COVER INFORMATION Station: CAMBG32M (Code Cm ) Experiment: Network Monitoring Experiment Exp. Code: N20C3 Schedule Version: 2.00 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: 6cm NME and ftp fringe test for Session 3 2020 (2 Gbps, L+R, 2-bit sampling, 32 MHz filters) v2: includes a 4Gbps portion at the end COVER LETTER: This is the schedule for the 6cm NME and ftp fringe-test on 29 October 2020 involving the following antennas: Jb2, Wb, Ef, Mc, On85, T6, Ur, Tr, Ys, Hh, Sv, Zc, Bd, Ir, Km, Cm, Da, De, Pi, Kn. The NME uses a standard setup with 2048 Mbps. The schedule consists of long integrations on calibrators J1751+0939 and J2031+1219 for ftp-fringe tests. The following ftp-fringe tests are scheduled throughout the experiment (UT times): 11:15:00 (scan 2, 2 sec, J1751+0939) 11:45:00 (scan 4, 2 sec, J1751+0939) 12:15:00 (scan 6, 2 sec, J1751+0939) 12:45:00 (scan 8, 2 sec, J1751+0939) *** 4Gbps portion *** 13:15:00 (scan 10, 2 sec, J2031+1219) 13:45:00 (scan 12, 2 sec, J2031+1219) Good luck with the session! Benito Marcote Mattermost: coms.evlbi.org Schedule for CAMBG32M (Code Cm ) 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 ---------------------------------------------------------------------------------------- --- Thu 29 Oct 2020 Day 303 --- Next scan frequencies: 4958.49 4958.49 Next BBC frequencies: 705.51 705.51 Next scan bandwidths: 64.00 64.00 11 00 00 J1751+0939 13 33 06 22.9 464.3 -4.3 -37.1 0 0 11 00 00 11 02 00 =1749+096 13 35 07 23.2 464.8 -4.3 -37.0 120 8 11 00 01 11 07 00 J1751+0939 13 40 07 24.0 465.8 -4.2 -36.8 295 8 11 07 00 11 17 00 =1749+096 13 50 09 25.4 468.0 -4.0 -36.3 600 46 11 07 01 11 22 00 J1751+0939 13 55 10 26.2 469.1 -4.0 -36.0 295 46 11 22 00 11 32 00 =1749+096 14 05 12 27.6 471.4 -3.8 -35.4 600 85 11 22 01 11 37 00 J1751+0939 14 10 12 28.3 472.5 -3.7 -35.1 295 85 11 37 00 11 47 00 =1749+096 14 20 14 29.7 474.9 -3.5 -34.4 600 124 11 37 01 11 52 00 J1751+0939 14 25 15 30.4 476.0 -3.5 -34.0 295 124 11 52 00 12 02 00 =1749+096 14 35 16 31.8 478.4 -3.3 -33.2 600 162 11 52 01 12 07 00 J1751+0939 14 40 17 32.4 479.7 -3.2 -32.7 295 162 12 07 00 12 17 00 =1749+096 14 50 19 33.8 482.2 -3.0 -31.8 600 201 12 07 01 12 22 00 J1751+0939 14 55 20 34.4 483.4 -3.0 -31.3 295 201 12 22 00 12 32 00 =1749+096 15 05 21 35.7 486.0 -2.8 -30.2 600 240 12 22 01 12 37 00 J1751+0939 15 10 22 36.3 487.4 -2.7 -29.6 295 240 12 37 00 12 47 00 =1749+096 15 20 24 37.5 490.1 -2.5 -28.4 600 278 12 37 01 12 52 00 J2031+1219 15 25 25 17.8 452.6 -5.1 -38.9 215 278 12 52 00 13 02 00 =2029+121 15 35 26 19.3 454.6 -5.0 -38.8 600 317 12 52 01 Next scan frequencies: 4888.49 4888.49 Next BBC frequencies: 735.51 735.51 13 07 00 J2031+1219 15 40 27 20.1 455.6 -4.9 -38.7 295 317 13 07 00 13 17 00 =2029+121 15 50 29 21.6 457.7 -4.7 -38.5 600 356 13 07 01 13 22 00 J2031+1219 15 55 30 22.4 458.7 -4.6 -38.4 295 356 13 22 00 13 32 00 =2029+121 16 05 31 23.9 460.8 -4.5 -38.1 600 394 13 22 01 13 37 00 J2031+1219 16 10 32 24.7 461.9 -4.4 -37.9 295 394 13 37 00 13 47 00 =2029+121 16 20 34 26.2 464.0 -4.2 -37.5 600 433 13 37 01 13 52 00 J2031+1219 16 25 35 26.9 465.1 -4.1 -37.3 295 433 13 52 00 14 00 00 =2029+121 16 33 36 28.1 466.9 -4.0 -36.9 480 464 13 52 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess320.C2048 --- 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: 17 Station: CAMBG32M Total bit rate: 512 Format: VDIF Bits per sample: 2 Sample rate:128.000 Number of channels: 2 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 5664.00 5664.00 Net SB= U U IF SB = L L Pol. = RCP LCP BBC = 1 9 BBC SB= L L IF = A1 B1 The following frequency sets based on these setups were used. Frequency Set: 16 Setup file default. Used with PCAL = off LO sum= 4958.49 4958.49 BBC fr= 705.51 705.51 Bandwd= 64.00 64.00 Matching frequency sets: 16 17 18 19 20 Track assignments are: track1= 1, 2 barrel=roll_off ======== Setup file: sess320.C4096 --- 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: 37 Station: CAMBG32M Total bit rate: 512 Format: VDIF Bits per sample: 2 Sample rate:128.000 Number of channels: 2 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 5624.00 5624.00 Net SB= U U IF SB = L L Pol. = RCP LCP BBC = 1 9 BBC SB= L L IF = A1 B1 The following frequency sets based on these setups were used. Frequency Set: 36 Setup file default. Used with PCAL = off LO sum= 4888.49 4888.49 BBC fr= 735.51 735.51 Bandwd= 64.00 64.00 Matching frequency sets: 36 37 38 39 40 Track assignments are: track1= 1, 2 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 1749+096 17 49 10.387930 * 17 51 32.818574 17 52 30.206006 0.00 * J1751+0939 09 39 42.82586 * 09 39 00.72841 09 38 53.77753 0.00 J1751+09 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 192391 observations. 2029+121 20 29 32.681260 * 20 31 54.994267 20 32 53.138831 0.01 * J2031+1219 12 09 28.75299 * 12 19 41.34015 12 24 03.67620 0.02 J2031+12 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 4314 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 J1751+0939 sess320.C2048 1 2 3 4 5 6 7 8 9 10 11 15 + 1.200 252.000 J2031+1219 sess320.C2048 1 2 3 4 5 6 7 8 9 10 11 15 + 0.167 35.000 sess320.C4096 22 23 24 25 26 27 28 29 31 + 0.633 120.333 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) J1751+0939 58.4 J2031+1219 96.7 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