By analyzing nearly a decade of NSF VLBA observations of the quasar TXS 2005+403, an international team led by the Center for Astrophysics | Harvard & Smithsonian (CfA) directly measured the tiny, turbulence-driven “ripples” imprinted on the quasar’s radio signal as it passes through a particularly chaotic region of the Milky Way.
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Radio Black Hole Trio Lights Up in Rare Galaxy Merger
Astronomers from the U.S. Naval Research Laboratory (NRL), in conjunction with scientists from the U.S. Naval Observatory (USNO) and NASA Goddard Space Flight Center (NASA GSFC), using U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) instruments have confirmed the first known triple system in which all three galaxies host actively feeding, radio-bright supermassive black holes.
Astronomers Detect Lowest Mass Dark Object Yet in Distant Universe
An international research team, using a worldwide network of radio telescopes, including the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) VLBA and GBT, has detected an enigmatic dark object with a mass about one million times that of our Sun without observing any emitted light. This is the lowest mass dark object ever detected at a cosmological distance using only its gravitational influence, marking a major milestone in the quest to unravel the nature of dark matter.
National Radio Astronomy Observatory to Outfit the VLBA with New Ultra Wideband Receivers
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) has begun a major upgrade to the NSF Very Long Baseline Array (NSF VLBA) with the development and installation of state-of-the-art ultra wideband receivers capable of operating across the frequency range of 8 to 40 gigahertz (GHz). This new technology, first prototyped by NRAO in collaboration with NASA’s Jet Propulsion Laboratory (JPL), and tested on the NSF VLBA’s Owens Valley station, promises to significantly expand the scientific capabilities of the NSF VLBA.
NSF NRAO Achieves First Successful Observations with New NSF VLBA Digital Architecture
The new NSF VLBA New Digital Architecture (VNDA) produced its first fringes and subsequent images in January 2025, demonstrating the successful implementation of next-generation technology that will enhance the NSF VLBA’s scientific capabilities for years to come.
Astronomers Catch Unprecedented Features at Brink of Active Black Hole
International teams of astronomers monitoring a supermassive black hole in the heart of a distant galaxy have detected features never seen before using data from NASA missions and other facilities including the National Science Foundation (NSF) National Radio Astronomy Observatory (NSF NRAO) Very Long Baseline Array (VLBA).