Foundation work for the Operations Support Facility (OSF) Technical Building is underway at the 9600 foot level. This building will be the nerve center of ALMA. ALMA personnel will work here, directing the operation of the Array at the 16,570 foot elevation Array Operations Site, collecting data and sending it onward to astronomers around the world. This building will be finished in 2008. For a larger picture of the site visit: OSF Building
Nearby is a temporary building for Assembly, Integration and Verification (AIV), under construction and scheduled for completion 2006 Nov 7. For a larger picture of the site visit: AIV Building
Final interior work continues at the Array Operations Site (AOS) Technical Building, which will house the electronics which bring together the signals from the antennas to be located nearby. For a picture of the site visit: AOS Building
There are about 183 persons working at the site. Most of these people live in ALMA lodging facilities elsewhere on the OSF site.
Images compliments of Dr. Seiichi Sakamoto of the Atacama Large Millimeter/Submillimeter Array (ALMA) Project Office, National Astronomical Observatory of Japan
(left) Foundation work for the Operations Support Facility (OSF) Technical Building. (right) Temporary building for Assembly, Integration and Verification (AIV).
The ALMA Project Scientist is responsible for ensuring that ALMA is constructed and commissioned in such a manner as to meet the scientific requirements of the ALMA Agreement. As a Key Staff Member of the JAO, the Project Scientist will contribute to decision making, overall policy development and strategic planning. The Project Scientist reports directly to the ALMA Director and interacts closely with the Project Manager and Project Engineer. For more information visit: ALMA Project Scientist
On May 10, 2006, NSF's Judith Sunley (Acting Assistant Director for Mathematical and Physical Sciences) notified the ALMA board that the U.S. National Science Board (NSB) has approved NSF's request for additional funding for ALMA, providing the NSF Director with spending authority that covers the revised ALMA baseline.
Minutes from the NSB meeting will be posted to http://www.nsf.gov/nsb/meetings/mtg_list.htm.
The 2nd pan-ALMA conference on "Science with ALMA: a new era for Astrophysics" will be held 13-16 November 2006 in Madrid, Spain. The venue will be the campus of the CSIC (Consejo Superior de Investigaciones Cientificas), in the centre of town. Information on the 2nd pan-ALMA meeting is available via http://www.oan.es/alma2006/.
The Atacama Large Millimeter Array (ALMA) will provide quantum leaps in improvement compared to existing facilities, enabling entirely new science at millimeter and submillimeter wavelengths. Star formation in the Milky Way will be revealed with a hundred-fold increase in sensitivity and resolution, making it possible to see evidence of protoplanets in protostellar disks and to measure disk chemical differentiation. Star-forming molecular gas in nearby galaxies will be imaged with high sensitivity at parsec-scale resolution, providing new insight into the structure and evolution of galaxies. Multiple transitions of molecular and atomic gas will be imaged in distant galaxies back to the era of recombination, providing information on the chemistry, structure, formation and evolution of the earliest galaxies.
The North American ALMA Science Center (NAASC) is sponsoring a special session at the 208th meeting of the American Astronomical Society, to be held 4-8 June 2006 in Calgary, Alberta, Canada. The special session will take place from 2:30-4:00pm on Monday June 5, in order to adjoin the meeting of the Canadian Astronomical Society (CASA). It will feature review talks highlighting ALMA's capabilities and scientific potential in three key research areas.
Speakers & Topic:
Copies of the presentations and some of the posters are available at the NAASC website at http://www.cv.nrao.edu/naasc/AAS/.
On January 13-14, Charlottesville welcomed 75 scientists from 37
institutions in nine different countries to the first NRAO North
American Science Center Workshop, "From Z-Machines to ALMA:
(Sub)millimeter Spectroscopy of Galaxies". In 26 oral and 23 poster
presentations, the participants assessed the technical challenges and
scientific promise of using wide-bandwidth spectroscopy to study
distant, dusty galaxy populations. The first day closed with a
reception sponsored by the NRAO Director, while the second ended with
a freewheeling discussion of the role played by current NRAO
facilities in this exciting scientific area, plus a view of the future
provided by North American ALMA Project Director Adrian Russell.
Proceedings for the workshop will be published by the Astronomical
Society of the Pacific before the end of 2006. The meeting program,
electronic versions of some of the presentations, and the conference
photograph (left) and candid pictures of participants (all courtesy of Jim
Condon) are available at ALMA held a Town Meeting at the
Last modified: Mon February 6, 2006