COVER INFORMATION Station: WSTRBORK (Code Wb ) 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 WSTRBORK (Code Wb ) 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: 379.49 379.49 379.49 379.49 395.49 395.49 395.49 395.49 411.49 411.49 411.49 411.49 427.49 427.49 427.49 427.49 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 22 45 41 41.5 95.8 -3.9 0.0 0 0 12 00 00 12 10 00 =0234+285 22 55 42 43.0 97.9 -3.7 0.0 600 39 12 00 01 12 13 00 J0237+2848 22 58 43 43.4 98.6 -3.7 0.0 169 39 12 13 00 12 25 00 =0234+285 23 10 45 45.2 101.3 -3.5 0.0 720 85 12 13 01 12 28 00 J0237+2848 23 13 45 45.7 102.0 -3.4 0.0 169 85 12 28 00 12 40 00 =0234+285 23 25 47 47.4 104.8 -3.2 0.0 720 131 12 28 01 12 43 00 J0237+2848 23 28 48 47.9 105.6 -3.2 0.0 169 131 12 43 00 12 55 00 =0234+285 23 40 50 49.6 108.6 -3.0 0.0 720 178 12 43 01 12 58 00 J0237+2848 23 43 50 50.0 109.4 -2.9 0.0 169 178 12 58 00 13 10 00 =0234+285 23 55 52 51.7 112.5 -2.7 0.0 720 224 12 58 01 13 13 00 J0237+2848 23 58 53 52.1 113.4 -2.7 0.0 169 224 13 13 00 13 25 00 =0234+285 00 10 55 53.8 116.8 -2.5 0.0 720 271 13 13 01 13 29 00 J0530+1331 00 14 55 17.2 90.2 -5.3 0.0 85 271 13 29 00 13 40 00 =0528+134 00 25 57 18.9 92.4 -5.1 0.0 660 313 13 29 01 13 43 00 J0530+1331 00 28 58 19.3 93.0 -5.1 0.0 169 313 13 43 00 13 55 00 =0528+134 00 40 59 21.1 95.4 -4.9 0.0 720 359 13 43 01 13 58 00 J0530+1331 00 44 00 21.6 96.1 -4.8 0.0 169 359 13 58 00 14 10 00 =0528+134 00 56 02 23.4 98.6 -4.6 0.0 720 406 13 58 01 14 13 00 J0530+1331 00 59 02 23.8 99.2 -4.6 0.0 169 406 14 13 00 14 25 00 =0528+134 01 11 04 25.6 101.7 -4.3 0.0 720 452 14 13 01 14 28 00 J0530+1331 01 14 05 26.1 102.4 -4.3 0.0 169 452 14 28 00 14 40 00 =0528+134 01 26 07 27.8 105.0 -4.1 0.0 720 499 14 28 01 14 43 00 J0530+1331 01 29 07 28.3 105.7 -4.0 0.0 169 499 14 43 00 14 55 00 =0528+134 01 41 09 30.0 108.4 -3.8 0.0 720 545 14 43 01 Schedule for WSTRBORK (Code Wb ) 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 01 44 10 30.4 109.0 -3.8 0.0 169 545 14 58 00 15 00 00 =0528+134 01 46 10 30.7 109.5 -3.8 0.0 120 553 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: 5 Station: WSTRBORK Total bit rate: 512 Format: VDIF 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= 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 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 = A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 2 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= 379.49 379.49 379.49 379.49 395.49 395.49 395.49 395.49 411.49 411.49 411.49 411.49 427.49 427.49 427.49 427.49 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: 2 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 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