COVER INFORMATION Station: TORUN (Code Tr ) Experiment: Network Monitoring Experiment Exp. Code: N23L2 Schedule Version: 2.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Junghwan Oh Address: JIVE Oude Hoogeveensedijk 4 Dwingeloo Netherlands Phone: +31 627454602 EMAIL: oh@jive.eu Fax: Phone during observation: +31 521 596 530 Observing mode: vlbi Notes: L-band (18cm) NME and ftp fringe test for Session 2, 2023. EVN: 1024 Mbps, L+R, 2-bit sampling, 8 BBC, 32 MHz filters MER: 512 Mbps, L+R, 2-bit sampling, 2 BBC, 64 MHz filters COVER LETTER: This is the schedule for the 18cm NME and ftp fringe test on June 8, 2023 involving 10 EVN antennas + eMERLIN: Jb2, Wb, Ef, Mc, Nt, O8, T6, Ur, Tr, Hh, Cm, Da, Kn, Pi, De. The NME uses a standard setup with a datarate of 1024 Mbps (512 Mbps for eMERLIN). The NME lasts for 3 hours and consists of long scans on calibrator J0956+2515 with ftp grabs every other scan at the following times (in UT): 12:10:00 (scan 2, 2 sec, J0956+2515) 12:40:00 (scan 4, 2 sec, J0956+2515) 13:10:00 (scan 6, 2 sec, J0956+2515) 13:40:00 (scan 8, 2 sec, J0956+2515) 14:10:00 (scan 10, 2 sec, J0956+2515) 14:40:00 (scan 12, 2 sec, J0956+2515) 14:57:00 (scan 14, 2 sec, J0956+2515) -- Junghwan Oh Mattermost: coms.evlbi.org Schedule for TORUN (Code Tr ) 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 ---------------------------------------------------------------------------------------- --- Thu 8 Jun 2023 Day 159 --- Next scan frequencies: 1626.49 1626.49 1626.49 1626.49 1690.49 1690.49 1690.49 1690.49 Next BBC frequencies: 673.51 673.51 673.51 673.51 609.51 609.51 609.51 609.51 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 12 00 00 J0956+2515 06 20 43 41.0 102.8 -3.6 -40.3 0 0 12 00 00 12 05 00 =0953+254 06 25 44 41.8 103.9 -3.5 -40.1 300 39 12 00 01 12 10 00 J0956+2515 06 30 45 42.5 105.1 -3.5 -39.8 293 39 12 10 00 12 15 00 =0953+254 06 35 46 43.2 106.3 -3.4 -39.5 300 77 12 10 01 12 20 00 J0956+2515 06 40 47 43.9 107.5 -3.3 -39.2 293 77 12 20 00 12 30 00 =0953+254 06 50 48 45.4 110.0 -3.1 -38.6 600 155 12 20 01 12 35 00 J0956+2515 06 55 49 46.1 111.3 -3.0 -38.2 293 155 12 35 00 12 45 00 =0953+254 07 05 51 47.5 113.9 -2.9 -37.3 600 232 12 35 01 12 50 00 J0956+2515 07 10 52 48.1 115.2 -2.8 -36.9 293 232 12 50 00 13 00 00 =0953+254 07 20 53 49.5 118.0 -2.6 -35.9 600 309 12 50 01 13 05 00 J0956+2515 07 25 54 50.2 119.4 -2.5 -35.3 293 309 13 05 00 13 15 00 =0953+254 07 35 56 51.4 122.4 -2.4 -34.1 600 386 13 05 01 13 20 00 J0956+2515 07 40 56 52.1 123.9 -2.3 -33.4 293 386 13 20 00 13 30 00 =0953+254 07 50 58 53.3 127.1 -2.1 -32.0 600 464 13 20 01 13 40 00 J0956+2515 08 01 00 54.5 130.3 -2.0 -30.4 592 464 13 40 00 13 50 00 =0953+254 08 11 01 55.6 133.8 -1.8 -28.6 600 541 13 40 01 13 55 00 J0956+2515 08 16 02 56.1 135.6 -1.7 -27.7 293 541 13 55 00 14 05 00 =0953+254 08 26 04 57.1 139.3 -1.5 -25.6 600 618 13 55 01 14 10 00 J0956+2515 08 31 05 57.6 141.2 -1.5 -24.6 293 618 14 10 00 14 20 00 =0953+254 08 41 06 58.5 145.1 -1.3 -22.3 600 696 14 10 01 14 25 00 J0956+2515 08 46 07 59.0 147.1 -1.2 -21.1 292 696 14 25 00 14 35 00 =0953+254 08 56 09 59.7 151.3 -1.0 -18.6 600 773 14 25 01 14 40 00 J0956+2515 09 01 10 60.1 153.5 -0.9 -17.2 292 773 14 40 00 14 50 00 =0953+254 09 11 11 60.7 157.9 -0.8 -14.5 600 850 14 40 01 14 55 00 J0956+2515 09 16 12 61.0 160.2 -0.7 -13.0 292 850 14 55 00 15 00 00 =0953+254 09 21 13 61.2 162.5 -0.6 -11.5 300 889 14 55 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess223.L1024 --- 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: 8 Station: TORUN Total bit rate: 1024 Format: VDIF Bits per sample: 2 Sample rate: 64.000 Number of channels: 8 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 Net SB= L L U U L L U U IF SB = L L L L L L L L Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 9 1 9 2 10 2 10 BBC SB= U U L L U U L L IF = A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 9 Setup file default. Used with PCAL = off LO sum= 1626.49 1626.49 1626.49 1626.49 1690.49 1690.49 1690.49 1690.49 BBC fr= 673.51 673.51 673.51 673.51 609.51 609.51 609.51 609.51 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 9 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 0953+254 09 53 59.738485 * 09 56 49.875379 09 58 08.548727 0.11 * J0956+2515 25 29 33.58574 * 25 15 16.04984 25 08 45.20186 0.10 From catalog imbedded in main SCHED input file. rfc_2022a Petrov and Kovalev, in preparation 33748 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 J0956+2515 sess223.L1024 1 2 3 4 5 6 7 8 9 10 11 1.917 201.250 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) J0956+2515 65.9 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