![]() Large APEX Bolometer Camera Bolometer Development Group Millimeter & Submillimeter Astronomy Group Max-Planck-Institut für Radioastronomie (MPIfR)
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Optics The design of
the optics for LABOCA has been rendered by E. Kreysa at MPIfR with
contributions from N. Halverson (UC
Berkeley). The limitations on the
space available in the Cassegrain cabin and the constraints due to
sharing one large common mirror with the ASZCa experiment,
required a
long, accurate and laborious optimization of the optical design,
carried out over several months with use of the software package ZEMAX.
The pictures below give an overview of the optics: on the left there is the APEX telescope, on the right a zoom on the tertiary optics installed in the Cassegrain cabin. After the telescope's primary and secondary mirrors (here named M1 and M2), the optical path is actively shaped by other 5 mirrors (here named M3, M4, M5, M6, M7) plus a lens placed at the receiver's cryostat window. Mirror M3 has
been manufactured by a machine shop of LBNL
(Berkeley)
and
is commonly used by LABOCA and the ASZCa experiment.
M3 has a diameter of 1.6 m (LABOCA uses only the
inner 80 cm circle) and surface accuracy of 20 µm (r.m.s.). It is
attached to the floor of the Cassegrain cabin, in the central area, by
means of a bearing which allows the operators to rotate the mirror to
send the telescope beam to LABOCA or to ASZCa alternatively.
![]() Click on the picture below to get a high-resolution WMF with a CAD drawing of the Cassegrain cabin with LABOCA and its optics (1.64 MB). ![]() |
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| web: gsiringo (at) mpifr-bonn.mpg.de | last edit: G. Siringo, MPIfR - August 2007 | |||||||||||