COVER INFORMATION Station: HART (Code Hh ) Experiment: Network Monitoring Experiment Exp. Code: N23X2 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Gabor Orosz Address: JIVE Oude Hoogeveensedijk 4 Dwingeloo Netherlands Phone: +31 521 596 530 EMAIL: orosz@jive.eu Fax: Phone during observation: +31 521 596 530 Observing mode: vlbi Notes: X-band (3.6cm) NME and ftp fringe test for Session 2, 2023. 2Gbps/8IF/32MHz/dual/2bit (W1:1Gbps/4IF/32MHz) evn4cm-2Gbps-32MHz.set COVER LETTER: This is the schedule for the 3.6cm NME FTP-FT on June 13, 2023 involving the following 11 antennas: Wb1, Ef, Mc, Nt, On60, Sh, Ur, Tr, Ys, Hh, Ib, Yd. The NME uses a standard 2 Gbps setup (16BBC/32MHz/dual), exc. Wb1 (1 Gbps). The NME lasts for 3 hours (13/06, 12-15UT) with long scans on calibrators: J0927+3902 (4C39.25) and J1159+2914 https://obs.vlba.nrao.edu/cst/calibsource/7138 https://obs.vlba.nrao.edu/cst/calibsource/9104 with ftp grabs every other scan at the following times (in UT): 12:10:00 (scan 2, 2 sec, J0927+3902) 12:40:00 (scan 4, 2 sec, J0927+3902) 13:10:00 (scan 6, 2 sec, J0927+3902) 13:40:00 (scan 8, 2 sec, J0927+3902) 14:10:00 (scan 10, 2 sec, J1159+2914) 14:40:00 (scan 12, 2 sec, J1159+2914) 14:58:00 (scan 14, 2 sec, J1159+2914) -- Gabor Orosz Mattermost: coms.evlbi.org Schedule for HART (Code Hh ) 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 13 Jun 2023 Day 164 --- Next scan frequencies: 8319.49 8319.49 8319.49 8319.49 8383.49 8383.49 8383.49 8383.49 8447.49 8447.49 8447.49 8447.49 8511.49 8511.49 8511.49 8511.49 Next BBC frequencies: 239.49 239.49 239.49 239.49 303.49 303.49 303.49 303.49 367.49 367.49 367.49 367.49 431.49 431.49 431.49 431.49 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 12 00 00 J0927+3902 07 16 55 18.2 26.4 -2.2 0.0 0 0 12 00 00 12 02 00 =4C39.25 07 18 56 18.4 26.1 -2.2 0.0 120 31 12 00 01 12 07 00 J0927+3902 07 23 56 18.9 25.2 -2.1 0.0 279 31 12 07 00 12 12 00 =4C39.25 07 28 57 19.4 24.3 -2.0 0.0 300 108 12 07 01 12 17 00 J0927+3902 07 33 58 19.9 23.3 -1.9 0.0 279 108 12 17 00 12 27 00 =4C39.25 07 44 00 20.7 21.5 -1.7 0.0 600 263 12 17 01 12 32 00 J0927+3902 07 49 00 21.1 20.5 -1.7 0.0 279 263 12 32 00 12 42 00 =4C39.25 07 59 02 21.9 18.6 -1.5 0.0 600 417 12 32 01 12 47 00 J0927+3902 08 04 03 22.2 17.6 -1.4 0.0 279 417 12 47 00 12 57 00 =4C39.25 08 14 05 22.9 15.6 -1.2 0.0 600 572 12 47 01 13 02 00 J0927+3902 08 19 05 23.2 14.6 -1.2 0.0 279 572 13 02 00 13 12 00 =4C39.25 08 29 07 23.7 12.6 -1.0 0.0 600 727 13 02 01 13 17 00 J0927+3902 08 34 08 23.9 11.5 -0.9 0.0 279 727 13 17 00 13 27 00 =4C39.25 08 44 10 24.3 9.4 -0.7 0.0 600 881 13 17 01 13 32 00 J0927+3902 08 49 10 24.5 8.4 -0.7 0.0 279 881 13 32 00 13 42 00 =4C39.25 08 59 12 24.8 6.3 -0.5 0.0 600 1036 13 32 01 13 47 00 J1159+2914 09 04 13 20.6 40.5 -2.9 0.0 198 1036 13 47 00 13 57 00 =1156+295 09 14 14 22.0 38.8 -2.8 0.0 600 1190 13 47 01 14 02 00 J1159+2914 09 19 15 22.7 37.8 -2.7 0.0 279 1190 14 02 00 14 12 00 =1156+295 09 29 17 24.1 36.0 -2.5 0.0 600 1345 14 02 01 14 17 00 J1159+2914 09 34 18 24.7 35.0 -2.4 0.0 279 1345 14 17 00 14 27 00 =1156+295 09 44 19 26.0 33.0 -2.3 0.0 600 1499 14 17 01 14 32 00 J1159+2914 09 49 20 26.6 32.0 -2.2 0.0 279 1499 14 32 00 14 42 00 =1156+295 09 59 22 27.8 29.9 -2.0 0.0 600 1654 14 32 01 14 47 00 J1159+2914 10 04 23 28.3 28.8 -1.9 0.0 279 1654 14 47 00 14 52 00 =1156+295 10 09 23 28.9 27.8 -1.9 0.0 300 1731 14 47 01 Schedule for HART (Code Hh ) 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 13 Jun 2023 Day 164 --- 14 57 00 J1159+2914 10 14 24 29.4 26.7 -1.8 0.0 279 1731 14 57 00 15 00 00 =1156+295 10 17 25 29.7 26.0 -1.7 0.0 180 1778 14 57 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess223.X2048 Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat: hhsx Values confirmed by E-mail Jonathan Quick 20140219 (CR) ****** Only 256.00 of 512.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. Setup group: 3 Station: HART Total bit rate: 2048 Format: VDIF 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= 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 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: 10 Setup file default. Used with PCAL = off LO sum= 8319.49 8319.49 8319.49 8319.49 8383.49 8383.49 8383.49 8383.49 8447.49 8447.49 8447.49 8447.49 8511.49 8511.49 8511.49 8511.49 BBC fr= 239.49 239.49 239.49 239.49 303.49 303.49 303.49 303.49 367.49 367.49 367.49 367.49 431.49 431.49 431.49 431.49 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: 10 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 29.492588 0.31 * J0927+3902 39 15 23.56644 * 39 02 20.85185 38 56 28.30004 0.16 0923+392 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J0927+39 GSFC 2016a X/S astro solution, 250526 observations. 1156+295 11 56 57.786211 * 11 59 31.833912 12 00 43.833994 0.00 * J1159+2914 29 31 25.73880 * 29 14 43.82690 29 07 06.31793 0.00 J1159+29 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 78215 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 sess223.X2048 1 2 3 4 5 6 7 8 9 10 12 1.117 73.700 J1159+2914 sess223.X2048 1 2 3 4 5 6 7 8 9 10 12 0.800 52.674 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 53.2 J1159+2914 85.9 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