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Subsections
Albrecht Sievers is now working in the Computer Group
of IRAM Granada. He will still be available as a Friend of
the Telescope and have some time to pursue his scientific
projects.
A team from the Spanish National Geographical Institute (IGN) has
determined the telescope's deviation from the vertical.
These data combined with inclinometer measurements will be used to
further improve our pointing model.
Large parts of the Sierra Nevada have been declared a Nature Park. This has
the consequence that a special identification is required to access the
observatory by car. During night time also a key is required to open a
gate to the access road. Visitors who want to go to the telescope by
taxi or rental car should contact Javier Lobato
(lobato@iram.es) or
Esther Franzin
(franzin@iram.es)
several days in advance.
Juan Peñalver has compiled a CD-ROM with photos from the Pico Veleta
Observatory and the 30-m telescope. If you are interested in a copy,
send him an email
(penalver@iram.es).
The observer can now determine the rejection of the image sideband (Gi)
for any of our heterodyne receivers using the OBS command
CALIBRATE /SSB rxname. This command measures the value of Gi using
a Martin-Puplett-Interferometer (but does not automatically change
Gi in OBS).
Under normal circumstances it is not necessary to use this command
since a high rejection is obtained in the automatic tuning process.
It might be useful if one is looking for very weak lines in ``crowded''
sources like Orion or SgrB2, for frequencies close to the limits of
the tuning range or if an extremely small calibration uncertainty of a
few percent is required. For more information use the HELP command
in OBS.
Rainer MAUERSBERGER
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bremer@iram.fr