Open Access Paper
22 June 2014 ALMA update (Presentation Video)
Pierre Cox
Author Affiliations +
Abstract
The Atacama Large Millimeter/submillimeter Array is transitioning from construction to operations. This connected element array currently operates from wavelengths of 3-mm to 350-microns with up to 66 array elements, 54 of 12-m diameter and 12 of 7-m diameter. While the antennas and most of the hardware for the receivers are on site, array capabilities are still expanding rapidly. In parallel with construction activities, early science observations have been going on since October 2011. At the time of the meeting, ALMA will be starting the third cycle of observing with many exciting, fundamental results already obtained. We will present the current status of the project and give an overview of the trailblazing science results obtained so far. The potential of the fully operational ALMA will be outlined as well as some of the development projects that are considered. In summary, this talk will address the past, present and future of ALMA, describe the transformational science that is and will be produced with ALMA.
00031_psisdg9143_914311_page_1_1.jpg
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Pierre Cox "ALMA update (Presentation Video)", Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 914311 (22 June 2014); https://doi.org/10.1117/12.2063484
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Video

Antennas

Infrared telescopes

Receivers

Current controlled current source

Extremely high frequency

Infrared radiation

RELATED CONTENT

The Spitzer Space Telescope: the first 30 months
Proceedings of SPIE (June 10 2006)
The Large Millimeter Telescope status
Proceedings of SPIE (February 04 2003)
APEX: five years of operations
Proceedings of SPIE (July 29 2010)

Back to Top