COVER INFORMATION Station: TORUN (Code Tr ) Experiment: Network Monitoring Experiment Exp. Code: N17L3 Schedule Version: 1.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Katharina Immer Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: immer@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: 512-8-2 Notes: 512 Mbps, 8x8 MHz, RCP & LCP, 2 bit sampling L Band/1.6 GHz COVER LETTER: This is the schedule for the 18cm NME and ftp fringe-test on 30 Oct 2017 involving 18 antennas. JB1, WB1, EF, MC, ON85, T6, UR, TR, Sv, Zc, Bd, Hh, Ir,[Ar], JODRELL2,CAMBG32M,DARNHALL,KNOCKIN,TABLEY. The NME uses 16x BBC (8 for each Pol.) of 8MHz bandwidth: Data rate of 512 Mbps. The schedule consists of: - long integrations on strong calibrators: J1751+0939, J2115+2933 for ftp-fringe tests; Ftp-fringe tests are scheduled every half hour throughout the experiment: 12:24:00 (scan 2, 2 sec, J1751+0939) 12:54:00 (scan 4, 2 sec, J2115+2933) 13:24:00 (scan 6, 2 sec, J2115+2933) 13:54:00 (scan 8, 2 sec, J2115+2933) 14:24:00 (scan 10, 2 sec, J2115+2933) 14:54:00 (scan 12, 2 sec, J2115+2933) All the best to everyone involved Katharina Skype account: jive.support.scientist Schedule for TORUN (Code Tr ) 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 ---------------------------------------------------------------------------------------- --- Mon 30 Oct 2017 Day 303 --- Next scan frequencies: 1642.49 1642.49 1642.49 1642.49 1674.49 1674.49 1674.49 1674.49 Next BBC frequencies: 657.51 657.51 657.51 657.51 625.51 625.51 625.51 625.51 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 12 00 00 J1751+0939 15 50 14 40.1 139.1 -2.0 -23.5 0 0 12 00 00 12 13 00 =1749+096 16 03 17 41.3 143.0 -1.8 -21.5 780 50 12 00 01 12 15 00 J1751+0939 16 05 17 41.5 143.6 -1.8 -21.2 113 50 12 15 00 12 28 00 =1749+096 16 18 19 42.6 147.7 -1.6 -19.0 780 100 12 15 01 12 34 00 J1848+3219 16 24 20 56.9 114.2 -2.4 -40.4 275 100 12 34 00 12 43 00 =1846+322 16 33 22 58.1 116.9 -2.3 -39.3 540 135 12 34 01 12 45 00 J1848+3219 16 35 22 58.4 117.5 -2.2 -39.1 113 135 12 45 00 12 58 00 =1846+322 16 48 24 60.1 121.8 -2.0 -37.2 780 185 12 45 01 13 00 00 J1848+3219 16 50 24 60.3 122.5 -2.0 -36.9 113 185 13 00 00 13 13 00 =1846+322 17 03 26 61.9 127.1 -1.8 -34.5 780 235 13 00 01 13 15 00 J1848+3219 17 05 27 62.2 127.8 -1.7 -34.2 113 235 13 15 00 13 28 00 =1846+322 17 18 29 63.6 132.9 -1.5 -31.4 780 285 13 15 01 13 30 00 J1848+3219 17 20 29 63.9 133.7 -1.5 -30.9 113 285 13 30 00 13 43 00 =1846+322 17 33 31 65.2 139.3 -1.3 -27.6 780 335 13 30 01 13 45 00 J1848+3219 17 35 32 65.4 140.2 -1.2 -27.0 113 335 13 45 00 13 58 00 =1846+322 17 48 34 66.6 146.4 -1.0 -23.2 780 385 13 45 01 14 00 00 J1848+3219 17 50 34 66.7 147.3 -1.0 -22.6 113 385 14 00 00 14 13 00 =1846+322 18 03 36 67.7 154.0 -0.8 -18.1 780 435 14 00 01 14 15 00 J1848+3219 18 05 37 67.8 155.1 -0.7 -17.4 112 435 14 15 00 14 28 00 =1846+322 18 18 39 68.5 162.2 -0.5 -12.5 780 485 14 15 01 14 30 00 J1848+3219 18 20 39 68.6 163.4 -0.5 -11.7 112 485 14 30 00 14 43 00 =1846+322 18 33 41 69.1 170.9 -0.3 -6.4 780 535 14 30 01 14 45 00 J1848+3219 18 35 42 69.1 172.1 -0.2 -5.6 112 535 14 45 00 15 00 00 =1846+322 18 50 44 69.2 181.0 0.0 0.7 900 592 14 45 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess317.L512nme --- 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: TORUN Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 8 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 Net SB= L L U U L L U U IF SB = L L L L L L L L Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 5 1 5 3 7 3 7 BBC SB= U U L L U U L L IF = A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 8 Setup file default. Used with PCAL = off LO sum= 1642.49 1642.49 1642.49 1642.49 1674.49 1674.49 1674.49 1674.49 BBC fr= 657.51 657.51 657.51 657.51 625.51 625.51 625.51 625.51 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 8 Track assignments are: track1= 2, 6, 10, 14, 4, 8, 12, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 1749+096 17 49 10.387931 * 17 51 32.818574 17 52 21.982296 0.00 * J1751+0939 09 39 42.82591 * 09 39 00.72847 09 39 04.07211 0.00 J1751+09 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 144578 observations. 1846+322 18 46 29.612032 * 18 48 22.088575 18 49 00.939412 0.00 * J1848+3219 32 15 36.66046 * 32 19 02.60386 32 20 38.33774 0.00 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 29306 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 sess317.L512nme 1 2 3 4 5 6 7 8 9 12 13 15 0.433 66.300 J1848+3219 sess317.L512nme 1 2 3 4 5 6 7 8 9 12 13 15 2.133 322.150 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 57.7 J1848+3219 79.2 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