The LMT at 10 degrees elevation
The ongoing tests have shown that the LMT
mechanical and electrical drive-systems are performing well.
The first holography campaign using the 12 GHz holography
receiver system successfully demonstrated its capability and
the readiness of the software system. Following the installation and
commissioning of the actuator system,
measurements and adjustments of surface panel-segments will be
made over the inner 30-m diameter to improve the efficiency
of the telescope surface. The outer two rings of segments,
providing the full 50-m diameter surface will be installed at
a later date. Temporary panels in rings 4 and 5 are currently
in place providing the required mass to maintain the balance
and thermal environment of the telescope antenna structure.
FCRAO is supported by NSF grant AST 05-40852
