COVER INFORMATION Station: WSTRBORK (Code Wb ) Experiment: Network Monitoring Experiment Exp. Code: N23C1 Schedule Version: 3.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Benito Marcote Address: JIVE Oude Hoogeveensedijk 4 Dwingeloo Netherlands Phone: +31 521 596 508 EMAIL: marcote@jive.eu Fax: Phone during observation: +31 521 596 508 Observing mode: vlbi Notes: C-band (6cm) NME and ftp fringe test for Session 1, 2023. EVN: 4 Gbps, 16 IFs, 32-MHz filters, L+R, 2-bit sampling MER: 512 Mbps (1 x 64-MHz), UR: 2 Gbps (8 x 32-MHz), Wb: 1 Gbps (4 x 32-MHz) with ON8_DBBC/Od and YS_DBBC/Yd DBBC3-testing stations in parallel COVER LETTER: This is the schedule for the 6cm NME and ftp fringe test on 23 February 2023 involving 12 EVN antennas + eMERLIN out-stations: Jb1, Wb, Ef, Mc, Nt, O8, T6, Ur, Tr, Ys, Hh, Ib, Cm, Da, Kn, Pi, De. (plus Od and Yd for DBBC3 testing) The NME uses a standard setup of 4 Gbps, with eMERLIN (0.5 Gbps), Ur (2 Gbps), Wb (1 Gbps). The NME lasts for 3 hours and consists of long scans on calibrators J0237+2848, J0319+4130, and J0530+1331. The following ftp-fringe tests are scheduled throughout the experiment (UTC times): 12:10:00 (scan 2, 2 sec, J0237+2848) 12:40:00 (scan 4, 2 sec, J0237+2848) 13:10:00 (scan 6, 2 sec, J0237+2848) 13:40:00 (scan 8, 2 sec, J0319+4130) 14:10:00 (scan 10, 2 sec, J0319+4130) 14:40:00 (scan 12, 2 sec, J0530+1331) Benito Marcote Mattermost: coms.evlbi.org Schedule for WSTRBORK (Code Wb ) 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 23 Feb 2023 Day 54 --- Next scan frequencies: 4888.00 4888.00 4888.00 4888.00 4952.00 4952.00 4952.00 4952.00 Next BBC frequencies: 371.00 371.00 371.00 371.00 435.00 435.00 435.00 435.00 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 12 00 00 J0237+2848 22 38 52 40.5 94.3 -4.0 0.0 0 0 12 00 00 12 02 00 =0234+285 22 40 53 40.8 94.7 -4.0 0.0 120 15 12 00 01 12 05 00 J0237+2848 22 43 53 41.2 95.3 -3.9 0.0 169 15 12 05 00 12 12 00 =0234+285 22 50 54 42.3 96.8 -3.8 0.0 420 70 12 05 01 12 17 00 J0237+2848 22 55 55 43.0 97.9 -3.7 0.0 289 70 12 17 00 12 27 00 =0234+285 23 05 57 44.5 100.2 -3.6 0.0 600 147 12 17 01 12 32 00 J0237+2848 23 10 57 45.2 101.3 -3.5 0.0 289 147 12 32 00 12 42 00 =0234+285 23 20 59 46.7 103.6 -3.3 0.0 600 224 12 32 01 12 47 00 J0237+2848 23 26 00 47.5 104.8 -3.2 0.0 289 224 12 47 00 12 57 00 =0234+285 23 36 02 48.9 107.3 -3.1 0.0 600 301 12 47 01 13 02 00 J0237+2848 23 41 02 49.6 108.6 -3.0 0.0 289 301 13 02 00 13 12 00 =0234+285 23 51 04 51.0 111.2 -2.8 0.0 600 379 13 02 01 13 17 00 J0319+4130 23 56 05 54.2 87.3 -3.4 0.0 245 379 13 17 00 13 27 00 =3C84 00 06 06 55.8 89.2 -3.3 0.0 600 456 13 17 01 13 32 00 J0319+4130 00 11 07 56.5 90.2 -3.2 0.0 289 456 13 32 00 13 42 00 =3C84 00 21 09 58.0 92.3 -3.0 0.0 600 533 13 32 01 13 47 00 J0319+4130 00 26 10 58.8 93.4 -2.9 0.0 289 533 13 47 00 13 57 00 =3C84 00 36 11 60.3 95.6 -2.8 0.0 600 611 13 47 01 14 02 00 J0319+4130 00 41 12 61.0 96.7 -2.7 0.0 289 611 14 02 00 14 12 00 =3C84 00 51 14 62.5 99.1 -2.5 0.0 600 688 14 02 01 14 17 00 J0319+4130 00 56 15 63.3 100.3 -2.4 0.0 289 688 14 17 00 14 27 00 =3C84 01 06 16 64.8 103.0 -2.3 0.0 600 765 14 17 01 14 32 00 J0530+1331 01 11 17 25.6 101.7 -4.3 0.0 179 765 14 32 00 14 42 00 =0528+134 01 21 19 27.1 103.9 -4.2 0.0 600 842 14 32 01 14 45 00 J0530+1331 01 24 19 27.5 104.6 -4.1 0.0 169 842 14 45 00 14 55 00 =0528+134 01 34 21 29.0 106.8 -4.0 0.0 600 920 14 45 01 14 57 00 J0530+1331 01 36 21 29.3 107.2 -3.9 0.0 109 920 14 57 00 15 00 00 =0528+134 01 39 22 29.7 107.9 -3.9 0.0 180 943 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: sess123.C4096 --- 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: 14 Station: WSTRBORK 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= 4517.00 4517.00 4517.00 4517.00 4517.00 4517.00 4517.00 4517.00 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 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 2 Setup file default. Used with PCAL = off LO sum= 4888.00 4888.00 4888.00 4888.00 4952.00 4952.00 4952.00 4952.00 BBC fr= 371.00 371.00 371.00 371.00 435.00 435.00 435.00 435.00 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 2 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 55.589590 * 02 37 52.405677 02 39 13.026135 0.00 * J0237+2848 28 35 11.40773 * 28 48 08.98999 28 54 10.55296 0.00 J0237+28 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 58420 observations. 3C84 03 16 29.567265 * 03 19 48.160096 03 21 19.007236 1.50 * J0319+4130 41 19 51.91692 * 41 30 42.10404 41 35 50.08200 2.86 0316+413 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J0319+41 GSFC 2016a X/S astro solution, 10291 observations. 0528+134 05 28 06.759216 * 05 30 56.416746 05 32 14.823942 0.21 * J0530+1331 13 29 42.28882 * 13 31 55.14948 13 32 56.79103 0.24 J0530+13 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 138236 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 sess123.C4096 1 2 3 4 5 6 7 8 9 11 12 13 0.817 139.650 J0319+4130 sess123.C4096 1 2 3 4 5 6 7 8 9 11 12 13 0.833 142.500 J0530+1331 sess123.C4096 1 2 3 4 5 6 7 8 9 11 12 13 0.383 63.848 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 72.2 J0319+4130 84.7 J0530+1331 108.2 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