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ACEAP Ambassadors on Weekly Space Hangout

Recent News

Next-Generation Very Large Array Antenna Design to be Used By German Astronomers

The U.S. National Science Foundation National Radio Astronomy Observatory has announced a significant collaboration with the Bavarian State Government to construct a cutting-edge radio telescope atop Germany’s highest mountain. This radio telescope will use the design of the proposed NSF NRAO’s Next Generation Very Large Array (ngVLA).

NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient

High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.

ACEAP Ambassadors on Weekly Space Hangout

This Friday, June 12 at 3-4 PM, ACEAP Ambassadors Brian Koberlein, Michael Prokosch, Vivian White, and ACEAP Principal Investigator Tim Spuck will be hosted on the Weekly Space Hangout with Fraser Cain.

Please join the Event online on Friday June 12 from 3-4 PM at https://plus.google.com/u/0/events/cifv884e6jsmo2bv2gvnut7vol4

Recent News

Next-Generation Very Large Array Antenna Design to be Used By German Astronomers

The U.S. National Science Foundation National Radio Astronomy Observatory has announced a significant collaboration with the Bavarian State Government to construct a cutting-edge radio telescope atop Germany’s highest mountain. This radio telescope will use the design of the proposed NSF NRAO’s Next Generation Very Large Array (ngVLA).

NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient

High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.