J. D. Cline, M. W. Castelaz
StarLab
Portable 8.2m diameter planetarium travels to grades K-8 schools
Duke Talent Identification
Program. Summer Field
Study in Astronomy
• Presentations to more than 32,000 students in Western North Carolina
• Six Learning Technologies, Inc
Programs offered
Pisgah Astronomical Research Institute is a not-for-profit public foundation located on 200 acres in
Western North Carolina in the Pisgah National Forest. This poster presents premier programs. Frequent seminars for high school and undergraduate students, and periodic astronomical research collaborations complete programs at
PARI. See http://www.pari.edu/ for more information for access to PARI Observatories.
N
Dr. David Moffett, Furman
University
• 327 MHz receiver installed on 26 East radio telescope.
• Timings of a dozen pulsars.
• Duke TIP Summer Field Study in
Astronomy
• Senior Projects
NSF Funded Internships In
Public Science Education
• NSF IPSE Interns in multimedia and physics developing a radio sky StarLab program
• UNC-Asheville Computer Science class developing remote radio telescope control and data analysis software
• Summer research students with funding from grants & donations as scholarships
Brian
Dennison, UNC-Asheville
• Long-term monitoring of interstellar turbulence via its effect on scattering of radio waves over a large sample of compact sources.
• Two element interferometer to reduce noise confusion and measure point sources.
• Two frequencies, 2.4 GHz and 8.4 GHz.
Graduate Students
• PARI Observatories available for testbed applications, monitoring and survey research
•
Administered by UNC-Asheville for the benefit of each university within the 16-campus University of
North Carolina system to promote and coordinates usage of the facilities at PARI.
•
Consortium of 6 universites and 2 community colleges to promote research and education using a 0.40m robotic telescope at PARI.
•
Native American, Hispanic, African American, and underrepresented high school students in rural Western North Carolina will have the opportunity to conduct space science research through visible and radio observations of the Sun.
Dr. Mel Blake, PARI
• Measure period changes in pulsating stars to study their evolution
• Measure period changes in close binaries to measure effects of magnetic winds.
• Use the PARI 0.35m telescope and CCD
The 26m radio telescopes have new control systems and pointing models
The optical telescopes are equipped with CCDs and
BVRI filters, and are under robotic control
Each feedbox has AC power, coax, 12 fibers and appropriate cabling as required by receiver configuration
Seeing average is 2 arcsec
Differential photometry average 3 nights/week
All labs, offices, telescopes linked via fiber optics and OC-48 network
Power backup across campus