New catalog adds 161 gravitational wave detections

Astronomers have published the largest gravitational wave catalog to date, bringing the total number of confirmed detections to 390. The update includes signals recorded through early 2025 by the international LVK network of detectors.

The Gravitational Wave Transient Catalogue-5.0, released by the LIGO-Virgo-KAGRA collaboration, incorporates 161 new black hole merger signals detected between April 2024 and January 2025. Researchers at the University of Glasgow contributed to detector technology and data analysis for the project.

Key records in the catalog include the clearest signal yet recorded, GW250114, which reached Earth on January 14, 2025, and the most precise sky localization of any gravitational wave source, achieved for event GW240615 on June 15, 2024. The data also provide further evidence of second-generation black holes formed through prior mergers.

Scientists used the expanded set of observations to refine measurements of the Hubble constant, which describes the rate of the universe's expansion. The catalog's release marks a shift toward population studies of black holes rather than analysis of single events.

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Physicists have found a potential signature of dark matter in data from a black hole merger observed in 2019. The signal known as GW190728 showed patterns consistent with the invisible substance interacting with the colliding objects. A new model developed by researchers at MIT and partner institutions made the analysis possible.

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A recent study from the University of Miami suggests that an unusual gravitational wave detected by LIGO could represent the first evidence of a primordial black hole. Researchers say such an object would support the idea that these ancient black holes make up dark matter.

Astronomers using NASA’s James Webb Space Telescope have produced the most detailed map yet of the universe’s cosmic web, the vast network of dark matter and gas that links galaxies. The map traces structures back to when the universe was roughly one billion years old.

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A superluminous supernova nicknamed SN Winny, located 10 billion light-years away, appears in the sky five times due to gravitational lensing by two foreground galaxies. Researchers from the Technical University of Munich and other institutions have analyzed this rare event to measure the universe's expansion rate, known as the Hubble constant. The discovery could help resolve the ongoing Hubble tension between different measurement methods.

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