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
Link To Document :
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