COVER INFORMATION Station: IRBENE (Code Ir ) Experiment: Network Monitoring Experiment Exp. Code: N19M2 Schedule Version: 1.00 Processed by SCHED version: 11.50 Development version 11.5. Started Apr. 2 PI: Olga Bayandina Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596507 EMAIL: bayandina@jive.eu Fax: Phone during observation: +31-521-596507 Observing mode: Notes: 5cm NME and ftp fringe test for Session 2 2019 (256 Mbps, L+R, 2-bit sampling, 4 MHz filters) Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 5cm NME and ftp fringe-test on 3rd June 2019 involving antennas: Jb2, Wb, Ef, Mc, Nt, On85, T6, Tr, Ys, Hh, Ir, Sr. The NME uses a standard setup with 256 Mbps. The schedule consists of long integrations on calibrators J0927+3902 and J1224+2122 for ftp-fringe tests. The following ftp-fringe tests are scheduled throughout the experiment (UT times): 14:15:00 (scan 2, 2 sec, J0927+3902) 14:45:00 (scan 4, 2 sec, J0927+3902) 15:15:00 (scan 6, 2 sec, J0927+3902) 15:45:00 (scan 8, 2 sec, J1224+2122) 16:15:00 (scan 10, 2 sec, J1224+2122) 16:45:00 (scan 12, 2 sec, J1224+2122) Good luck with the session! Olga Bayandina Mattermost: coms.evlbi.org Schedule for IRBENE (Code Ir ) 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 3 Jun 2019 Day 154 --- Next scan frequencies: 6655.49 6655.49 6655.49 6655.49 6663.49 6663.49 6663.49 6663.49 6671.49 6671.49 6671.49 6671.49 6679.49 6679.49 6679.49 6679.49 Next BBC frequencies: 555.49 555.49 555.49 555.49 563.49 563.49 563.49 563.49 571.49 571.49 571.49 571.49 579.49 579.49 579.49 579.49 Next scan bandwidths: 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 14 00 00 J0927+3902 08 14 23 67.9-220.8 -1.2 -26.8 0 0 14 00 00 14 04 00 =4C39.25 08 18 23 68.2-218.9 -1.2 -25.7 240 8 14 00 01 14 07 00 J0927+3902 08 21 24 68.5-217.5 -1.1 -24.8 177 8 14 07 00 14 17 00 =4C39.25 08 31 25 69.2-212.6 -0.9 -21.8 600 27 14 07 01 14 20 00 J0927+3902 08 34 26 69.4-211.0 -0.9 -20.8 177 27 14 20 00 14 32 00 =4C39.25 08 46 28 70.2-204.6 -0.7 -16.7 720 50 14 20 01 14 35 00 J0927+3902 08 49 28 70.4-202.9 -0.6 -15.6 177 50 14 35 00 14 47 00 =4C39.25 09 01 30 70.9-196.0 -0.4 -11.0 720 73 14 35 01 14 50 00 J0927+3902 09 04 31 71.0-194.3 -0.4 -9.8 177 73 14 50 00 15 02 00 =4C39.25 09 16 33 71.3-187.1 -0.2 -4.9 720 97 14 50 01 15 05 00 J0927+3902 09 19 33 71.4-185.3 -0.1 -3.6 177 97 15 05 00 15 17 00 =4C39.25 09 31 35 71.4-178.0 0.1 1.4 720 120 15 05 01 15 24 00 J1224+2122 09 38 36 42.8-237.8 -2.8 -29.2 386 120 15 24 00 15 32 00 =1222+216 09 46 38 43.6-235.5 -2.7 -28.3 480 135 15 24 01 15 35 00 J1224+2122 09 49 38 44.0-234.7 -2.6 -28.0 177 135 15 35 00 15 47 00 =1222+216 10 01 40 45.3-231.2 -2.4 -26.7 720 158 15 35 01 15 50 00 J1224+2122 10 04 41 45.6-230.3 -2.4 -26.3 177 158 15 50 00 16 02 00 =1222+216 10 16 43 46.8-226.6 -2.2 -24.7 720 182 15 50 01 16 05 00 J1224+2122 10 19 43 47.1-225.7 -2.1 -24.3 177 182 16 05 00 16 17 00 =1222+216 10 31 45 48.2-221.9 -1.9 -22.6 720 205 16 05 01 16 20 00 J1224+2122 10 34 46 48.5-220.9 -1.9 -22.2 177 205 16 20 00 16 32 00 =1222+216 10 46 48 49.5-216.9 -1.7 -20.2 720 228 16 20 01 16 35 00 J1224+2122 10 49 48 49.7-215.9 -1.6 -19.7 177 228 16 35 00 16 47 00 =1222+216 11 01 50 50.6-211.8 -1.4 -17.6 720 251 16 35 01 16 50 00 J1224+2122 11 04 51 50.8-210.7 -1.4 -17.1 177 251 16 50 00 17 00 00 =1222+216 11 14 52 51.5-207.1 -1.2 -15.2 600 271 16 50 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess219.M256 --- 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: 12 Station: IRBENE Total bit rate: 256 Format: VDIF Bits per sample: 2 Sample rate: 8.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 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 = A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 The following frequency sets based on these setups were used. Frequency Set: 11 Setup file default. Used with PCAL = off LO sum= 6655.49 6655.49 6655.49 6655.49 6663.49 6663.49 6663.49 6663.49 6671.49 6671.49 6671.49 6671.49 6679.49 6679.49 6679.49 6679.49 BBC fr= 555.49 555.49 555.49 555.49 563.49 563.49 563.49 563.49 571.49 571.49 571.49 571.49 579.49 579.49 579.49 579.49 Bandwd= 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 Matching frequency sets: 11 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 4C39.25 09 23 55.319216 * 09 27 03.013937 09 28 13.623159 0.31 * J0927+3902 39 15 23.56644 * 39 02 20.85185 38 57 27.56781 0.16 0923+392 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc J0927+39 GSFC 2016a X/S astro solution, 250526 observations. 1222+216 12 22 23.408719 * 12 24 54.458404 12 25 52.483759 0.05 * J1224+2122 21 39 23.03695 * 21 22 46.38856 21 16 31.21740 0.09 J1224+21 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 386 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 J0927+3902 sess219.M256 1 2 3 4 5 6 7 8 9 10 11 13 1.033 80.600 J1224+2122 sess219.M256 1 2 3 4 5 6 7 8 9 10 11 13 1.300 100.622 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) J0927+3902 61.5 J1224+2122 103.2 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