COVER INFORMATION Station: JB2_2G (Code Jf ) Experiment: Network Monitoring Experiment Exp. Code: N17C3 Schedule Version: 2.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Benito Marcote Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: marcote@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 6cm NME and ftp fringe test for session 3/2017 with 2 modes (512 and 2048 Mbps, L+R, 2-bit sampling, 8 and 32 MHz filters) Please send the disk pack by express to JIVE 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 2017 involving antennas: Jb2, Wb, Ef, Mc, Nt, On85, T6, Ur, Tr, Ys, Sv, Zc, Bd, Hh, Ir, Nk, and MERLIN outstations. The NME uses a standard setup with 512 Mbps during the first 2 hr. The NME uses a standard setup with 2048 Mbps during the last hr (Jb 2Gb). The schedule consists of: - long integrations on calibrator J1848+3219 for ftp-fringe tests; Strong fringes were found in N16C3 on this source. The following ftp-fringe tests are scheduled throughout the experiment (512 Mbps): 12:15:00 (scan 2, 2 sec, J1848+3219) 12:45:00 (scan 6, 2 sec, J1848+3219) 13:15:00 (scan 10, 2 sec, J1848+3219) 13:45:00 (scan 14, 2 sec, J1848+3219) Change to 2048 Mbps setup. 14:10:00 (scan 17, 2 sec, J1848+3219) 14:30:00 (scan 19, 2 sec, J1848+3219) 14:50:00 (scan 21, 2 sec, J1848+3219) Good luck with the session! Benito Marcote Skype account: jive.support.scientist Slack: evlbi.slack.com Schedule for JB2_2G (Code Jf ) 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 ---------------------------------------------------------------------------------------- --- Wed 25 Oct 2017 Day 298 --- Next scan frequencies: 4830.49 4830.49 4830.49 4830.49 4894.49 4894.49 4894.49 4894.49 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 Next BBC frequencies: 130.49 130.49 130.49 130.49 194.49 194.49 194.49 194.49 258.49 258.49 258.49 258.49 322.49 322.49 322.49 322.49 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 13 52 00 J1848+3219 15 59 22 53.3 107.5 -2.8 -42.5 0 0 13 52 00 13 56 00 =1846+322 16 03 22 53.9 108.5 -2.8 -42.2 240 62 13 52 01 14 01 00 J1848+3219 16 08 23 54.6 109.9 -2.7 -41.8 293 62 14 01 00 14 05 00 =1846+322 16 12 24 55.2 111.0 -2.6 -41.4 240 123 14 01 01 14 07 00 J1848+3219 16 14 24 55.4 111.5 -2.6 -41.2 114 123 14 07 00 14 12 00 =1846+322 16 19 25 56.1 113.0 -2.5 -40.7 300 200 14 07 01 14 19 00 J1848+3219 16 26 26 57.1 115.0 -2.4 -39.9 413 200 14 19 00 14 25 00 =1846+322 16 32 27 57.9 116.8 -2.3 -39.2 360 292 14 19 01 14 27 00 J1848+3219 16 34 28 58.2 117.5 -2.2 -38.9 114 292 14 27 00 14 32 00 =1846+322 16 39 28 58.8 119.0 -2.2 -38.3 300 369 14 27 01 14 39 00 J1848+3219 16 46 30 59.7 121.3 -2.0 -37.2 412 369 14 39 00 14 45 00 =1846+322 16 52 30 60.5 123.4 -1.9 -36.3 360 462 14 39 01 14 47 00 J1848+3219 16 54 31 60.7 124.1 -1.9 -35.9 114 462 14 47 00 14 52 00 =1846+322 16 59 32 61.4 125.9 -1.8 -35.0 300 538 14 47 01 14 56 00 J1848+3219 17 03 32 61.8 127.3 -1.8 -34.3 233 538 14 56 00 15 00 00 =1846+322 17 07 33 62.3 128.8 -1.7 -33.5 240 600 14 56 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess317.C2048nme --- 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: 25 Station: JB2_2G Total bit rate: 2048 Format: MARK5B 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= 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 4700.00 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 3 11 3 11 5 13 5 13 7 15 7 15 BBC SB= L L U U L L U U L L U U L L U U IF = A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 35 Setup file default. Used with PCAL = off LO sum= 4830.49 4830.49 4830.49 4830.49 4894.49 4894.49 4894.49 4894.49 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 BBC fr= 130.49 130.49 130.49 130.49 194.49 194.49 194.49 194.49 258.49 258.49 258.49 258.49 322.49 322.49 322.49 322.49 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: 35 Track assignments are: track1= 18, 26, 2, 10, 20, 28, 4, 12, 22, 30, 6, 14, 24, 32, 8, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 1846+322 18 46 29.612032 * 18 48 22.088575 18 49 01.039387 0.00 * J1848+3219 32 15 36.66046 * 32 19 02.60386 32 20 39.00936 0.00 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 29306 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 J1848+3219 sess317.C512nme 1 2 3 4 5 6 7 8 9 10 11 14 + 1.200 228.000 sess317.C2048nme 21 22 23 24 25 26 27 28 31 + 0.650 68.250 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) J1848+3219 82.0 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