Evaluation of the ALMA Prototype Antennas
arXiv:astro-ph/0609329 · doi:10.1086/508298
Abstract
The ALMA North American and European prototype antennas have been evaluated by a variety of measurement systems to quantify the major performance specifications. Nearfield holography was used to set the reflector surfaces to 17 microns RMS. Pointing and fast switching performance was determined with an optical telescope and by millimeter wavelength radiometry, yielding 2 arcsec absolute and 0.6 arcsec offset pointing accuracies. Path length stability was measured to be less than or approximately equal to 20 microns over 10 minute time periods using optical measurement devices. Dynamical performance was studied with a set of accelerometers, providing data on wind induced tracking errors and structural deformation. Considering all measurements made during this evaluation, both prototype antennas meet the major ALMA antenna performance specifications.
83 pages, 36 figures, AASTex format, to appear in PASP September 2006 issue
Cited by in corpus (16)
- First M87 Event Horizon Telescope Results. II. Array and Instrumentation
- The Atacama Large Millimeter/submillimeter Array
- CMB-S4 Science Case, Reference Design, and Project Plan
- Wide field aplanatic two-mirror telescopes for ground-based gamma-ray astronomy
- Observing the Sun with Atacama Large Millimeter/submillimeter Array (ALMA): High Resolution Interferometric Imaging
- Near-Field Radio Holography of Large Reflector Antennas
- Precipitable Water Vapor, Temperature, and Wind Statistics At Sites Suitable for mm and Submm Wavelength Astronomy in Northern Chile
- First Very Long Baseline Interferometry Detections at 870μm
- Mechanical Measurements of the ALMA Prototype Antennas
- Study of the Dynamics of Large Reflector Antennas with Accelerometers
- First-generation Science Cases for Ground-based Terahertz Telescopes
- Pulsar Timing Sensitivity to Very-Low-Frequency Gravitational Waves
- Greenland Telescope Project --- Direct Confirmation of Black Hole with Sub-millimeter VLBI
- Advanced Gain Calibration Techniques in Radio Interferometry
- Betelgeuse scope: Single-mode-fibers-assisted optical interferometer design for dedicated stellar activity monitoring
- CTbend: A Bayesian open-source framework to model pointing corrections for Cherenkov telescopes