Dear Observatory Staff and Global 3mm VLBI PIs, Please find below Version 1 of the Block Schedule for the coming Global 3mm VLBI session in May. The projects which are scheduled have been approved by the VLBA Scheduler and myself, on the basis of the proposal reviews in Europe and at NRAO. Thomas Krichbaum will assist in making an integrated observing schedule for the session, and PIs are asked to contact him, to specify to what extent they wish to be involved in the schedule making for the part of the schedule when their source(s) is (are) being observed. ===> Please contact him by 7th APRIL. ********* The final, integrated schedule for the session will be made available to the observatories by 21st APRIL, 2 weeks before the start of the session on 5th MAY. Antennas -------- The antennas available at the VLBA are NL,FD,LA,PT,KP,BR,OV,MK. The European telescopes ("Eu" on the block schedule) are Pico Veleta, Plateau de Bure, Effelsberg, Onsala-20m and (possibly) Metsahovi. Recording mode -------------- All GMVA continuum projects will be observed with a recorded bit-rate of 512 Mb/s, since at 3mm wavelength the short atmospheric coherence is the main limitation to detection sensitivity. All observatories will record using MK5 disk systems, with correlation at the Bonn DiFX software correlator. MK5 disk availability, and VLBA disk-change logistics will determine the fraction of the scheduled time which can be spent recording data. Walter Alef will make a final decision on this when all the constraints have been considered. Polarization ------------ Note that GF017A, GT009 and GM066A all request dual LHC+RHC recording at observatories where this is possible. General considerations ---------------------- ===> Please contact me (porcas@mpifr-bonn.mpg.de) IMMEDIATELY if you find any mistakes or problems with this version of the schedule. Regards Richard Porcas (European Global 3mm VLBI Scheduler) ==================================================================================================== Schedule Version 1.0 (24 March) GMVA MAY 2011 ================================ ================= START CODE PI SOURCE POL DAY NO. UT-START UT-STOP COMMENTS ====== ============= ================== === ====== =========== =========== ================== GL035B LOBANOV source survey L Eu 125 1900(05/05)-0500(07/05) 34 hours US 125 1900(05/05)-0500(07/05) 34 hours GT009 TRIPPE 3C84 polarization L+R Eu 127 0500(07/05)-2100(07/05) US 127 1030(07/05)-0100(08/05) GF016A FUHRMANN PKS 1502+107 L+R Eu 127 2200(07/05)-0600(08/05) US 128 0100(08/05)-1200(08/05) GM066A MARSCHER Gamma-ray Blazars L+R Eu 128 0600(08/05)-2400(10/05) 66 hours US 128 1200(08/05)-2400(10/05) 60 hours ====================================================================================================