
Properties and Expected Number Counts of Active Galactic Nuclei and their Hosts in the Far Infrared
Free accessArXiv | 2011| -
On the contribution of active galactic nuclei to reionization (Research Note)
Free accessArXiv | 2013| -
On the Blazar Contribution to the Cosmic X‐ray Background: Implications for the Compton Thick Population
American Institute of Physics | 2010| -
Iron K-alpha Emission from X-ray Reflection: Predictions for Gamma-Ray Burst Models
Free accessArXiv | 2001|
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