Detection Methods LIGO Detection Black Hole Mergers Detection Techniques Astrophysical Phenomena LIGO-Virgo-KAGRA Astrophysics Detection Technology Black Holes Space-Time Dark Matter Binary Systems Supermassive Black Holes LISA Mission Research Methods Frequency Range 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 Neutron Stars Cosmological Phenomena Formation High-Frequency Gravitational Waves LIGO Detectors Research Techniques Statistical Techniques Merging Black Holes Wave Spectrum Observatories Cosmic Phenomena Gravitational Wave Background Low-frequency Gravitational Waves Origins Theoretical Foundations Confirmation of Einstein's Theory Research Collaboration
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.