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- Experiments in Gravitation with Highly Stable Clocks
- Laboratory Measurements of Newtons's Constant, G
- Tests of Gravity at Short Range

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- Advanced Technologies for Space Gravitational Wave Detectors
- Effective One Body Formalism
- Gravitational Wave Sources: Binaries (High and Low Frequency)
- Gravitational Waves from Extreme Mass Ratio Inspiral (EMRI)
- Gravitational Waves from Ultra-compact Binaries
- Interface Between Gravitational Waves and Astronomy
- Pulsar Timing and Low Frequency Gravitational Wave Detection
- Rates for Binary Coalescences
- Stellar Dynamics and Extreme Mass Ratio Inspirals
- Stochastic GW Background Detection Methods
- Terrestrial Gravity Fluctuations
- The ADM canonical approach to the post-Newtonian motion of compact binaries
- The Square-Kilometre-Array (SKA)

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- History of Gravitational Wave Research

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- Area Angular Momentum Charge Inequality
- Cosmic Censorship (toolbox)
- Exact Solutions
- Integrable Reductions of the Einstein Equations
- Newtonian Limit
- The Constraint Problem for Einstein's Equations

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- Algebraic Computing in General Relativity
- Formulations of Einstein's Equations for Numerical Relativity
- Interface of Post-Newtonian Theories and Numerical Relativity
- Numerical Relativity for Black Holes
- Numerical Simulations of Core-Collapse Supernovae
- Reduced Order Modeling
- Strong-Field Dynamics of Astrophysical Black Hole Mergers

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- Cosmic Evolution of Super Massive Black Holes in Galactic Centers (the X-Ray view)
- The Impact of Galaxy Mergers on the Growth of Supermassive Black Holes

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- Causal Sets

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- Electromagnetic Counterparts to Supermassive Black Hole Mergers
- Masses of known neutron stars
- Massive Black Holes in Galaxies
- Microquasars
- Testing General Relativity with the Event Horizon Telescope
- The Magnetic Fields of Neutron Stars

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- Asymptotic Charges and Symmetries
- Black Holes, Hidden Symmetry and Complete Integrability
- Solitonic Solutions of Supergravity