COVER INFORMATION Station: WSTRBORK (Code Wb ) Experiment: Network Monitoring Experiment Exp. Code: N21X1 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Benito Marcote Address: JIVE Oude Hoogeveensedijk 4 7991PD Dwingeloo The Netherlands Phone: +31 521 596 508 EMAIL: marcote@jive.eu Fax: Phone during observation: +31 521 596 508 Observing mode: Notes: 3.6cm NME and ftp fringe test for Session 1 2021 (2048 Mbps, L+R, 2-bit sampling, 32 MHz filters) Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 3.6cm NME and ftp fringe-test on 12 March 2021 involving the following antennas: Wb, Ef, Mc, Nt, On60, T6, Ur, Ys, Hh, Sv, Zc, Bd, Ir, Km. The NME uses a standard setup with 2048 Mbps. The schedule consists of long integrations on calibrators J0237+2848 and DA193 for ftp-fringe tests. The following ftp-fringe tests are scheduled throughout the experiment (UT times): 12:10:00 (scan 2, 2 sec, J0237+2848) 12:40:00 (scan 4, 2 sec, J0237+2848) 13:10:00 (scan 6, 2 sec, J0237+2848) 13:40:00 (scan 8, 2 sec, J0237+2848) 14:10:00 (scan 10, 2 sec, DA193) 14:40:00 (scan 12, 2 sec, DA193) Good luck with the session! Benito Marcote 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 ---------------------------------------------------------------------------------------- --- Fri 12 Mar 2021 Day 71 --- Next scan frequencies: 8383.49 8383.49 8383.49 8383.49 8447.49 8447.49 8447.49 8447.49 Next BBC frequencies: 371.49 371.49 371.49 371.49 435.49 435.49 435.49 435.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 12 00 00 J0237+2848 23 47 48 50.6 110.4 -2.9 0.0 0 0 12 00 00 12 02 00 =0234+285 23 49 49 50.9 110.9 -2.8 0.0 120 15 12 00 01 12 07 00 J0237+2848 23 54 49 51.6 112.2 -2.7 0.0 289 15 12 07 00 12 12 00 =0234+285 23 59 50 52.3 113.6 -2.7 0.0 300 54 12 07 01 12 15 00 J0237+2848 00 02 51 52.7 114.5 -2.6 0.0 169 54 12 15 00 12 27 00 =0234+285 00 14 53 54.3 117.9 -2.4 0.0 720 147 12 15 01 12 30 00 J0237+2848 00 17 53 54.7 118.8 -2.4 0.0 169 147 12 30 00 12 42 00 =0234+285 00 29 55 56.3 122.6 -2.2 0.0 720 240 12 30 01 12 45 00 J0237+2848 00 32 56 56.7 123.6 -2.1 0.0 169 240 12 45 00 12 57 00 =0234+285 00 44 58 58.1 127.6 -1.9 0.0 720 332 12 45 01 13 00 00 J0237+2848 00 47 58 58.5 128.7 -1.9 0.0 169 332 13 00 00 13 12 00 =0234+285 01 00 00 59.9 133.1 -1.7 0.0 720 425 13 00 01 13 15 00 J0237+2848 01 03 01 60.2 134.2 -1.6 0.0 169 425 13 15 00 13 27 00 =0234+285 01 15 02 61.4 139.0 -1.4 0.0 720 518 13 15 01 13 30 00 J0237+2848 01 18 03 61.7 140.2 -1.4 0.0 169 518 13 30 00 13 42 00 =0234+285 01 30 05 62.8 145.3 -1.2 0.0 720 611 13 30 01 13 45 00 DA193 01 33 05 44.4 79.0 -4.4 0.0 4 611 13 45 00 13 57 00 --- 01 45 07 46.2 81.1 -4.2 0.0 720 703 13 45 01 14 00 00 DA193 01 48 08 46.6 81.6 -4.1 0.0 169 703 14 00 00 14 12 00 --- 02 00 10 48.4 83.7 -3.9 0.0 720 796 14 00 01 14 15 00 DA193 02 03 10 48.9 84.3 -3.9 0.0 169 796 14 15 00 14 27 00 --- 02 15 12 50.7 86.5 -3.7 0.0 720 889 14 15 01 14 30 00 DA193 02 18 13 51.1 87.1 -3.6 0.0 169 889 14 30 00 14 42 00 --- 02 30 15 52.9 89.4 -3.4 0.0 720 982 14 30 01 14 45 00 DA193 02 33 15 53.4 90.0 -3.4 0.0 169 982 14 45 00 14 57 00 --- 02 45 17 55.2 92.5 -3.2 0.0 720 1074 14 45 01 14 58 00 DA193 02 46 17 55.4 92.7 -3.2 0.0 49 1074 14 58 00 15 00 00 --- 02 48 18 55.7 93.1 -3.1 0.0 120 1090 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: sess121.X2048 --- 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: 14 Station: WSTRBORK Total bit rate: 1024 Format: VDIF Bits per sample: 2 Sample rate: 64.000 Number of channels: 8 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 8012.00 8012.00 8012.00 8012.00 8012.00 8012.00 8012.00 8012.00 Net SB= L L U U L L U U IF SB = U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 9 1 9 2 10 2 10 BBC SB= L L U U L L U U IF = A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 1 Setup file default. Used with PCAL = off LO sum= 8383.49 8383.49 8383.49 8383.49 8447.49 8447.49 8447.49 8447.49 BBC fr= 371.49 371.49 371.49 371.49 435.49 435.49 435.49 435.49 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 1 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8 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 05.377543 0.00 * J0237+2848 28 35 11.40773 * 28 48 08.98999 28 53 33.10867 0.00 J0237+28 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 58420 observations. 0552+398 05 52 01.407168 * 05 55 30.805611 05 56 58.506778 0.00 J0555+3948 39 48 21.94581 * 39 48 49.16496 39 49 04.86148 0.00 * DA193 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J0555+39 GSFC 2016a X/S astro solution, 415688 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 sess121.X2048 1 2 3 4 5 6 7 8 9 10 14 1.317 119.817 DA193 sess121.X2048 1 2 3 4 5 6 7 8 9 10 14 1.033 93.536 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 55.2 DA193 96.9 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