DD
Daniel J. D'Orazio
Space Telescope Science Institute, Johns Hopkins University, Columbia University Columbia College, Juniata College, Københavns Universitet Niels Bohr Instituttet
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Galaxies: Formation, Evolution, Phenomena
0000-0002-1271-6247
Employment
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Space Telescope Science Institute Assistant Astronomer2024 - Present
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Johns Hopkins University Associate Research Scientist2024 - Present
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Københavns Universitet Niels Bohr Instituttet Assistant Professor2020 - Present
- 2019 - 2020
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Harvard University NASA Einstein Postdoctoral Fellow2016 - 2019
Education
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Columbia University Columbia College PhD2010 - 2016
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Juniata College B.S. Summa Cum Laude2005 - 2009
Projects & Funding
Projects & funding information is unavailable.
Publications (114)
- Dynamics and Detectability of Long-lived Nonaccretion Phases for Massive Black Hole Binaries in Cold Thermally Regulating Disks Save
- Supermassive Black Hole Binaries in the Multi-messenger Context of Ground and Spaceborne VLBI* Save
- Primordial-Black-Hole-Based Pathways to Little Red Dots Save
- Gaseous Dynamical Friction on Hyperbolic Scatterings Save
- The Era of Binary Supermassive Black Holes: Coordination of Nanohertz-Frequency Gravitational-Wave Follow-up Save
- Insights from Analytical Theory of Eccentric Circumbinary Disks Save
- deci-Hz Gravitational Wave Observations on the Moon and Beyond Save
- Spiral Density Waves and Torque Balance in the Kerr Geometry Save
- Hot, Cold, and Multicomponent Accretion Flows around Supermassive Black Hole Binaries Save
- A cosmologist's take on Little Red Dots Save
- The LISA Astrophysics "Disc-IMRI" Code Comparison Project: Intermediate-Mass-Ratio Binaries in AGN-Like Discs Save
- Stellar Stripping and Disruption in Disks around Supermassive Black Hole Binaries: Repeating Nuclear Transients Prior to LISA Events Save
- Gravitational Wave Decoupling in Retrograde Circumbinary Disks Save
- Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries Save
- Bridging the micro-Hz gravitational wave gap via Doppler tracking with the Uranus Orbiter and Probe mission: Massive black hole binaries, early Universe signals, and ultralight dark matter Save
- Testing compact massive black hole binary candidates through multi-epoch spectroscopy Save
- Gravitational-wave Phase Shifts in Eccentric Black Hole Mergers as a Probe of Dynamical Formation Environments Save
- The Host Galaxies of Pulsar Timing Array Sources: Converting Supermassive Black Hole Binary Parameters into Electromagnetic Observables Save
- Dissecting environmental effects with eccentric gravitational wave sources Save
- Gaseous Dynamical Friction on Hyperbolic Scatterings Save