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VLBI Observations and Call


In October 2002 and April 2003, two global VLBI experiments at 3mm wavelength have taken place involving both IRAM instruments, with the 6-antenna Plateau de Bure in phased-array mode for the first time. The IRAM 30-m telescope has already prooved its value in global VLBI observations for many years, but these two experiments now have shown that also the Plateau de Bure can work reliably as a phased array VLBI station. Both IRAM instruments are now ready to offer observing time in VLBI mode to the scientific community.

Call for Global VLBI Proposals at 3mm wavelength

We announce the opportunity for coordinated, high angular resolution and high sensitivity GLOBAL VLBI observations in the 3mm band (85 - 95 GHz), complementing existing stand-alone VLBA observations at this frequency. The Global 3mm VLBI Array consists of 8 VLBA antennas equipped with 3mm receivers, plus the IRAM 30-m telescope on Pico Veleta (Spain), the IRAM phased 6-element interferometer on Plateau de Bure (France), and the MPIfR 100-m radio telescope in Effelsberg (Germany). Other telescopes may join later.

The Global 3mm VLBI Array is the successor to the former Coordinated Millimeter VLBI Array (CMVA) and offers 3 to 4 times more sensitivity than the stand-alone VLBA. Observations with the Global 3mm VLBI array will be scheduled in time blocks in special observing sessions, performed twice per year. The next two sessions are tentatively planned for April 16-21, 2004 and October 8-13, 2004. The actual duration of each session will depend on proposal pressure.

The Global 3mm VLBI Array basically supports the same observing modes as the VLBA. For standard continuum observations the VLBI recording will be done at 256 Mbit/s (corresponding to a bandwith of 128 MHz). Correlation will be performed in absentia at the MPIfR MK4 correlator in Bonn unless some technical reason for using another correlator is given in the proposal. The P.I. will receive the correlated data in uv-fits format.

Proposals for the April 2004 session should be prepared in a similar fashion as ``normal cm-VLBI proposals'', using the standard VLBI cover sheet and instructions available on the web under URL and should be submitted electronically as e-mail before

October 1st 2003, the normal VLBI deadline

to the following two addresses (in copy):


Proposals will be reviewed by NRAO and the participating European Observatories.

The European Schedule Coordinator, Dr. R. Porcas (MPIfR), will forward proposal copies to the participating European Institutes and ensure the scientific evaluation of the proposals by the respective local committees. Finally, the referee ratings of these observatories and the NRAO will be combined.

Global VLBI observations at 3mm are subject to some technical restrictions, which are summarized on the following web-page

( The following persons are ready to provide help: at IRAM: Dr. Michael BREMER ( and at MPIfR: Dr. Thomas Krichbaum (

The IRAM and MPIfR VLBI teams

next up previous
Next: VLBI: what changes compared Up: IRAM Newsletter 56 (August 2003) Previous: Call for Observing Proposals