COVER INFORMATION Station: SVETLOE (Code Sv ) Experiment: Network Monitoring Experiment Exp. Code: N19C2 Schedule Version: 4.00 Processed by SCHED version: 11.50 Development version 11.5. Started Apr. 2 PI: Benito Marcote Address: JIVE Oude Hoogeveensedijk 4 7991PD Dwingeloo The Netherlands Phone: +31 521 596 508 EMAIL: marcote@jive.eu Fax: Phone during observation: +31 521 596 508 Observing mode: Notes: 6cm NME and ftp fringe test for Session 2 2019 (512 Mbps, L+R, 2-bit sampling, 2 MHz filters) V4: adds out-stations COVER LETTER: This is the schedule for the 6cm NME and ftp fringe-test on 5th June 2019 involving antennas: Jb2, Wb, Ef, Mc, Nt, On85, T6, Ur, Tr, Ys, Hh, Sv, Zc, Bd, Ir, Ar, Km. Arecibo may join after 14:55UT. The NME uses a standard setup with 512 Mbps. The schedule consists of long integrations on calibrators J1014+2301 and J0336+3218 for ftp-fringe tests. The following ftp-fringe tests are scheduled throughout the experiment (UT times): 13:15:00 (scan 2, 2 sec, J1014+2301) 13:45:00 (scan 4, 2 sec, J1014+2301) 14:15:00 (scan 6, 2 sec, J1014+2301) 14:45:00 (scan 8, 2 sec, J1014+2301) 15:15:00 (scan 10, 2 sec, J0336+3218) --- Arecibo joins 15:45:00 (scan 12, 2 sec, J0336+3218) Good luck with the session! Benito Marcote Mattermost: coms.evlbi.org Schedule for SVETLOE (Code Sv ) 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 5 Jun 2019 Day 156 --- Next scan frequencies: 4966.49 4966.49 4966.49 4966.49 4982.49 4982.49 4982.49 4982.49 4998.49 4998.49 4998.49 4998.49 5014.49 5014.49 5014.49 5014.49 Next BBC frequencies: 466.49 466.49 466.49 466.49 482.49 482.49 482.49 482.49 498.49 498.49 498.49 498.49 514.49 514.49 514.49 514.49 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 13 00 00 J1014+2301 07 53 48 45.1 490.8 -2.4 -23.9 0 0 13 00 00 13 04 00 =1012+232 07 57 49 45.4 492.0 -2.3 -23.4 240 15 13 00 01 13 07 00 J1014+2301 08 00 50 45.7 492.9 -2.3 -23.0 173 15 13 07 00 13 17 00 =1012+232 08 10 51 46.6 496.0 -2.1 -21.8 600 54 13 07 01 13 20 00 J1014+2301 08 13 52 46.9 496.9 -2.0 -21.4 173 54 13 20 00 13 32 00 =1012+232 08 25 54 47.8 500.7 -1.8 -19.8 720 100 13 20 01 13 35 00 J1014+2301 08 28 54 48.1 501.7 -1.8 -19.3 173 100 13 35 00 13 47 00 =1012+232 08 40 56 48.9 505.7 -1.6 -17.5 720 146 13 35 01 13 50 00 J1014+2301 08 43 57 49.1 506.7 -1.5 -17.1 173 146 13 50 00 14 02 00 =1012+232 08 55 59 49.9 510.8 -1.3 -15.1 720 192 13 50 01 14 05 00 J1014+2301 08 58 59 50.1 511.8 -1.3 -14.6 173 192 14 05 00 14 17 00 =1012+232 09 11 01 50.7 516.0 -1.1 -12.5 720 238 14 05 01 14 20 00 J1014+2301 09 14 02 50.9 517.1 -1.0 -12.0 173 238 14 20 00 14 32 00 =1012+232 09 26 04 51.4 521.4 -0.8 -9.8 720 285 14 20 01 14 35 00 J1014+2301 09 29 04 51.5 522.5 -0.8 -9.2 173 285 14 35 00 14 47 00 =1012+232 09 41 06 51.9 527.0 -0.6 -6.9 720 331 14 35 01 14 55 10 J0336+3218 09 49 17 26.4 649.6 6.2 33.3 344 331 14 55 10 15 02 00 =NRAO140 09 56 08 25.6 651.0 6.3 32.9 410 357 14 55 11 15 05 00 J0336+3218 09 59 09 25.3 651.6 6.4 32.8 174 357 15 05 00 15 17 00 =NRAO140 10 11 11 23.9 653.9 6.6 32.2 720 403 15 05 01 15 20 00 J0336+3218 10 14 11 23.6 654.5 6.6 32.0 174 403 15 20 00 15 32 00 =NRAO140 10 26 13 22.3 656.8 6.8 31.3 720 449 15 20 01 15 35 00 J0336+3218 10 29 14 21.9 657.4 6.9 31.1 174 449 15 35 00 15 47 00 =NRAO140 10 41 16 20.6 659.8 7.1 30.4 720 496 15 35 01 15 50 00 J0336+3218 10 44 16 20.3 660.4 7.1 30.2 174 496 15 50 00 16 00 00 =NRAO140 10 54 18 19.3 662.3 7.3 29.5 600 534 15 50 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess219.C512 Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq_RDBE.dat: kvzr_c Added by Des Small, 24 February 2012 Setup group: 1 Station: SVETLOE Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 4500.00 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 = A B A B A B A B A B A B A B A B The following frequency sets based on these setups were used. Frequency Set: 12 Setup file default. Used with PCAL = off LO sum= 4966.49 4966.49 4966.49 4966.49 4982.49 4982.49 4982.49 4982.49 4998.49 4998.49 4998.49 4998.49 5014.49 5014.49 5014.49 5014.49 BBC fr= 466.49 466.49 466.49 466.49 482.49 482.49 482.49 482.49 498.49 498.49 498.49 498.49 514.49 514.49 514.49 514.49 Bandwd= 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 Matching frequency sets: 12 13 14 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) NRAO140 03 33 22.404686 * 03 36 30.107604 03 37 40.516290 0.01 * J0336+3218 32 08 36.66042 * 32 18 29.34218 32 22 04.11078 0.02 0333+321 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc J0336+32 GSFC 2016a X/S astro solution, 3443 observations. 1012+232 10 12 00.505069 * 10 14 47.065465 10 15 50.149061 0.02 * J1014+2301 23 16 12.09875 * 23 01 16.57077 22 55 37.31133 0.01 J1014+23 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 3941 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 J0336+3218 sess219.C512 1 2 3 4 5 6 9 10 12 17 18 2 + 0.881 104.717 J1014+2301 sess219.C512 1 2 3 4 5 6 7 8 9 10 11 12 + 1.433 301.000 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) J0336+3218 19.4 J1014+2301 73.2 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