COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: Network Monitoring Experiment Exp. Code: N23K1 Schedule Version: 1.00 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: 1.3cm NME and ftp fringe test for 2023 session 2 (2048 Mbps, L+R, 2-bit sampling, 32 MHz filters) Please send the disk pack by express to JIVE Please DO NOT use the phase cal signal. COVER LETTER: This is the schedule for the 1.3cm NME and ftp fringe-test on 3 June 2023 involving 19 antennas: Jb2 Ef Mc Nt O6 T6 Ur Tr Mh Ys Hh Kt Ky Ku Cm Da De Kn Pi. (Kt out -> 18 antennas) The NME uses the RCP-only 2 Gbps mode used in EC092 The schedule consists of long integrations on the strong calibrators J1058+0133 and J1159+2914, for ftp-fringe tests; and the sources J1152+2930 and J1221+2813 will be observed for phase-referencing test purposes. Seven ftp-fringe tests are scheduled throughout the experiment: 14:10:00 (scan 1, 4 sec, J1058+0133) 14:40:00 (scan 3, 4 sec, J1058+0133) 15:10:00 (scan 5, 4 sec, J1159+2914) 15:40:00 (scan 7, 4 sec, J1159+2914) 16:10:00 (scan 9, 4 sec, J1159+2914) 16:35:00 (scan 15, 4 sec, J1159+2914) 16:58:00 (scan 21, 4 sec, J1159+2914) Good luck with the session! Benito Marcote Mattermost: coms.evlbi.org Schedule for URUMQI (Code Ur ) 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 ---------------------------------------------------------------------------------------- --- Sat 3 Jun 2023 Day 154 --- Next scan frequencies: 22024.99 22024.99 22088.99 22088.99 22152.99 22152.99 22216.99 22216.99 22280.99 22280.99 22344.99 22344.99 22408.99 22408.99 22472.99 22472.99 Next BBC frequencies: 32.99 32.99 96.99 96.99 160.99 160.99 224.99 224.99 288.99 288.99 352.99 352.99 416.99 416.99 480.99 480.99 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 14 00 00 J1058+0133 12 35 48 42.8 213.7 1.6 23.8 0 0 14 00 00 14 12 00 =1055+018 12 47 50 41.6 217.4 1.8 26.2 720 185 14 00 01 14 15 00 J1058+0133 12 50 50 41.2 218.3 1.9 26.7 178 185 14 15 00 14 27 00 =1055+018 13 02 52 39.8 221.8 2.1 28.9 720 369 14 15 01 14 30 00 J1058+0133 13 05 53 39.5 222.6 2.1 29.5 178 369 14 30 00 14 42 00 =1055+018 13 17 55 37.9 226.0 2.3 31.5 720 554 14 30 01 14 45 00 J1058+0133 13 20 55 37.5 226.8 2.4 31.9 178 554 14 45 00 14 57 00 =1055+018 13 32 57 35.9 229.9 2.6 33.7 720 738 14 45 01 15 02 00 J1159+2914 13 37 58 65.9 241.6 1.6 46.9 236 738 15 02 00 15 12 00 =1156+295 13 47 59 64.2 245.1 1.8 48.9 600 892 15 02 01 15 17 00 J1159+2914 13 53 00 63.4 246.7 1.9 49.7 298 892 15 17 00 15 27 00 =1156+295 14 03 02 61.7 249.7 2.0 51.2 600 1046 15 17 01 15 32 00 J1159+2914 14 08 03 60.9 251.1 2.1 51.8 298 1046 15 32 00 15 42 00 =1156+295 14 18 04 59.1 253.8 2.3 52.9 600 1200 15 32 01 15 47 00 J1159+2914 14 23 05 58.3 255.1 2.4 53.4 298 1200 15 47 00 15 57 00 =1156+295 14 33 07 56.5 257.5 2.5 54.2 600 1354 15 47 01 16 02 00 J1159+2914 14 38 08 55.6 258.6 2.6 54.5 298 1354 16 02 00 16 12 00 =1156+295 14 48 09 53.8 260.8 2.8 55.1 600 1508 16 02 01 16 15 00 J1159+2914 14 51 10 53.3 261.4 2.8 55.2 178 1508 16 15 00 16 16 30 =1156+295 14 52 40 53.0 261.7 2.9 55.3 90 1531 16 15 01 16 16 30 J1221+2813 14 52 40 56.3 255.4 2.5 52.8 -10 1531 No stop 16 18 00 =1219+285 14 54 10 56.0 255.8 2.5 52.9 80 1554 16 16 31 16 18 00 J1159+2914 14 54 10 52.7 262.0 2.9 55.4 -10 1554 No stop 16 19 30 =1156+295 14 55 41 52.5 262.3 2.9 55.4 80 1577 16 18 01 16 19 30 J1152+2930 14 55 41 51.4 264.0 3.0 55.9 -6 1577 No stop 16 21 00 --- 14 57 11 51.2 264.3 3.0 56.0 84 1600 16 19 31 Schedule for URUMQI (Code Ur ) 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 ---------------------------------------------------------------------------------------- --- Sat 3 Jun 2023 Day 154 --- 16 21 00 J1152+2930 14 57 11 51.2 264.3 3.0 56.0 -2 1600 No stop 16 22 30 --- 14 58 41 50.9 264.6 3.1 56.0 88 1623 16 21 01 16 27 00 J1159+2914 15 03 12 51.1 263.9 3.0 55.7 264 1623 16 27 00 16 37 00 =1156+295 15 13 13 49.3 265.8 3.2 55.9 600 1777 16 27 01 16 40 00 J1159+2914 15 16 14 48.7 266.3 3.3 56.0 178 1777 16 40 00 16 41 30 =1156+295 15 17 44 48.5 266.6 3.3 56.0 90 1800 16 40 01 16 41 30 J1221+2813 15 17 44 51.9 261.0 2.9 54.4 -10 1800 No stop 16 43 00 =1219+285 15 19 14 51.6 261.3 2.9 54.4 80 1823 16 41 31 16 43 00 J1159+2914 15 19 14 48.2 266.9 3.3 56.0 -10 1823 No stop 16 44 30 =1156+295 15 20 45 47.9 267.2 3.3 56.1 80 1846 16 43 01 16 44 30 J1152+2930 15 20 45 46.9 268.7 3.4 56.4 -5 1846 No stop 16 46 00 --- 15 22 15 46.6 268.9 3.5 56.4 85 1869 16 44 31 16 46 00 J1152+2930 15 22 15 46.6 268.9 3.5 56.4 -2 1869 No stop 16 47 30 --- 15 23 45 46.3 269.2 3.5 56.4 88 1892 16 46 01 16 51 30 J1159+2914 15 27 46 46.7 268.4 3.5 56.1 235 1892 16 51 30 17 00 00 =1156+295 15 36 17 45.1 269.9 3.6 56.2 510 2023 16 51 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess223.K2048geoOD --- 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: 9 Station: URUMQI Total bit rate: 2048 Format: MARK5B Bits per sample: 2 Sample rate: 64.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 21992.00 Net SB= L U L U L U L U L U L U L U L U IF SB = U U U U U U U U U U U U U U U U Pol. = RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP BBC = 1 1 2 2 3 3 4 4 5 5 6 6 7 7 8 8 BBC SB= L U L U L U L U L U L U L U L U IF = A2 A2 A2 A2 A2 A2 A2 A2 B2 B2 B2 B2 B2 B2 B2 B2 The following frequency sets based on these setups were used. Frequency Set: 7 Setup file default. Used with PCAL = 1MHz LO sum= 22024.99 22024.99 22088.99 22088.99 22152.99 22152.99 22216.99 22216.99 22280.99 22280.99 22344.99 22344.99 22408.99 22408.99 22472.99 22472.99 BBC fr= 32.99 32.99 96.99 96.99 160.99 160.99 224.99 224.99 288.99 288.99 352.99 352.99 416.99 416.99 480.99 480.99 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 7 Track assignments are: track1= 18, 2, 20, 4, 22, 6, 24, 8, 26, 10, 28, 12, 30, 14, 32, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * J1152+2930 11 50 23.621999 * 11 52 58.760000 11 54 11.324627 0.00 29 46 56.33378 * 29 30 15.05200 29 22 37.38029 0.00 From catalog imbedded in main SCHED input file. 1055+018 10 55 55.313730 * 10 58 29.605208 10 59 41.269740 0.01 * J1058+0133 01 50 03.53722 * 01 33 58.82372 01 26 29.68802 0.01 J1058+01 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 8263 observations. 1156+295 11 56 57.786211 * 11 59 31.833912 12 00 43.936740 0.00 * J1159+2914 29 31 25.73880 * 29 14 43.82690 29 07 05.60950 0.00 J1159+29 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 78215 observations. 1219+285 12 19 01.115596 * 12 21 31.690516 12 22 42.323046 0.04 * J1221+2813 28 30 36.52562 * 28 13 58.50017 28 06 21.13888 0.05 J1221+28 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 755 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 J1152+2930 sess223.K2048geoOD 1 2 3 4 5 6 7 8 9 10 11 13 + 0.100 12.802 J1058+0133 sess223.K2048geoOD 1 2 3 4 5 6 7 8 9 10 11 13 + 0.800 122.400 J1159+2914 sess223.K2048geoOD 1 2 3 4 5 6 7 8 9 10 11 13 + 1.242 187.318 J1221+2813 sess223.K2048geoOD 1 2 3 4 5 6 7 8 9 10 11 13 + 0.050 5.053 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) J1152+2930 93.0 J1058+0133 92.7 J1159+2914 94.3 J1221+2813 99.0 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