COVER INFORMATION Station: SVETLOE (Code Sv ) Experiment: Network Monitoring Experiment Exp. Code: N18L2 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: Notes: 18cm (L-band) NME and ftp fringe test for session 2/2018 (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 18cm NME and ftp fringe-test on 29 May 2018 involving 11 antennas. JB2, WB1, EF, MC, ON85, TR, SV, ZC, BD, HH, SR. 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: 0234+285, 3C84 for ftp-fringe tests; Ftp-fringe tests are scheduled every half hour throughout the experiment: 08:25:00 (scan 2, 2 sec, 0234+285) 08:55:00 (scan 4, 2 sec, 0234+285) 09:25:00 (scan 6, 2 sec, 0234+285) 09:55:00 (scan 8, 2 sec, 0234+285) 10:25:00 (scan 10, 2 sec, 0234+285) 10:55:00 (scan 12, 2 sec, 3C84) 11:25:00 (scan 14, 2 sec, 3C84) 11:55:00 (scan 16, 2 sec, 3C84) All the best to everyone involved Katharina Schedule for SVETLOE (Code Sv ) 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 29 May 2018 Day 149 --- Next scan frequencies: 1634.49 1634.49 1634.49 1634.49 1650.49 1650.49 1650.49 1650.49 1666.49 1666.49 1666.49 1666.49 1682.49 1682.49 1682.49 1682.49 Next BBC frequencies: 374.49 374.49 374.49 374.49 390.49 390.49 390.49 390.49 406.49 406.49 406.49 406.49 422.49 422.49 422.49 422.49 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 08 00 00 0234+285 02 26 21 58.3 534.8 -0.2 -2.9 0 0 08 00 00 08 14 00 --- 02 40 23 58.3 540.6 0.0 0.3 840 54 08 00 01 08 15 00 0234+285 02 41 23 58.3 541.0 0.0 0.6 53 54 08 15 00 08 29 00 --- 02 55 25 58.2 546.9 0.3 3.9 840 108 08 15 01 08 30 00 0234+285 02 56 25 58.2 547.3 0.3 4.1 53 108 08 30 00 08 44 00 --- 03 10 28 57.9 553.1 0.5 7.3 840 162 08 30 01 08 45 00 0234+285 03 11 28 57.9 553.5 0.5 7.5 53 162 08 45 00 08 59 00 --- 03 25 30 57.4 559.1 0.8 10.6 840 215 08 45 01 09 00 00 0234+285 03 26 30 57.3 559.5 0.8 10.8 53 215 09 00 00 09 14 00 --- 03 40 33 56.7 565.1 1.0 13.8 840 269 09 00 01 09 15 00 0234+285 03 41 33 56.6 565.5 1.0 14.0 53 269 09 15 00 09 29 00 --- 03 55 35 55.8 570.8 1.3 16.7 840 323 09 15 01 09 30 00 0234+285 03 56 35 55.8 571.2 1.3 16.9 53 323 09 30 00 09 44 00 --- 04 10 38 54.8 576.3 1.5 19.4 840 377 09 30 01 09 45 00 0234+285 04 11 38 54.7 576.6 1.5 19.6 53 377 09 45 00 09 59 00 --- 04 25 40 53.6 581.6 1.8 21.9 840 431 09 45 01 10 00 00 0234+285 04 26 40 53.6 581.9 1.8 22.0 53 431 10 00 00 10 14 00 --- 04 40 43 52.4 586.6 2.0 24.1 840 485 10 00 01 10 15 00 0234+285 04 41 43 52.3 586.9 2.0 24.2 54 485 10 15 00 10 29 00 --- 04 55 45 51.0 591.4 2.3 26.0 840 538 10 15 01 10 31 00 3C84 04 57 45 66.0 588.9 1.6 29.7 75 538 10 31 00 10 44 00 --- 05 10 47 64.7 593.9 1.8 32.1 780 588 10 31 01 10 45 00 3C84 05 11 48 64.6 594.3 1.8 32.3 53 588 10 45 00 10 59 00 --- 05 25 50 63.2 599.3 2.1 34.4 840 642 10 45 01 11 00 00 3C84 05 26 50 63.1 599.6 2.1 34.6 53 642 11 00 00 11 14 00 --- 05 40 52 61.6 604.2 2.3 36.3 840 696 11 00 01 Schedule for SVETLOE (Code Sv ) 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 29 May 2018 Day 149 --- 11 15 00 3C84 05 41 53 61.4 604.5 2.3 36.4 54 696 11 15 00 11 29 00 --- 05 55 55 59.9 608.8 2.6 37.8 840 750 11 15 01 11 30 00 3C84 05 56 55 59.7 609.1 2.6 37.9 54 750 11 30 00 11 44 00 --- 06 10 57 58.1 613.1 2.8 39.0 840 804 11 30 01 11 45 00 3C84 06 11 57 58.0 613.3 2.8 39.0 54 804 11 45 00 12 00 00 --- 06 27 00 56.2 617.3 3.1 39.9 900 862 11 45 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess218.L512 Matching groups in /home/jops/sched_11.4mod/catalogs/freq_RDBE.dat: kvzr_l passed by Alexey Melnikov, Mar2014 Setup group: 1 Station: SVETLOE Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 1260.00 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 = A B A B A B A B A B A B A B A B The following frequency sets based on these setups were used. Frequency Set: 7 Setup file default. Used with PCAL = off LO sum= 1634.49 1634.49 1634.49 1634.49 1650.49 1650.49 1650.49 1650.49 1666.49 1666.49 1666.49 1666.49 1682.49 1682.49 1682.49 1682.49 BBC fr= 374.49 374.49 374.49 374.49 390.49 390.49 390.49 390.49 406.49 406.49 406.49 406.49 422.49 422.49 422.49 422.49 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: 7 8 9 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 38 55.460203 0.00 J0237+2848 28 35 11.40776 * 28 48 08.99001 28 52 37.32995 0.00 J0237+28 /home/jops/sched_11.4mod/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 54650 observations. * 3C84 03 16 29.567263 * 03 19 48.160094 03 20 58.873202 1.30 J0319+4130 41 19 51.91701 * 41 30 42.10413 41 34 23.63278 2.69 0316+413 /home/jops/sched_11.4mod/catalogs/sources.gsfc J0319+41 GSFC 2015a astro solution, unpublished 10208 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 0234+285 sess218.L512 1 2 3 4 5 6 7 10 11 2.333 128.333 3C84 sess218.L512 1 2 3 4 5 6 7 10 11 1.400 74.833 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) 0234+285 25.0 3C84 24.1 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