Abstract
The Atacama Large Millimeter Array (ALMA), a joint project between Europe and the U.S. and at present in its design and development phase, is a major new ground based telescope facility for millimeter and submillimeter astronomy. Its huge collecting area (7000 m2), sensitive receivers and location at one of the driest sites on Earth will make it a unique instrument. We present preliminary design concepts for the overall receiver configuration. Optics and cryostat design concepts from OSO, OVRO, RAL, IRAM, NRAO and SRON and their main features are described.
| Original language | English |
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| Title of host publication | Proc. SPIE 4015, Radio Telescopes |
| Editors | H.R. Butcher |
| Publisher | SPIE.Digital Library |
| Pages | 320-327 |
| Number of pages | 8 |
| Volume | 4015 |
| DOIs | |
| Publication status | Published - 2000 |
| Event | Astronomical Telescopes and Instrumentation, 2000, Munich, Germany - Munich, Germany Duration: 29-Mar-2000 → 30-Mar-2000 |
Conference
| Conference | Astronomical Telescopes and Instrumentation, 2000, Munich, Germany |
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| Country/Territory | Germany |
| City | Munich |
| Period | 29/03/2000 → 30/03/2000 |