A&A 454, L25-L28 (2006)
DOI: 10.1051/0004-6361:20065359
Letter
APECS - the Atacama pathfinder experiment control system
D. Muders1, H. Hafok1, F. Wyrowski1, E. Polehampton1, 2, A. Belloche1, C. König1, R. Schaaf1, 3, F. Schuller1, J. Hatchell1, 4 and F. van der Tak1, 51 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
e-mail: dmuders@mpifr-bonn.mpg.de
2 Space Science and Technology Department, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UK
3 Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
4 School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK
5 SRON National Institute for Space Research, Landleven 12, 9747 AD Groningen, The Netherlands
(Received 4 April 2006 / Accepted 3 May 2006 )
Abstract
APECS is the distributed control system of the new Atacama Pathfinder
EXperiment (APEX) telescope located on the Llano de Chajnantor at an altitude
of 5107 m in the Atacama desert in northern Chile. APECS is based on Atacama
Large Millimeter Array (ALMA) software and employs a modern, object-oriented
design using the Common Object Request Broker Architecture (CORBA) as the
middleware. New generic device interfaces simplify adding instruments to the
control system. The Python based observer command scripting language allows
using many existing software libraries and facilitates creating more complex
observing modes. A new self-descriptive raw data format (Multi-Beam FITS or
MBFITS) has been defined to store the multi-beam, multi-frequency data.
APECS provides an online pipeline for initial calibration, observer feedback
and a quick-look display. APECS is being used for regular science observations
in local and remote mode since August 2005.
Key words: telescopes -- methods: data analysis -- methods: numerical -- astronomical data bases: miscellaneous
© ESO 2006

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