COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: Network Monitoring Experiment Exp. Code: N16L1 Schedule Version: 2.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 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: 18cm NME and 4 ftp fringe tests for session 1/2016 512 Mbps, L+R, 2-bit sampling, 8 MHz filters Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 18cm NME and ftp fringe-test on 03 March 2016 involving 14 antennas: Ef Wb1 Jb1 O8 Mc Sh T6 Ur Tr Sv Zc Bd Hh Sr. The NME uses a standard 512 Mbps setup. The schedule consists of long integrations on strong calibrators (0234+285 & 3C84) for ftp-fringe tests. At 18cm, 0234+285 is ~1.3 Jy/beam and 3C84 is ~10.4Jy/beam) Four ftp-fringe tests are scheduled throughout the experiment: 12:09:00 (scan 2, 2 sec, 0234+285, all ants) 12:54:00 (scan 8, 2 sec, 3C84, Hh ~20deg) 13:39:00 (scan 14, 2 sec, 0234+285, Sh & T6 ~15deg) 14:24:00 (scan 20, 2 sec, 3C84, no Zc; Sh, T6, Hh ~20deg) 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 URUMQI (Code Ur ) 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 3 Mar 2016 Day 63 --- Next scan frequencies: 1634.49 1634.49 1634.49 1634.49 1650.49 1650.49 1650.49 1650.49 1666.49 1666.49 1666.49 1666.49 1682.49 1682.49 1682.49 1682.49 Next BBC frequencies: 334.49 334.49 334.49 334.49 350.49 350.49 350.49 350.49 366.49 366.49 366.49 366.49 382.49 382.49 382.49 382.49 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 0234+285 04 35 29 62.5 247.6 1.9 50.0 0 0 12 00 00 12 04 00 --- 04 39 30 61.8 248.8 2.0 50.6 240 15 12 00 04 12 06 00 0234+285 04 41 30 61.5 249.4 2.0 50.9 118 15 12 06 00 12 10 00 --- 04 45 31 60.8 250.6 2.1 51.4 240 31 12 06 04 12 12 00 0234+285 04 47 31 60.5 251.1 2.1 51.6 118 31 12 12 00 12 15 00 --- 04 50 32 60.0 251.9 2.2 52.0 180 42 12 12 04 12 16 00 0234+285 04 51 32 59.8 252.2 2.2 52.1 58 42 12 16 00 12 24 00 --- 04 59 33 58.4 254.3 2.3 52.9 480 73 12 16 04 12 25 00 0234+285 05 00 33 58.2 254.5 2.4 53.0 58 73 12 25 00 12 33 00 --- 05 08 35 56.8 256.5 2.5 53.7 480 104 12 25 04 12 34 00 0234+285 05 09 35 56.6 256.7 2.5 53.8 58 104 12 34 00 12 42 00 --- 05 17 36 55.2 258.6 2.6 54.3 480 135 12 34 04 12 45 00 3C84 05 20 37 68.0 275.4 2.0 74.9 151 135 12 45 00 12 49 00 --- 05 24 37 67.2 275.9 2.1 74.8 240 150 12 45 04 12 51 00 3C84 05 26 38 66.9 276.2 2.1 74.7 118 150 12 51 00 12 55 00 --- 05 30 38 66.2 276.7 2.2 74.4 240 165 12 51 04 12 57 00 3C84 05 32 39 65.8 276.9 2.2 74.3 118 165 12 57 00 13 00 00 --- 05 35 39 65.3 277.3 2.2 74.2 180 177 12 57 04 13 01 00 3C84 05 36 39 65.1 277.4 2.3 74.1 58 177 13 01 00 13 09 00 --- 05 44 41 63.6 278.4 2.4 73.7 480 208 13 01 04 13 10 00 3C84 05 45 41 63.5 278.5 2.4 73.6 58 208 13 10 00 13 18 00 --- 05 53 42 62.0 279.5 2.5 73.1 480 238 13 10 04 13 19 00 3C84 05 54 42 61.8 279.6 2.6 73.0 58 238 13 19 00 13 27 00 --- 06 02 44 60.4 280.5 2.7 72.5 480 269 13 19 04 13 30 00 0234+285 06 05 44 46.5 268.1 3.4 55.9 150 269 13 30 00 13 34 00 --- 06 09 45 45.8 268.8 3.5 55.9 240 285 13 30 04 Schedule for URUMQI (Code Ur ) 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 3 Mar 2016 Day 63 --- 13 36 00 0234+285 06 11 45 45.4 269.2 3.5 56.0 118 285 13 36 00 13 40 00 --- 06 15 46 44.7 269.9 3.6 56.0 240 300 13 36 04 13 42 00 0234+285 06 17 46 44.4 270.2 3.6 56.0 118 300 13 42 00 13 45 00 --- 06 20 47 43.8 270.7 3.7 56.0 180 312 13 42 04 13 46 00 0234+285 06 21 47 43.6 270.9 3.7 56.0 58 312 13 46 00 13 54 00 --- 06 29 48 42.2 272.2 3.8 55.9 480 342 13 46 04 13 55 00 0234+285 06 30 48 42.0 272.4 3.9 55.9 58 342 13 55 00 14 03 00 --- 06 38 50 40.5 273.7 4.0 55.8 480 373 13 55 04 14 04 00 0234+285 06 39 50 40.4 273.9 4.0 55.8 58 373 14 04 00 14 12 00 --- 06 47 51 38.9 275.2 4.2 55.6 480 404 14 04 04 14 15 00 3C84 06 50 51 51.9 285.8 3.5 69.0 150 404 14 15 00 14 19 00 --- 06 54 52 51.2 286.3 3.6 68.6 240 419 14 15 04 14 21 00 3C84 06 56 52 50.9 286.5 3.6 68.5 118 419 14 21 00 14 25 00 --- 07 00 53 50.2 286.9 3.7 68.1 240 435 14 21 04 14 27 00 3C84 07 02 53 49.8 287.1 3.7 68.0 118 435 14 27 00 14 30 00 --- 07 05 54 49.3 287.5 3.8 67.7 180 446 14 27 04 14 32 00 3C84 07 07 54 48.9 287.7 3.8 67.6 118 446 14 32 00 14 40 00 --- 07 15 56 47.6 288.5 3.9 66.9 480 477 14 32 04 14 42 00 3C84 07 17 56 47.2 288.8 4.0 66.7 118 477 14 42 00 14 50 00 --- 07 25 57 45.8 289.6 4.1 66.0 480 508 14 42 04 14 52 00 3C84 07 27 58 45.5 289.9 4.1 65.8 118 508 14 52 00 15 00 00 --- 07 35 59 44.1 290.7 4.3 65.1 480 538 14 52 04 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess116.L5nme Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat: ur18cm update L.Xiang 9Feb05 Setup group: 5 Station: URUMQI 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= 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 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 = 2 1 2 1 4 3 4 3 6 5 6 5 8 7 8 7 BBC SB= L L U U L L U U L L U U L L U U IF = 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N The following frequency sets based on these setups were used. Frequency Set: 13 Setup file default. Used with PCAL = off LO sum= 1634.49 1634.49 1634.49 1634.49 1650.49 1650.49 1650.49 1650.49 1666.49 1666.49 1666.49 1666.49 1682.49 1682.49 1682.49 1682.49 BBC fr= 334.49 334.49 334.49 334.49 350.49 350.49 350.49 350.49 366.49 366.49 366.49 366.49 382.49 382.49 382.49 382.49 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: 13 Track assignments are: track1= 20, 18, 4, 2, 24, 22, 8, 6, 28, 26, 12, 10, 32, 30, 16, 14 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 38 49.086810 0.00 J0237+2848 28 35 11.40776 * 28 48 08.99001 28 52 13.64079 0.00 J0237+28 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 54650 observations. * 3C84 03 16 29.567263 * 03 19 48.160094 03 20 52.163420 1.30 J0319+4130 41 19 51.91701 * 41 30 42.10413 41 34 08.86432 2.69 0316+413 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc J0319+41 GSFC 2015a astro solution, unpublished 10208 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 0234+285 sess116.L5nme 1 2 3 4 5 6 7 8 11 12 13 14 + 1.167 122.500 3C84 sess116.L5nme 1 2 3 4 5 6 7 8 11 12 13 14 + 1.167 110.833 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) 0234+285 63.6 3C84 76.5 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