Meet Mario Vargas, a technical specialist III at the U.S. National Science Foundation National Radio Astronomy Observatory’s Central Development Laboratory.
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.
Einstein Fellows: Best Practices in STEM Education, 2014 Book of the Year
Tim Spuck’s book, Einstein Fellows: Best Practices in STEM Education has received the Book of the Year award by its publisher, Peter Lang Publishing, a major international academic publishing house.
Congratulations to Tim!
Recent News
10 Questions: Mario Vargas
Meet Mario Vargas, a technical specialist III at the U.S. National Science Foundation National Radio Astronomy Observatory’s Central Development Laboratory.
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.