Detection Methods LIGO Detection Black Hole Mergers Detection Techniques Astrophysical Phenomena LIGO-Virgo-KAGRA Space-Time Black Holes Detection Technology Astrophysics Supermassive Black Holes Dark Matter Research Methods Binary Systems Cosmic Phenomena LISA Mission Low-Frequency Gravitational Waves Ultra-low Frequency Gravitational Waves Types Sources Research Accretion Disks Observational Astronomy Observational Techniques Mass Transfer Cosmic Events LISA LISA Spacecraft LISA Observatory Black Hole Dynamics Space-Time Distortions Ultralow Frequency Gravitational Waves Cosmic History Frequency Analysis Black Hole Interactions Wave Behavior Pulsar Timing Arrays Wave Observations Stellar Mergers Signal Analysis Laser Interferometry Cosmic Strings Neutron Star Physics Primordial Gravitational Waves Binary Coalescences Cosmological Phenomena Gravitational Recoil Interferometry General Relativity Neutron Stars Einstein Telescope Formation High-Frequency Gravitational Waves LIGO Detectors Research Techniques Statistical Techniques Merging Black Holes Wave Spectrum Quasiperiodic Oscillations Observatories Gravitational Wave Background Low-frequency Gravitational Waves Origins Theoretical Foundations Confirmation of Einstein's Theory Research Collaboration Frequency Range
Analyses of AT 2024wpp show an energy output far beyond supernovae, pointing to an extreme tidal disruption that refocuses how astronomers will search for these events.
