Ten high school students have been awarded for academic achievement, community involvement and leadership skills.
Recent News
NSF NRAO Leads Future of U.S. Radio Astronomy with First Light from Next Generation Very Large Array Prototype
The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.
VLBA Maps Turbulent ‘Weather’ in the Milky Way
Astronomers using the U.S. National Science Foundation’s Very Long Baseline Array (NSF VLBA), operated by the NSF National Radio Astronomy Observatory (NSF NRAO), have made the first clear, radio-wavelength detection of how turbulent gas in our own Galaxy distorts light from a distant quasar.
NSF Scholarships in Science, Technology, Engineering, and Mathematics (S-STEM)
Full Proposal Deadline Date: September 22, 2015
Program Guidelines: NSF 15-581
The National Science Foundation (NSF) Scholarships in Science, Technology, Engineering, and Mathematics program (S-STEM) addresses the need for a high quality STEM workforce in areas of national priorities. The program seeks to increase the success of low-income academically talented students with demonstrated financial need who are pursuing associate, baccalaureate, or graduate degrees in science, technology, engineering, and mathematics (STEM). The program provides awards to…
More at http://www.nsf.gov/funding/pgm_summ.jsp?pims_id=5257&WT.mc_id=USNSF_39&WT.mc_ev=click
For more information, contact Tim Spuck.
Recent News
AUI Announces 2026 Scholarship Recipients
Ten high school students have been awarded for academic achievement, community involvement and leadership skills.
NSF NRAO Leads Future of U.S. Radio Astronomy with First Light from Next Generation Very Large Array Prototype
The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.
VLBA Maps Turbulent ‘Weather’ in the Milky Way
Astronomers using the U.S. National Science Foundation’s Very Long Baseline Array (NSF VLBA), operated by the NSF National Radio Astronomy Observatory (NSF NRAO), have made the first clear, radio-wavelength detection of how turbulent gas in our own Galaxy distorts light from a distant quasar.