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ALMA: status report on construction and early results from commissioning
| Content Provider | Semantic Scholar |
|---|---|
| Author | Hills, Richard E. Kurz, Richard Peck, Alison B. |
| Copyright Year | 2010 |
| Abstract | The Atacama Large Millimeter/submillimeter Array (ALMA) is an international facility at an advanced stage of construction in the Atacama region of northern Chile. ALMA will consist of two arrays of high-precision antennas: one made up of twelve 7-meter diameter antennas operating in closely-packed configurations of about 50m in diameter, and the other of up to sixty-four 12-meter antennas arranged in configurations with diameters ranging from about 150 meters to 15 km. There will be four more 12-meter antennas to provide the "zero-spacing" information, which is critical for making accurate images of extended objects. The antennas will be equipped with sensitive millimeter-wave receivers covering most of the frequency range 84 to 950 GHz. State-of-the-art microwave, digital, photonic and software systems will capture the signals, transfer them to the central building and correlate them, while maintaining accurate synchronization. ALMA will provide images of a wide range of astronomical objects with great sensitivity and very high spectral resolution. The images will have much higher "fidelity" than those from existing mm/submm telescopes. This paper gives an update on the status of construction and on progress with the testing and scientific commissioning. |
| File Format | PDF HTM / HTML |
| DOI | 10.1117/12.857017 |
| Volume Number | 7733 |
| Alternate Webpage(s) | http://www.eso.org/sci/libraries/SPIE2010/7733-38.pdf |
| Alternate Webpage(s) | https://doi.org/10.1117/12.857017 |
| Journal | Astronomical Telescopes + Instrumentation |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Report |