2 research outputs found
The Yuan-Tseh Lee Array for Microwave Background Anisotropy
The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the
first interferometer dedicated to studying the cosmic microwave background
(CMB) radiation at 3mm wavelength. The choice of 3mm was made to minimize the
contributions from foreground synchrotron radiation and Galactic dust emission.
The initial configuration of seven 0.6m telescopes mounted on a 6-m hexapod
platform was dedicated in October 2006 on Mauna Loa, Hawaii. Scientific
operations began with the detection of a number of clusters of galaxies via the
thermal Sunyaev-Zel'dovich effect. We compare our data with Subaru weak lensing
data in order to study the structure of dark matter. We also compare our data
with X-ray data in order to derive the Hubble constant.Comment: accepted for publication in ApJ (13 pages, 7 figures); a version with
high resolution figures available at
http://www.asiaa.sinica.edu.tw/~keiichi/upfiles/AMiBA7/pho_highreso.pd
The AMiBA Hexapod Telescope Mount
AMiBA is the largest hexapod astronomical telescope in current operation. We
present a description of this novel hexapod mount with its main mechanical
components -- the support cone, universal joints, jack screws, and platform --
and outline the control system with the pointing model and the operating modes
that are supported. The AMiBA hexapod mount performance is verified based on
optical pointing tests and platform photogrammetry measurements. The
photogrammetry results show that the deformations in the inner part of the
platform are less than 120 micron rms. This is negligible for optical pointing
corrections, radio alignment and radio phase errors for the currently
operational 7-element compact configuration. The optical pointing error in
azimuth and elevation is successively reduced by a series of corrections to
about 0.4 arcmin rms which meets our goal for the 7-element target
specifications.Comment: Accepted for ApJ, 33 pages, 15 figure