Observations of Active Galactic Nuclei via a Student Operated Remote Observatory Whitney Wills Michael Carini-Faculty Mentor Department of Physics and.
Science with SKA:. The SKA will provide continuous frequency coverage from 50 MHz to 14 GHz in the first two phases of its construction. A third phase.
Argentina and Brazil A possible site to host the SKA M. Arnal, G. Dubner, E. Giacani, J. Lepine, H. Levato, R. Morras, E. Reynoso AAA, 2005, La Plata.
The SKA Molonglo Prototype (SKAMP) Project Molonglo 40th Anniversary, November 2005.
SVO: The Spanish Virtual Observatory svo.laeffta.es
1 AUI Cooperative Agreement — NSF Panel Review August 25 – 28, 2008 National Radio Astronomy Observatory Science enabled by NRAO facilities into the next.
Argentina and Brazil A possible site to host the SKA
Observations of Active Galactic Nuclei via a Student Operated Remote Observatory Whitney Wills
SVO: The Spanish Virtual Observatory Enrique Solano, LAEFF / SVO Partner’s VO Project Census of Spanish Data Centres Partner.
The Origin and Evolution of Cosmic Magnetism: Perspective from SKA
