These joint efforts support the pathfinder for ngVLA technologies, focusing on very long baseline interferometry (VLBI) capabilities that enable ultra-sharp imaging of the Universe.
Recent News
Astronomers Detect Magnetic Fingerprint of a Cosmic Explosion for the First Time
Using the U.S. National Science Foundation Very Large Array (NSF VLA) radio telescope, which is operated by the U. S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO), the team detected polarized light from a gamma-ray burst (GRB) afterglow for the first time at radio wavelengths.
NSF VLA Sky Survey Sets New Standard for High-Resolution, Wide-Area Radio Astronomy
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) has completed observations for the Very Large Array Sky Survey (VLASS), the most detailed radio survey of the sky ever conducted.
Breakthrough Listen, NSF Green Bank Telescope Probe Galactic Heart for Hidden Pulsars
Artist’s impression of the NSF Green Bank Telescope gathering data on the center of the Milky Way. The inset image shows the black hole at our Galaxy’s center, and a nearby candidate (unconfirmed) pulsar. Image credit: Danielle Futselaar / Breakthrough Listen
Astronomers discover possible millisecond pulsar, challenging ideas about how many neutron stars lurk around the Milky Way’s central black hole
Astronomers from Breakthrough Listen have used the U.S. National Science Foundation National Radio Astronomy Observatory’s Green Bank Telescope (NSF GBT) to carry out one of the most sensitive pulsar searches ever aimed at the Milky Way’s Galactic Center.
The Galactic Center, home to the supermassive black hole Sagittarius A* and dense stellar populations, presents unique scientific opportunities and challenges for understanding stellar dynamics, extreme astrophysical environments, and tests of Einstein’s theory of General Relativity. In this research, recent Columbia University PhD graduate Karen Perez and collaborators conducted more than 20 hours of observations with the NSF GBT using the Breakthrough Listen Digital Backend, which enabled high-time and high-frequency resolution data products across a wide radio bandwidth. Of these observations, 11 hours were dedicated to the innermost 1.4 arcminutes of the Galactic Center, resulting in one of the deepest and most sensitive pulsar surveys ever performed toward this region.
These observations uncovered a promising candidate for a millisecond pulsar, with a rotation period of 8.19 milliseconds. If confirmed it would be the first such object found in the Galactic Center.
Find links to the paper, press materials, artwork, and the datasets and software at the University of Oxford Physics Department and the Breakthrough Listen Research Group.
About NRAO
The National Radio Astronomy Observatory (NRAO) is a facility of the U.S. National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
This news article was originally published on the NRAO website on February 9, 2026.
Recent News
U.S. National Science Foundation, NSF National Radio Astronomy Observatory and U.S. Naval Observatory Partner on Pathfinder for Next Generation Very Large Array
These joint efforts support the pathfinder for ngVLA technologies, focusing on very long baseline interferometry (VLBI) capabilities that enable ultra-sharp imaging of the Universe.
Astronomers Detect Magnetic Fingerprint of a Cosmic Explosion for the First Time
Using the U.S. National Science Foundation Very Large Array (NSF VLA) radio telescope, which is operated by the U. S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO), the team detected polarized light from a gamma-ray burst (GRB) afterglow for the first time at radio wavelengths.
NSF VLA Sky Survey Sets New Standard for High-Resolution, Wide-Area Radio Astronomy
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) has completed observations for the Very Large Array Sky Survey (VLASS), the most detailed radio survey of the sky ever conducted.