============================================================================================================================ Schedule Version 1.4 (16 Sep. 2019) GMVA OCT 2019 ====================================== ================== Updates: 16sep19: move start time for MM017A to 277-0430 (EU) and 277-0600 (US) 05sep19: for VLBA change start time for MB011B, and stop time in Europe 28aug19: Added slot on day 278 for polarisation calibration 23aug19: Time for Cui et al. extended to compensate for different duty cycle in original proposal ============================================================================================================================ START CODE PI PROGRAM POL DAY NO. UT-START UT-STOP STATIONS COMMENTS ======== ============== ================== === ====== =========== =========== ==================== =============== CAL ROTTMANN Gain Calibration L+R Eu 276 1000(03/10)-1200(03/10) Pv Eb Ys On Mh KVN see comment 1 TEST KRICHBAUM Fringe-test L+R Eu 276 1200(03/10)-1400(03/10) Pv Eb Ys On Mh see comment 2 MC004 CUI 1803+784 L+R Eu 276 1830(03/10)-0430(04/10) Pv Eb Ys On Mh see comment 3 KV 276 1830(03/10)-0430(04/10) KVN US 276 1830(03/10)-0430(04/10) VLBA (no GBT) +GLT see comment 4 MM017A MARSCHER FERMI sources L+R Eu 277 0430(04/10)-0730(05/10) Pv Eb Ys On Mh 24 hours KV 277 0730(04/10)-0730(05/10) KVN 24 hours US 277 0600(04/10)-0730(05/10) VLBA (no GBT) +GLT 24 hours, see 4 CAL KRICHBAUM Polaris. Calib L+R Eu 278 0900(05/10)-1300(05/10) Pv Eb Ys On Mh see comment 5 KV 278 0900(05/10)-1300(05/10) KVN see comment 5 US 278 0900(05/10)-1300(05/10) VLBA (no GBT) + GLT see comment 5 MB011B BACH Cygnus A L+R Eu 278 1315(05/10)-0300(06/10) Pv Eb Ys On Mh +GLT KV 278 1315(05/10)-1800(05/10) KVN (Part I) source setting KV 279 0300(06/10)-0930(06/10) KVN (Part II) source rising US 278 1930(05/10)-0930(06/10) VLBA (no GBT) + GLT ========================================================================================================================= Comments: (1) Nominal period for station amplitude calibration, as requested by the GMVA Technical Group (GTG). The actual period when amplitude calibration is performed can be chosen by each individual observatory. Antenna temperature measurement of a suitable planet or other primary flux calibrator is recommended. (2) Traditional fringe-verification test. This specific 2-hour interval was recommended by the GTG. (3) Requested GST 19-01 assuming a duty cycle of 75%, time extended to 18:30 to 04:30 UT (4) Participation of LMT and GLT telescopes must be arranged by the PIs (5) Period for polarisation and additional calibration ====================================================================================================================== Contact email addresses for PIs ------------------------------- MC004 yuzhu.cui@nao.ac.jp MM017A marscher@bu.edu MB011B ubach@mpifr-bonn.mpg.de ======================================================================================================================