COVER INFORMATION Station: SVETLOE (Code Sv ) Experiment: Network Monitoring Experiment Exp. Code: N15C2 Schedule Version: 2.00 Processed by SCHED version: 11.30 Version 11.3 update 1. April 14, 2014 PI: Minnie Mao Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: mao@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 6cm NME and 4 ftp fringe test for session 2/2015 512 Mbps, L+R, 2-bit sampling, 16 MHz filters Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 6cm NME and ftp fringe-test on 4 Jun 2015 involving 14 antennas: Eb Wb Jb1 On85 Mc Nt Tr Sh Sv Zc Bd Hh Ys Ar. The NME uses a standard 512 Mbps setup. The schedule consists of long integrations on strong calibrators (J0126+2559, J1051+2119) for ftp-fringe tests. (J1026+2559 ~1.4Jy/beam, J1051+2119 ~1.3Jy/beam) Four ftp-fringe tests are scheduled throughout the experiment: 12:09:00 (scan 2, 2 sec, J0126+2559) 13:15:00 (scan 8, 2 sec, J0126+2559) 13:43:00 (scan 11, 2 sec, J1051+2119) 14:49:00 (scan 17, 2 sec, J1051+2119) All antennas will participate in at least two FTP fringe tests. Please make sure that the autoftp is set up correctly. Thanks! Good luck with the session and see you on Skype! Minnie Skype account: mini_mintaka 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 ---------------------------------------------------------------------------------------- --- Thu 4 Jun 2015 Day 155 --- 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 12 00 00 J0126+2559 06 49 35 27.1 635.6 5.4 33.0 0 0 12 00 00 12 04 00 =0123+257 06 53 35 26.6 636.5 5.4 33.0 240 15 12 00 01 12 06 00 J0126+2559 06 55 36 26.4 636.9 5.5 32.9 114 15 12 06 00 12 10 00 =0123+257 06 59 36 25.9 637.7 5.5 32.9 240 31 12 06 01 12 12 00 J0126+2559 07 01 37 25.6 638.1 5.6 32.8 114 31 12 12 00 12 16 00 =0123+257 07 05 37 25.1 639.0 5.6 32.7 240 46 12 12 01 12 18 00 J0126+2559 07 07 38 24.9 639.4 5.7 32.7 114 46 12 18 00 12 32 00 =0123+257 07 21 40 23.2 642.3 5.9 32.3 840 100 12 18 01 12 34 00 J0126+2559 07 23 40 23.0 642.7 5.9 32.3 114 100 12 34 00 12 48 00 =0123+257 07 37 42 21.3 645.6 6.2 31.8 840 154 12 34 01 12 50 00 J0126+2559 07 39 43 21.0 646.0 6.2 31.8 114 154 12 50 00 13 04 00 =0123+257 07 53 45 19.4 648.9 6.4 31.2 840 208 12 50 01 13 06 00 J0126+2559 07 55 45 19.2 649.3 6.5 31.1 114 208 13 06 00 13 10 00 =0123+257 07 59 46 18.7 650.1 6.5 30.9 240 223 13 06 01 13 12 00 J0126+2559 08 01 46 18.5 650.5 6.6 30.9 114 223 13 12 00 13 16 00 =0123+257 08 05 47 18.0 651.3 6.6 30.7 240 238 13 12 01 13 18 00 J0126+2559 08 07 47 17.8 651.7 6.7 30.6 114 238 13 18 00 13 22 00 =0123+257 08 11 48 17.3 652.6 6.7 30.4 240 254 13 18 01 13 34 00 J1051+2119 08 23 50 42.9 489.7 -2.5 -24.0 530 254 13 34 00 13 38 00 =1049+215 08 27 51 43.3 490.9 -2.4 -23.5 240 269 13 34 01 13 40 00 J1051+2119 08 29 51 43.5 491.5 -2.4 -23.3 113 269 13 40 00 13 44 00 =1049+215 08 33 52 43.8 492.7 -2.3 -22.8 240 285 13 40 01 13 46 00 J1051+2119 08 35 52 44.0 493.3 -2.3 -22.6 113 285 13 46 00 13 50 00 =1049+215 08 39 53 44.4 494.5 -2.2 -22.1 240 300 13 46 01 13 52 00 J1051+2119 08 41 53 44.5 495.1 -2.2 -21.9 113 300 13 52 00 14 06 00 =1049+215 08 55 55 45.7 499.4 -1.9 -20.1 840 354 13 52 01 Schedule for SVETLOE (Code Sv ) 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 ---------------------------------------------------------------------------------------- --- Thu 4 Jun 2015 Day 155 --- 14 08 00 J1051+2119 08 57 56 45.9 500.0 -1.9 -19.8 113 354 14 08 00 14 22 00 =1049+215 09 11 58 46.9 504.5 -1.7 -17.8 840 408 14 08 01 14 24 00 J1051+2119 09 13 58 47.1 505.2 -1.6 -17.5 113 408 14 24 00 14 38 00 =1049+215 09 28 01 48.0 509.8 -1.4 -15.4 840 462 14 24 01 14 40 00 J1051+2119 09 30 01 48.1 510.5 -1.4 -15.1 113 462 14 40 00 14 44 00 =1049+215 09 34 02 48.4 511.9 -1.3 -14.4 240 477 14 40 01 14 46 00 J1051+2119 09 36 02 48.5 512.5 -1.3 -14.1 113 477 14 46 00 14 50 00 =1049+215 09 40 03 48.7 513.9 -1.2 -13.4 240 492 14 46 01 14 52 00 J1051+2119 09 42 03 48.8 514.6 -1.2 -13.1 113 492 14 52 00 15 00 00 =1049+215 09 50 04 49.2 517.4 -1.0 -11.7 480 523 14 52 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess215.C512 Matching groups in /aps3/opt/share/sched_11.3U1/catalogs/freq_RDBE.dat: kvzr_c Added by Des Small, 24 February 2012 Setup group: 3 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: 8 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: 8 9 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) * J0126+2559 01 23 57.254021 * 01 26 42.792640 01 27 33.431173 0.11 0123+257 25 43 27.95555 * 25 59 01.30009 26 03 36.08092 0.11 J0126+25 /aps3/opt/share/sched_11.3U1/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 1729 observations * J1051+2119 10 49 07.187573 * 10 51 48.789073 10 52 38.366574 0.11 1049+215 21 35 48.53736 * 21 19 52.31374 21 14 58.36810 0.11 J1051+21 /aps3/opt/share/sched_11.3U1/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 1666 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 J0126+2559 sess215.C512 1 2 3 4 6 7 8 10 11 1.100 63.317 J1051+2119 sess215.C512 1 2 3 4 6 7 8 10 13 15 1.167 106.150 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) J0126+2559 45.8 J1051+2119 82.8 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