For any questions regarding the telescope and the control programs, we recommend to consult the NCS web pages (../IRAMES/ncs30m) and our page with the summary of telescope parameters.
The report entitled ``Calibration of spectral line data at the IRAM 30m telescope'' explains in detail the applied calibration procedure. Both documents can be retrieved from the URL ../IRAMES/otherDocuments/manuals/index.html. A catalog of well calibrated spectra for a range of sources and transitions (Mauersberger et al. [9]) is very useful for monitoring spectral line calibration. A copy of the 30m file with the calibrated spectra can be downloaded from the Spanish web site.
The astronomer on duty (whose schedule can be found at URL /IRAMES/mainWiki/AstronomerOnDutySchedule) should be contacted well in advance for any special questions concerning the preparation of an observing run.
Frequency switching is available for both HERA and the single pixel
SIS receivers. This observing mode is interesting for observations
of narrow lines where flat baselines are not essential, although
the spectral baselines with HERA are among the best known in frequency
switching. Certain limitations exist with respect
to maximum frequency throw (
km/s),
backends, phase times etc.; for a detailed report see [4].
This report also explains how to identify mesospheric lines which may
easily be confused in some cases with genuine astronomical lines from cold
clouds.
If your observations with the 30-m telescope results in a publication, please acknowledge this in a footnote "Based on observations with the IRAM 30-m telescope. IRAM is supported by CNRS/INSU (France), the MPG (Germany) and the IGN (Spain). Please email a copy of the publication to Dennis Downes (downes@iram.fr).