The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is supporting Intuitive Machines’ second lunar mission, IM-2, which landed on the surface of the Moon, Thursday, March 6th.
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.
Applications Accepted for 2018 Astronomy in Chile Educator Ambassadors Program
Cerro Mayu Observatory outside La Serena, Chile. The Milky Way arches over sculptures near the Observatory. The Large and Small Magellanic Clouds can be seen near the horizon (right). Photo taken by 2017 ACEAP Ambassador Matt Dieterich (ACEAP/NSF)
Applications are now being accepted for the 2018 Astronomy in Chile Educator Ambassadors Program (ACEAP).
This program, in its fourth year, brings amateur astronomers, planetarium personnel, and astronomy educators to several U.S.-funded astronomy observatories in Chile. While there, ambassadors will receive behind-the-scenes tours of some of the world’s most productive and advanced telescopes, including in-depth information on their instruments and discoveries.
ACEAP is a collaborative project of Associated Universities, Inc., the National Radio Astronomy Observatory, National Optical Astronomy Observatory, and Gemini Observatory. ACEAP was initially funded in 2015 as a two-year pilot program by the National Science Foundation (NSF). Due to its success, NSF decided to fund the program for an additional two years.
To be eligible for this program, individuals must be U.S. citizens or permanent residents. Ambassadors may be either amateur astronomers, kindergarten through college (formal and informal) educators who teach astronomy as part of their curriculum or program, planetarium educators, or others who communicate astronomy to the public.
The ACEAP partners will select eight ambassadors from across the United States and its territories for the excursion, which will begin on 10 June 2018 and continue through 18 June 2018. This nine-day expedition (not including travel time between the U.S. and Chile) will include stops at the Cerro Tololo Inter-American Observatory (CTIO), Gemini-South Observatory, and the Atacama Large Millimeter/submillimeter Array (ALMA).
APPLY NOW – http://epe.aui.edu/programs/astronomy-in-chile-educator-ambassadors-program/
ACEAP 2016 Ambassadors. Ambassadors visit the Atacama Desert following a successful visit to the ALMA high-site at 16,500 ft. Photo by Tim Spuck (AUI/NSF).
Recent News
Space Company Taps Coast-to-Coast Radio Telescopes for Moon Mission
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is supporting Intuitive Machines’ second lunar mission, IM-2, which landed on the surface of the Moon, Thursday, March 6th.
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.