TB
Tamara Bogdanovic
Georgia Institute of Technology
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysical Phenomena and Observations · Galaxies: Formation, Evolution, Phenomena · Pulsars and Gravitational Waves Research
Employment
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Georgia Institute of Technology Professor
Education
Education history is unavailable.
Projects & Funding
Projects & funding information is unavailable.
Publications (88)
- Chandra X-Ray Observations of Quasars with Velocity-offset Broad Lines: Assessing the Binary Supermassive Black Hole Hypothesis Save
- Evolution of Supermassive Black Hole Pairs on Inclined Orbits in Postmerger Galaxies Save
- The Era of Binary Supermassive Black Holes: Coordination of Nanohertz-Frequency Gravitational-Wave Follow-up Save
- The Tantalizing Case of the Quasar J0950+5128. I. Presentation of the Data and Detailed Exploration of the Binary Supermassive Black Hole Scenario Save
- Radiative Magnetohydrodynamics Simulation of Minidisks in Equal-mass Massive Black Hole Binaries Save
- X-Ray Reflection Signatures of Supermassive Black Hole Binaries Save
- Radiation Magnetohydrodynamic Simulation of Sub-Eddington Circumbinary Disk around an Equal-mass Massive Black Hole Binary Save
- A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes. IV. Ultraviolet Spectroscopy* † Save
- Contaminating Electromagnetic Transients in LISA Gravitational-wave Localization Volumes. I. The Intrinsic Rates Save
- Insights into supermassive black hole mergers from the gravitational wave background Save
- Massive Black Hole Binaries from the TNG50-3 Simulation. II. Using Dual AGNs to Predict the Rate of Black Hole Mergers Save
- Astrophysics with the Laser Interferometer Space Antenna Save
- The X-ray view of optically selected dual AGN Save
- Massive Black Hole Binaries as LISA Precursors in the Roman High Latitude Time Domain Survey Save
- Electromagnetic counterparts to massive black-hole mergers Save
- Massive Black Hole Binaries from the TNG50-3 Simulation. I. Coalescence and LISA Detection Rates Save
- Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven Hα Filaments Save
- Multimessenger time-domain signatures of supermassive black hole binaries Save
- The effect of mission duration on LISA science objectives Save
- On the Mass Loading of AGN-driven Outflows in Elliptical Galaxies and Clusters Save