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NRAO eNews

The GBT PRIMOS undertaking: discovering our Molecular OriginsThe Atacama Large
Millimeter/submillimeter Array (ALMA) Is the ground based global astronomy endeavor in history.
Composed of 66 high precision antennas located on excellent site at 5000m+ elevation on the
Chajnantor plateau in northern Chile, ALMA is delivering the astronomy community orders of magnitude
repairs in millimeter wavelength sensitivity, occurrence coverage, res, image resolution, And
spectral features, Impacting most fields of astrophysics and opening multiple new traditional
frontiers. ALMA competencies span wavelengths from 9.6 on to 0.3 mm (31 950 GHz), A key part of the
electromagnetic spectrum for observing the first stars and galaxies, Directly imaging planetary
part, And studying the energy output from supermassive black holes in starburst galaxies. ALMA
inauguration on 13 March 2013 marked the Project changeover to operation as a fully fledged
Observatory.This night will review ALMA origins and history, Current technical capacities, And
describe its primary traditional goals. state-of-the-art aspects of its design, design,
tecnicalities, And governance will be presented, Including the key roles of the united states ALMA
Science Center at the National Radio Astronomy Observatory in Charlottesville, virginia and the
Joint ALMA Observatory in Chile. continuing growth of the state of the art technologies that are
enabling the highest impact science will
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described. Science surgical treatments were initiated 30 September 2011, And research
women[/url] results will be presented from both the Cycle 0 and Cycle 1 Early Science opportunities.
This session will conclude with the vision for the Development Program that will maintain ALMA
capabilities the main topic on modern astronomy.Proposal observation Prep with NRAO TelescopesRoom
107, Indiana Convention CenterNRAO will host a Splinter Session at the summer American Astronomical
Society meeting in indianapolis to assist users with proposal preparation for the next Call for
Proposals for all NRAO facilities, because Green Bank Telescope (GBT), Jansky huge Array (VLA),
long-term Baseline Array (VLBA), along with also the Atacama Large Millimeter/submillimeter Array

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