COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: Network Monitoring Experiment Exp. Code: N20C1 Schedule Version: 1.00 Processed by SCHED version: 11.50 Development version 11.5. Started Apr. 2 PI: Olga Bayandina Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: bayandina@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 6cm (C-band) NME and ftp fringe test for session 1/2020 (512 Mbps, L+R, 2-bit sampling, 8 MHz filters) Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 6cm NME and ftp fringe-test on 25 Feb 2020 involving 18 antennas. Jb2, Wb, Ef, O8, T6, Ur, Tr, Ys, Hh, Sv, Zc, Bd, Ir, Cm, Da, De, Kn, Pi. The NME uses a standard setup with 512 Mbps. The schedule consists of: - long integrations on calibrators J0237+2848 and J0530+1331 for ftp-fringe tests; Ftp-fringe tests are scheduled every half hour throughout the experiment (UT times): 12:23:00 (scan 2, 2 sec, J0237+2848) 12:53:00 (scan 4, 2 sec, J0237+2848) 13:23:00 (scan 6, 2 sec, J0237+2848) 13:53:00 (scan 8, 2 sec, J0530+1331) 14:23:00 (scan 10, 2 sec, J0530+1331) 14:53:00 (scan 12, 2 sec, J0530+1331) Good luck with the session! Olga Bayandina Mattermost: coms.evlbi.org Schedule for URUMQI (Code Ur ) Page 2 Network Monitoring Experiment UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Tue 25 Feb 2020 Day 56 --- ---------- N20C1 ---------- Next scan frequencies: 4966.49 4966.49 4966.49 4966.49 4982.49 4982.49 4982.49 4982.49 4998.49 4998.49 4998.49 4998.49 5014.49 5014.49 5014.49 5014.49 Next BBC frequencies: 346.49 346.49 346.49 346.49 362.49 362.49 362.49 362.49 378.49 378.49 378.49 378.49 394.49 394.49 394.49 394.49 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 12 00 00 J0237+2848 04 08 01 67.0 238.0 1.5 44.7 0 0 12 00 00 12 10 00 =0234+285 04 18 02 65.4 241.8 1.7 46.9 600 38 12 00 01 12 13 00 J0237+2848 04 21 03 64.9 242.9 1.7 47.5 178 38 12 13 00 12 25 00 =0234+285 04 33 05 63.0 246.8 1.9 49.6 720 85 12 13 01 12 28 00 J0237+2848 04 36 05 62.5 247.8 2.0 50.1 178 85 12 28 00 12 40 00 =0234+285 04 48 07 60.4 251.2 2.2 51.7 720 131 12 28 01 12 43 00 J0237+2848 04 51 08 59.9 252.1 2.2 52.1 178 131 12 43 00 12 55 00 =0234+285 05 03 10 57.8 255.2 2.4 53.2 720 177 12 43 01 12 58 00 J0237+2848 05 06 10 57.3 255.9 2.5 53.5 178 177 12 58 00 13 10 00 =0234+285 05 18 12 55.1 258.7 2.7 54.4 720 223 12 58 01 13 13 00 J0237+2848 05 21 13 54.6 259.3 2.7 54.5 178 223 13 13 00 13 25 00 =0234+285 05 33 15 52.5 261.9 2.9 55.1 720 269 13 13 01 13 29 00 J0530+1331 05 37 15 60.1 182.5 0.1 1.9 155 269 13 29 00 13 40 00 =0528+134 05 48 17 59.9 187.9 0.3 5.9 660 312 13 29 01 13 43 00 J0530+1331 05 51 18 59.8 189.3 0.3 6.9 178 312 13 43 00 13 55 00 =0528+134 06 03 20 59.3 195.0 0.5 11.2 720 358 13 43 01 13 58 00 J0530+1331 06 06 20 59.2 196.4 0.6 12.2 178 358 13 58 00 14 10 00 =0528+134 06 18 22 58.5 201.9 0.8 16.2 720 404 13 58 01 14 13 00 J0530+1331 06 21 23 58.3 203.2 0.8 17.1 178 404 14 13 00 14 25 00 =0528+134 06 33 25 57.3 208.4 1.0 20.8 720 450 14 13 01 14 28 00 J0530+1331 06 36 25 57.0 209.7 1.1 21.7 178 450 14 28 00 14 40 00 =0528+134 06 48 27 55.9 214.5 1.3 25.0 720 496 14 28 01 14 43 00 J0530+1331 06 51 28 55.6 215.7 1.3 25.8 178 496 14 43 00 14 55 00 =0528+134 07 03 30 54.2 220.2 1.5 28.8 720 542 14 43 01 Schedule for URUMQI (Code Ur ) Page 3 Network Monitoring Experiment UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Tue 25 Feb 2020 Day 56 --- 14 58 00 J0530+1331 07 06 30 53.9 221.3 1.6 29.5 178 542 14 58 00 15 00 00 =0528+134 07 08 30 53.6 222.0 1.6 30.0 120 550 14 58 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess120.C512 --- WARNING --- This group does not match an entry in the frequency catalog. This might be ok because the catalog is not complete. But be very careful to be sure that the setup is correct. Setup group: 12 Station: URUMQI Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 4620.00 Net SB= L L U U L L U U L L U U L L U U IF SB = U U U U U U U U U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 9 1 9 2 10 2 10 3 11 3 11 4 12 4 12 BBC SB= L L U U L L U U L L U U L L U U IF = A2 C1 A2 C1 A2 C1 A2 C1 A2 C1 A2 C1 A2 C1 A2 C1 The following frequency sets based on these setups were used. Frequency Set: 6 Setup file default. Used with PCAL = off LO sum= 4966.49 4966.49 4966.49 4966.49 4982.49 4982.49 4982.49 4982.49 4998.49 4998.49 4998.49 4998.49 5014.49 5014.49 5014.49 5014.49 BBC fr= 346.49 346.49 346.49 346.49 362.49 362.49 362.49 362.49 378.49 378.49 378.49 378.49 394.49 394.49 394.49 394.49 Bandwd= 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 Matching frequency sets: 6 Track assignments are: track1= 18, 26, 2, 10, 20, 28, 4, 12, 22, 30, 6, 14, 24, 32, 8, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 0234+285 02 34 55.589590 * 02 37 52.405677 02 39 02.102749 0.00 * J0237+2848 28 35 11.40773 * 28 48 08.98999 28 53 16.94302 0.00 J0237+28 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 58420 observations. 0528+134 05 28 06.759216 * 05 30 56.416746 05 32 04.166514 0.21 * J0530+1331 13 29 42.28882 * 13 31 55.14948 13 32 41.13647 0.24 J0530+13 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 138236 observations. SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Setup file Frequency sets Observing hours (duplicates not shown) Scan Baseline J0237+2848 sess120.C512 1 2 3 4 5 6 7 8 9 10 14 1.167 178.500 J0530+1331 sess120.C512 1 2 3 4 5 6 7 8 9 10 14 1.217 184.245 EFFECT OF SOLAR CORONA The solar corona can cause unstable phases for sources too close to the Sun. SCHED provides warnings at individual scans for distances less than 10 degrees. The distance from the Sun to each source in this schedule is: Source Sun distance (deg) J0237+2848 70.5 J0530+1331 106.5 Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes that the Sun will cause amplitude reductions on the longest VLBA baselines at a solar distance of 60deg F^(-0.6) where F is in GHz. For common VLBI bands, this is: 327 MHz 117. deg 610 MHz 81. deg 1.6 GHz 45. deg 2.3 GHz 36. deg 5.0 GHz 23. deg 8.4 GHz 17. deg 15.0 GHz 12. deg 22.0 GHz 9. deg 43.0 GHz 6. deg