COVER INFORMATION Station: HART (Code Hh ) Experiment: Network Monitoring Experiment Exp. Code: N22L1 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Gabor Orosz Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31 686337748 EMAIL: orosz@jive.eu Fax: Phone during observation: +31 521 596 508 Observing mode: Notes: L-band (18/21cm) NME and ftp fringe test for Session 1, 2022. 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 Including 21cm mode in last half hour for FAST COVER LETTER: This is the schedule for the 18cm NME and ftp fringe-test on February 24, 2022 involving 14 EVN antennas + eMERLIN + FAST: Jb1, Wb, Ef, Mc, Nt, O8, T6, Ur, Tr, Hh, Sv, Zc, Bd, Ir, Cm, Da, Kn, Pi, De, Fa. The NME uses a standard setup with 1024 Mbps (512 Mbps for eMERLIN). The schedule has two segments: 12:00-14:15 long scans on J0237+2848 with ftp grabs every other scan (18cm setup); 14:20-15:00 a long scan on J0730+4049 with an ftp grab then alternating short scans on J0730+4049 and J0727+4052 with an ftp grab in scans 17 and 23 (21cm setup). The following ftp-fringe tests are scheduled throughout the experiment (UT times): 12:10:00 (scan 2, 2 sec, J0237+2848, 18cm setup) 12:40:00 (scan 4, 2 sec, J0237+2848, 18cm setup) 13:10:00 (scan 6, 2 sec, J0237+2848, 18cm setup) 13:40:00 (scan 8, 2 sec, J0237+2848, 18cm setup) 14:10:00 (scan 10, 2 sec, J0237+2848, 18cm setup) 14:25:00 (scan 12, 2 sec, J0730+4049, 21cm setup) 14:41:00 (scan 17, 2 sec, J0730+4049, 21cm setup) 14:56:00 (scan 23, 2 sec, J0730+4049, 21cm setup) Thank you for taking part in this NME. With kind regards, 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 ---------------------------------------------------------------------------------------- --- Thu 24 Feb 2022 Day 55 --- Next scan frequencies: 1626.49 1626.49 1626.49 1626.49 1690.49 1690.49 1690.49 1690.49 Next BBC frequencies: 116.49 116.49 116.49 116.49 180.49 180.49 180.49 180.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 12 00 00 J0237+2848 00 08 08 24.3 36.0 -2.5 0.0 0 0 12 00 00 12 05 00 =0234+285 00 13 09 25.0 35.1 -2.4 0.0 300 39 12 00 01 12 10 00 J0237+2848 00 18 10 25.6 34.1 -2.3 0.0 279 39 12 10 00 12 20 00 =0234+285 00 28 11 26.8 32.1 -2.2 0.0 600 116 12 10 01 12 25 00 J0237+2848 00 33 12 27.4 31.0 -2.1 0.0 279 116 12 25 00 12 35 00 =0234+285 00 43 14 28.6 28.9 -1.9 0.0 600 193 12 25 01 12 40 00 J0237+2848 00 48 15 29.1 27.8 -1.8 0.0 279 193 12 40 00 12 50 00 =0234+285 00 58 16 30.1 25.5 -1.7 0.0 600 271 12 40 01 12 55 00 J0237+2848 01 03 17 30.6 24.4 -1.6 0.0 279 271 12 55 00 13 05 00 =0234+285 01 13 19 31.5 22.1 -1.4 0.0 600 348 12 55 01 13 10 00 J0237+2848 01 18 19 31.9 20.9 -1.3 0.0 279 348 13 10 00 13 20 00 =0234+285 01 28 21 32.6 18.4 -1.2 0.0 600 425 13 10 01 13 25 00 J0237+2848 01 33 22 33.0 17.2 -1.1 0.0 279 425 13 25 00 13 35 00 =0234+285 01 43 24 33.6 14.7 -0.9 0.0 600 502 13 25 01 13 40 00 J0237+2848 01 48 24 33.9 13.4 -0.8 0.0 279 502 13 40 00 13 50 00 =0234+285 01 58 26 34.3 10.8 -0.7 0.0 600 580 13 40 01 13 55 00 J0237+2848 02 03 27 34.5 9.5 -0.6 0.0 279 580 13 55 00 14 05 00 =0234+285 02 13 29 34.9 6.9 -0.4 0.0 600 657 13 55 01 14 10 00 J0237+2848 02 18 29 35.0 5.5 -0.3 0.0 279 657 14 10 00 14 15 00 =0234+285 02 23 30 35.1 4.2 -0.3 0.0 300 696 14 10 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess122.L1024 Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat: hh18cm Values confirmed by E-mail Jonathan Quick 20140219 (CR) ****** Only 122.49 of 256.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. Setup group: 9 Station: HART 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= 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 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 9 1 9 2 10 2 10 BBC SB= L L U U L L U U IF = 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= 1626.49 1626.49 1626.49 1626.49 1690.49 1690.49 1690.49 1690.49 BBC fr= 116.49 116.49 116.49 116.49 180.49 180.49 180.49 180.49 Bandwd= 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 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 0234+285 02 34 55.589593 * 02 37 52.405680 02 39 09.238752 0.11 * J0237+2848 28 35 11.40778 * 28 48 08.99003 28 53 52.27119 0.10 From catalog imbedded in main SCHED input file. rfc_2021d Petrov and Kovalev, in preparation 21528 observations 0727+409 07 27 24.091632 * 07 30 51.346591 07 32 23.320556 0.15 * J0730+4049 40 56 10.73890 * 40 49 50.82638 40 47 07.55893 0.12 From catalog imbedded in main SCHED input file. rfc_2021d Petrov and Kovalev, in preparation 894 observations 0724+409 07 24 05.305952 * 07 27 32.941920 07 29 05.068700 0.97 * J0727+4052 40 58 16.62792 * 40 52 10.14373 40 49 32.89930 0.90 From catalog imbedded in main SCHED input file. rfc_2021d Petrov and Kovalev, in preparation 35 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 J0237+2848 sess122.L1024 1 2 3 4 5 6 7 8 9 10 11 14 + 1.500 285.000 J0730+4049 sess122.H1024 21 22 23 24 25 26 27 28 29 + 0.250 43.383 J0727+4052 sess122.H1024 21 22 23 24 25 26 27 28 29 + 0.200 36.100 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) J0237+2848 71.0 J0730+4049 129.6 J0727+4052 129.1 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