COVER INFORMATION Station: WSTRBORK (Code Wb ) Experiment: Network Monitoring Experiment Exp. Code: N16X1 Schedule Version: 1.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Benito Marcote Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: marcote@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 3.6cm (X-band) NME and ftp fringe test for session 3/2016 (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 3.6cm NME and ftp fringe-test on 7 November 2016 involving 11 antennas: Wb1, Ef, Mc, Nt, O6, T6, Ur, Ys, Sv, Zc, Bd The NME uses a standard setup with 512 Mbps. The schedule consists of: - long integrations on strong calibrator, J1927+7358, for ftp-fringe tests; Ftp-fringe tests are scheduled every half hour throughout the experiment: 12:15:00 (scan 2, 2 sec, J1927+7358) 12:45:00 (scan 5, 2 sec, J1927+7358) 13:15:00 (scan 8, 2 sec, J1927+7358) 13:45:00 (scan 11, 2 sec, J1927+7358) 14:15:00 (scan 14, 2 sec, J1927+7358) 14:45:00 (scan 17, 2 sec, J1927+7358) Please make sure that the autoftp is set up correctly. Thanks! Benito. Skype account: jive.support.scientist 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 ---------------------------------------------------------------------------------------- --- Mon 7 Nov 2016 Day 312 --- Next scan frequencies: 8399.49 8399.49 8399.49 8399.49 8431.49 8431.49 8431.49 8431.49 Next BBC frequencies: 402.49 402.49 402.49 402.49 434.49 434.49 434.49 434.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 12 00 00 J1927+7358 15 34 51 58.7 26.8 -3.9 0.0 0 0 12 00 00 12 09 00 =1928+738 15 43 53 59.3 26.6 -3.7 0.0 540 35 12 00 01 12 10 00 J1927+7358 15 44 53 59.4 26.5 -3.7 0.0 49 35 12 10 00 12 19 00 =1928+738 15 53 55 60.0 26.2 -3.6 0.0 540 69 12 10 01 12 20 00 J1927+7358 15 54 55 60.1 26.2 -3.5 0.0 49 69 12 20 00 12 29 00 =1928+738 16 03 56 60.7 25.9 -3.4 0.0 540 104 12 20 01 12 30 00 J1927+7358 16 04 56 60.7 25.8 -3.4 0.0 49 104 12 30 00 12 39 00 =1928+738 16 13 58 61.3 25.4 -3.2 0.0 540 138 12 30 01 12 40 00 J1927+7358 16 14 58 61.4 25.3 -3.2 0.0 49 138 12 40 00 12 49 00 =1928+738 16 23 59 62.0 24.9 -3.1 0.0 540 173 12 40 01 12 50 00 J1927+7358 16 25 00 62.0 24.8 -3.0 0.0 49 173 12 50 00 12 59 00 =1928+738 16 34 01 62.6 24.2 -2.9 0.0 540 208 12 50 01 13 00 00 J1927+7358 16 35 01 62.6 24.2 -2.9 0.0 49 208 13 00 00 13 09 00 =1928+738 16 44 03 63.2 23.5 -2.7 0.0 540 242 13 00 01 13 10 00 J1927+7358 16 45 03 63.3 23.5 -2.7 0.0 49 242 13 10 00 13 19 00 =1928+738 16 54 04 63.8 22.8 -2.6 0.0 540 277 13 10 01 13 20 00 J1927+7358 16 55 05 63.8 22.7 -2.5 0.0 49 277 13 20 00 13 29 00 =1928+738 17 04 06 64.4 21.9 -2.4 0.0 540 312 13 20 01 13 30 00 J1927+7358 17 05 06 64.4 21.8 -2.4 0.0 49 312 13 30 00 13 39 00 =1928+738 17 14 08 64.9 20.9 -2.2 0.0 540 346 13 30 01 13 40 00 J1927+7358 17 15 08 65.0 20.8 -2.2 0.0 49 346 13 40 00 13 49 00 =1928+738 17 24 09 65.4 19.9 -2.1 0.0 540 381 13 40 01 13 50 00 J1927+7358 17 25 09 65.5 19.7 -2.0 0.0 49 381 13 50 00 13 59 00 =1928+738 17 34 11 65.9 18.7 -1.9 0.0 540 415 13 50 01 14 00 00 J1927+7358 17 35 11 66.0 18.6 -1.9 0.0 49 415 14 00 00 14 09 00 =1928+738 17 44 13 66.4 17.4 -1.7 0.0 540 450 14 00 01 14 10 00 J1927+7358 17 45 13 66.5 17.3 -1.7 0.0 49 450 14 10 00 14 19 00 =1928+738 17 54 14 66.8 16.1 -1.6 0.0 540 485 14 10 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 ---------------------------------------------------------------------------------------- --- Mon 7 Nov 2016 Day 312 --- 14 20 00 J1927+7358 17 55 14 66.9 15.9 -1.5 0.0 49 485 14 20 00 14 29 00 =1928+738 18 04 16 67.2 14.6 -1.4 0.0 540 519 14 20 01 14 30 00 J1927+7358 18 05 16 67.3 14.5 -1.4 0.0 49 519 14 30 00 14 39 00 =1928+738 18 14 17 67.6 13.1 -1.2 0.0 540 554 14 30 01 14 40 00 J1927+7358 18 15 18 67.6 13.0 -1.2 0.0 49 554 14 40 00 14 49 00 =1928+738 18 24 19 67.9 11.5 -1.1 0.0 540 588 14 40 01 14 50 00 J1927+7358 18 25 19 68.0 11.3 -1.0 0.0 49 588 14 50 00 14 59 00 =1928+738 18 34 21 68.2 9.8 -0.9 0.0 540 623 14 50 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess316.X512nme --- 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: 13 Station: WSTRBORK 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= 7997.00 7997.00 7997.00 7997.00 7997.00 7997.00 7997.00 7997.00 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 5 1 5 3 7 3 7 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= 8399.49 8399.49 8399.49 8399.49 8431.49 8431.49 8431.49 8431.49 BBC fr= 402.49 402.49 402.49 402.49 434.49 434.49 434.49 434.49 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 1 Track assignments are: track1= 10, 14, 2, 6, 12, 16, 4, 8 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 1928+738 19 28 49.350209 * 19 27 48.495162 19 27 26.302589 0.04 * J1927+7358 73 51 44.92746 * 73 58 01.56990 74 00 33.14394 0.01 J1927+73 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 4075 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 J1927+7358 sess316.X512nme 1 2 3 4 5 6 7 8 9 12 13 2.700 210.600 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) J1927+7358 100.2 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