COVER INFORMATION Station: IRBENE16 (Code Ib ) Experiment: Network Monitoring Experiment Exp. Code: N24C3 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; Feburary 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 3, 2024. EVN: 4 Gbps, 16 IFs, 32 MHz filters, L+R, 2-bit sampling MER: 512Mbps/2IF/64MHz, UR: 2Gbps/8IF/32MHz, W1: 1 Gbps/4IF/32MHz Please DO NOT use the phase cal signal. COVER LETTER: This is the schedule for the 6cm NME and ftp fringe test on 25 October 2024 involving 11 EVN antennas + eMERLIN: Jb2, Wb, Ef, O8, T6, Ur, Tr, Ys, Hh, Ir, Sr, Cm, Da, Kn, Pi, De. The NME uses a standard setup with a datarate of 4 Gbps, with eMERLIN at 0.5 Gbps, Ur at 2 Gbps, and Wb at 1 Gbps. The NME lasts for 3 hours and consists of long scans on calibrators: J1751+0939 and J2031+1219. with ftp grabs every other scan at the following times (in UT): 12:10:00 (scan 2, 2 sec, J1751+0939) 12:40:00 (scan 4, 2 sec, J1751+0939) 13:10:00 (scan 6, 2 sec, J2031+1219) 13:40:00 (scan 8, 2 sec, J2031+1219) 14:10:00 (scan 10, 2 sec, J2031+1219) 14:40:00 (scan 12, 2 sec, J2031+1219) 14:59:00 (scan 14, 2 sec, J2031+1219) Good luck with the session! Benito Marcote Mattermost: coms.evlbi.org Schedule for IRBENE16 (Code Ib ) 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 ---------------------------------------------------------------------------------------- --- Fri 25 Oct 2024 Day 299 --- Next scan frequencies: 4824.00 4824.00 4824.00 4824.00 4888.00 4888.00 4888.00 4888.00 4952.00 4952.00 4952.00 4952.00 5016.00 5016.00 5016.00 5016.00 Next BBC frequencies: 736.00 736.00 736.00 736.00 800.00 800.00 800.00 800.00 864.00 864.00 864.00 864.00 928.00 928.00 928.00 928.00 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 J1751+0939 15 44 52 36.2-220.3 -2.1 -20.6 0 0 12 00 00 12 02 00 =1749+096 15 46 52 36.3-219.7 -2.1 -20.3 120 31 12 00 01 12 07 00 J1751+0939 15 51 53 36.8-218.3 -2.0 -19.7 297 31 12 07 00 12 12 00 =1749+096 15 56 54 37.2-216.8 -1.9 -19.0 300 108 12 07 01 12 17 00 J1751+0939 16 01 55 37.6-215.3 -1.8 -18.3 297 108 12 17 00 12 27 00 =1749+096 16 11 56 38.3-212.3 -1.7 -16.9 600 263 12 17 01 12 32 00 J1751+0939 16 16 57 38.7-210.8 -1.6 -16.2 297 263 12 32 00 12 42 00 =1749+096 16 26 59 39.3-207.8 -1.4 -14.7 600 417 12 32 01 12 47 00 J2031+1219 16 31 59 26.2-250.9 -4.0 -31.3 275 417 12 47 00 12 57 00 =2029+121 16 42 01 27.4-248.6 -3.9 -30.7 600 572 12 47 01 13 02 00 J2031+1219 16 47 02 28.1-247.4 -3.8 -30.5 297 572 13 02 00 13 12 00 =2029+121 16 57 04 29.3-245.0 -3.6 -29.8 600 727 13 02 01 13 17 00 J2031+1219 17 02 04 29.9-243.7 -3.5 -29.5 297 727 13 17 00 13 27 00 =2029+121 17 12 06 31.1-241.3 -3.3 -28.8 600 881 13 17 01 13 32 00 J2031+1219 17 17 07 31.7-240.0 -3.3 -28.4 297 881 13 32 00 13 42 00 =2029+121 17 27 09 32.8-237.4 -3.1 -27.6 600 1036 13 32 01 13 47 00 J2031+1219 17 32 09 33.4-236.1 -3.0 -27.1 297 1036 13 47 00 13 57 00 =2029+121 17 42 11 34.5-233.5 -2.8 -26.2 600 1190 13 47 01 14 02 00 J2031+1219 17 47 12 35.0-232.2 -2.8 -25.7 297 1190 14 02 00 14 12 00 =2029+121 17 57 13 36.1-229.4 -2.6 -24.7 600 1345 14 02 01 14 17 00 J2031+1219 18 02 14 36.6-228.1 -2.5 -24.1 297 1345 14 17 00 14 27 00 =2029+121 18 12 16 37.6-225.3 -2.3 -23.0 600 1499 14 17 01 14 32 00 J2031+1219 18 17 17 38.0-223.8 -2.3 -22.4 297 1499 14 32 00 14 42 00 =2029+121 18 27 18 38.9-220.9 -2.1 -21.1 600 1654 14 32 01 14 47 00 J2031+1219 18 32 19 39.4-219.4 -2.0 -20.4 297 1654 14 47 00 14 52 00 =2029+121 18 37 20 39.8-217.9 -1.9 -19.7 300 1731 14 47 01 Schedule for IRBENE16 (Code Ib ) 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 ---------------------------------------------------------------------------------------- --- Fri 25 Oct 2024 Day 299 --- 14 57 00 J2031+1219 18 42 21 40.2-216.4 -1.8 -19.0 297 1731 14 57 00 15 00 00 =2029+121 18 45 21 40.4-215.5 -1.8 -18.6 180 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: sess324.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: 10 Station: IRBENE16 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= 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 4088.00 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= 4824.00 4824.00 4824.00 4824.00 4888.00 4888.00 4888.00 4888.00 4952.00 4952.00 4952.00 4952.00 5016.00 5016.00 5016.00 5016.00 BBC fr= 736.00 736.00 736.00 736.00 800.00 800.00 800.00 800.00 864.00 864.00 864.00 864.00 928.00 928.00 928.00 928.00 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) 1749+096 17 49 10.387930 * 17 51 32.818574 17 52 42.554513 0.00 * J1751+0939 09 39 42.82586 * 09 39 00.72841 09 38 43.72523 0.00 J1751+09 /Users/hawky/.pysched/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 192391 observations. 2029+121 20 29 32.681260 * 20 31 54.994267 20 33 05.414525 0.01 * J2031+1219 12 09 28.75299 * 12 19 41.34015 12 24 51.31940 0.02 J2031+12 /Users/hawky/.pysched/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 4314 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 J1751+0939 sess324.C4096 1 2 3 4 5 6 7 9 10 11 12 0.450 54.000 J2031+1219 sess324.C4096 1 2 3 4 5 6 7 9 10 11 12 1.467 176.000 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) J1751+0939 61.4 J2031+1219 100.1 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