COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Network Monitoring Experiment Exp. Code: F14M1 Schedule Version: 2.00 Processed by SCHED version: 10.20 Release of about July 12, 2012 PI: Gabriele Surcis Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: surcis@jive.nl Fax: Phone during observation: +31-521-596508 Observing mode: Notes: Ftp fringe test for session 1/2014 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 5cm ftp fringe-test F13M1 on 27 Feb 2014 involving 9 antennas: Eb Wb Jb2 On25 Mc Nt Tr Sh Ys Sr (Td, Md, Yd). Two ftp-fringe tests are scheduled throughout the experiment: 13:09 UT (scan 2, 2 sec, 3C48) 13:59 UT (scan 8, 2 sec, DA193) Please make sure that the autoftp is set up correctly. Thanks! Good luck with the session! Gabriele Support Scientist, JIVE Schedule for SHANGHAI (Code Sh ) 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 27 Feb 2014 Day 58 --- Next scan frequencies: 6644.52 6644.52 6644.52 6644.52 6660.52 6660.52 6660.52 6660.52 6676.52 6676.52 6676.52 6676.52 6692.52 6692.52 6692.52 6692.52 Next BBC frequencies: 744.52 744.52 744.52 744.52 760.52 760.52 760.52 760.52 776.52 776.52 776.52 776.52 792.52 792.52 792.52 792.52 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 3C48 06 33 46 28.9 -66.5 4.9 69.9 0 0 12 00 00 12 05 00 --- 06 38 47 27.9 -66.1 5.0 69.4 300 19 12 00 01 12 06 00 3C48 06 39 47 27.7 -66.0 5.0 69.3 58 19 12 06 00 12 10 00 --- 06 43 48 26.9 -65.7 5.1 68.9 240 35 12 06 01 12 14 00 3C48 06 47 49 26.1 -65.4 5.2 68.5 238 35 12 14 00 12 20 00 --- 06 53 50 24.9 -64.8 5.3 67.9 360 58 12 14 01 12 22 00 DA193 06 55 50 75.1 -50.0 1.0 121.3 32 58 12 22 00 12 30 00 --- 07 03 51 73.8 -52.8 1.1 117.3 480 89 12 22 01 12 32 00 DA193 07 05 52 73.5 -53.5 1.2 116.4 118 89 12 32 00 12 40 00 --- 07 13 53 72.1 -55.6 1.3 113.0 480 120 12 32 01 12 42 00 DA193 07 15 53 71.7 -56.1 1.3 112.3 118 120 12 42 00 12 50 00 --- 07 23 54 70.3 -57.8 1.5 109.4 480 151 12 42 01 12 52 00 DA193 07 25 55 69.9 -58.2 1.5 108.7 118 151 12 52 00 13 00 00 --- 07 33 56 68.4 -59.5 1.6 106.2 480 182 12 52 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess114.M512 Matching groups in ./SH65.freq.dat: sh5cm Email from Shen Zhiqiang, 30 Jan 2010 Setup group: 6 Station: SHANGHAI 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= 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 Net SB= L L U U L L U U L L U U L L U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 2 1 2 3 4 3 4 5 6 5 6 7 8 7 8 BBC SB= L L U U L L U U L L U U L L U U IF = C A C A C A C A C A C A C A C A The following frequency sets based on these setups were used. Frequency Set: 9 Setup file default. Used pcal sets: 1 LO sum= 6644.52 6644.52 6644.52 6644.52 6660.52 6660.52 6660.52 6660.52 6676.52 6676.52 6676.52 6676.52 6692.52 6692.52 6692.52 6692.52 BBC fr= 744.52 744.52 744.52 744.52 760.52 760.52 760.52 760.52 776.52 776.52 776.52 776.52 792.52 792.52 792.52 792.52 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: 9 14 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 S5 S6 S7 S8 PCALXB2= M1 M2 M3 M4 M5 M6 M7 M8 PCALFR1= 0 0 0 0 0 0 0 0 PCALFR2= 0 0 0 0 0 0 0 0 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32 barrel=roll_off SOURCES USED IN RECORDING SCANS -- Network Monitoring Experiment Catalog positions marked with *. Precession of date coordinates is based on stop time of first scan. Names used in schedule marked with *. Short names used in VLA and SNAP files marked with +. Observation date used in B1950/J2000 coordinate conversion (PRECDATE): 1979.900 No adjustments are made for rates (DRA, DDEC). Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) J0137+3309 01 34 49.826374 * 01 37 41.299440 01 38 29.959329 0.52 0134+329 32 54 20.25881 * 33 09 35.13299 33 13 55.41232 0.50 * 3C48 /aps3/sched10.2/catalogs/sources.vlba J0137+33 rfc_2012b Petrov, 2012, unpublished 140 observations 0.250 scan and 22.750 baseline hours in setup: sess114.M512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 12 13 J0555+3948 05 52 01.407174 * 05 55 30.805616 05 56 31.625055 0.13 0552+398 39 48 21.94578 * 39 48 49.16493 39 48 52.17836 0.10 * DA193 /aps3/sched10.2/catalogs/sources.vlba J0555+39 rfc_2012b Petrov, 2012, unpublished 376994 observations 0.533 scan and 40.626 baseline hours in setup: sess114.M512 Frequency sets (dups not shown): 1 3 4 5 6 7 8 9 10 12 13 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) 3C48 59.0 DA193 109.6 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