DocumentCode
2734504
Title
ALMA and Sub-millimeter-wave Astronomy
Author
Lo, Fred K Y
Author_Institution
Nat. Radio Astron. Obs., Charlottesville
fYear
2006
fDate
18-22 Sept. 2006
Firstpage
3
Lastpage
3
Abstract
The Atacama Large Millimeter/submillimeter Array (ALMA) will be the premier millimeter and submillimeter telescope in the world when completed in 2012. ALMA will be a transformational telescope that allows astronomers to image and study at unprecedented detail the origin of stars and planets, galaxies and biologically relevant chemistry, fundamental issues in our attempt to understand how the Universe developed. ALMA represents a qualitative step forward - it will be 10-100 times more sensitive and have 10-100 times better angular resolution than any current telescope working at these wavelengths. The combination of unprecedented sensitivity and excellent resolution of ALMA will transform the astrophysics of the birth of planets, stars and galaxies from the realm of largely theoretical modeling to the realm of directly viewing nature at work. The current status of ALMA will be described. Other submillimeter astronomical projects currently under construction or consideration will also be described.
Keywords
radiotelescopes; submillimetre astronomy; ALMA; Atacama Large Millimeter/submillimeter Array; astrophysics; submillimeter astronomical projects; submillimeter telescope; submillimeter-wave astronomy; transformational telescope; Antenna arrays; Astrochemistry; Astrophysics; Earth; Europe; North America; Observatories; Planets; Radio astronomy; Telescopes;
fLanguage
English
Publisher
ieee
Conference_Titel
Infrared Millimeter Waves and 14th International Conference on Teraherz Electronics, 2006. IRMMW-THz 2006. Joint 31st International Conference on
Conference_Location
Shanghai
Print_ISBN
1-4244-0400-2
Electronic_ISBN
1-4244-0400-2
Type
conf
DOI
10.1109/ICIMW.2006.368213
Filename
4221947
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