COVER INFORMATION Station: CAMBG32M (Code Cm ) Experiment: Network Monitoring Experiment Exp. Code: N10M2 Schedule Version: 1.00 Processed by SCHED version: 9.30 Release near March 23, 2010 PI: Stefanie Muehle Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: muehle@jive.nl Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 5cm NME and ftp fringe test for session 2/2010 Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 5cm NME and ftp fringe-test on 01 June 2010. The NME uses a setup that mimics the astro setup of EB039G and EZ020A and that is typical for methanol spectral line experiments, but with 16 channels, i.e. using both sidebands of all BBCs, and 8 MHz filters. The schedule consists of long integrations on the strong calibrators 4C39.25 and J0958+4725 as well as a fast phase-referencing part. Three ftp-fringe tests are scheduled throughout the experiment. The data transfers are scheduled to begin at estimated max. transfer time (Sh): ~12:15 (scan 02, 4 sec, 4C39.25) 60min ~13:27 (scan 09, 4 sec, J0958+4725) 60min ~14:50 (scan 33, 8 sec, 4C39.25) 120min Please make sure that the autoftp is set up correctly. Thanks! Good luck with the session! Stefanie Schedule for CAMBG32M (Code Cm ) Page 2 Network Monitoring Experiment UP: D => Below limits; H => Below horizon mask. blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Tapes: Drive, Index, Start footage / Direction, Head Group, End footage. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Tue 1 Jun 2010 Day 152 --- Next scan frequencies: 6636.52 6636.52 6636.52 6636.52 6652.52 6652.52 6652.52 6652.52 6668.52 6668.52 6668.52 6668.52 6684.52 6684.52 6684.52 6684.52 Next BBC frequencies: 516.52 516.52 516.52 516.52 532.52 532.52 532.52 532.52 548.52 548.52 548.52 548.52 564.52 564.52 564.52 564.52 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 4C39.25 04 39 36 40.1 435.1 -4.8 -49.7 0 1 1 0 12 00 00 12 10 00 --- 04 49 38 41.6 436.8 -4.6 -50.2 600 F 1 39 12 00 01 12 11 00 4C39.25 04 50 38 41.7 436.9 -4.6 -50.2 45 1 1 39 12 11 00 12 16 00 --- 04 55 39 42.5 437.8 -4.5 -50.5 300 F 1 58 12 11 01 12 20 00 4C39.25 04 59 39 43.1 438.4 -4.5 -50.6 220 1 1 58 12 20 00 12 27 00 --- 05 06 41 44.1 439.6 -4.4 -50.9 420 F 1 85 12 20 01 12 28 00 4C39.25 05 07 41 44.3 439.8 -4.3 -51.0 45 1 1 85 12 28 00 12 38 00 --- 05 17 42 45.8 441.5 -4.2 -51.3 600 F 1 124 12 28 01 12 39 00 4C39.25 05 18 42 46.0 441.7 -4.2 -51.3 45 1 1 124 12 39 00 12 49 00 --- 05 28 44 47.5 443.5 -4.0 -51.6 600 F 1 163 12 39 01 12 50 00 4C39.25 05 29 44 47.6 443.7 -4.0 -51.7 45 1 1 163 12 50 00 13 00 00 --- 05 39 46 49.2 445.5 -3.8 -51.9 600 F 1 201 12 50 01 13 01 00 4C39.25 05 40 46 49.3 445.7 -3.8 -51.9 45 1 1 201 13 01 00 13 06 00 --- 05 45 47 50.1 446.6 -3.7 -52.0 300 F 1 221 13 01 01 13 08 00 J0958+4725 05 47 47 50.4 431.1 -4.2 -58.9 61 1 1 221 13 08 00 13 18 00 =0955+476 05 57 49 51.9 432.4 -4.0 -59.7 600 F 1 259 13 08 01 13 19 00 J0958+4725 05 58 49 52.0 432.6 -4.0 -59.8 45 1 1 259 13 19 00 13 29 00 =0955+476 06 08 51 53.5 434.0 -3.8 -60.5 600 F 1 298 13 19 01 13 33 00 4C39.25 06 12 51 54.2 451.9 -3.2 -52.1 178 1 1 298 13 33 00 13 38 00 --- 06 17 52 55.0 452.9 -3.2 -52.0 300 F 1 317 13 33 01 13 39 00 4C39.25 06 18 52 55.2 453.1 -3.1 -52.0 44 1 1 317 13 39 00 13 44 00 --- 06 23 53 55.9 454.2 -3.1 -51.9 300 F 1 337 13 39 01 Schedule for CAMBG32M (Code Cm ) Page 3 Network Monitoring Experiment UP: D => Below limits; H => Below horizon mask. blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Tapes: Drive, Index, Start footage / Direction, Head Group, End footage. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Tue 1 Jun 2010 Day 152 --- 13 45 00 4C39.25 06 24 53 56.1 454.4 -3.0 -51.9 44 1 1 337 13 45 00 13 46 30 --- 06 26 24 56.3 454.7 -3.0 -51.9 90 F 1 343 13 45 01 13 46 30 J0926+4029 06 26 24 57.4 452.8 -3.0 -53.6 -27 1 1 343 No stop 13 48 00 =0922+407 06 27 54 57.6 453.1 -3.0 -53.6 63 F 1 348 13 46 31 13 48 00 4C39.25 06 27 54 56.5 455.0 -3.0 -51.8 -27 1 1 348 No stop 13 49 30 --- 06 29 24 56.8 455.4 -3.0 -51.8 63 F 1 354 13 48 01 13 49 30 J0926+4029 06 29 24 57.8 453.4 -3.0 -53.6 -27 1 1 354 No stop 13 51 00 =0922+407 06 30 54 58.0 453.8 -2.9 -53.5 63 F 1 360 13 49 31 13 51 00 4C39.25 06 30 54 57.0 455.7 -2.9 -51.7 -27 1 1 360 No stop 13 52 30 --- 06 32 25 57.2 456.0 -2.9 -51.7 63 F 1 366 13 51 01 13 52 30 J0926+4029 06 32 25 58.3 454.1 -2.9 -53.5 -27 1 1 366 No stop 13 54 00 =0922+407 06 33 55 58.5 454.4 -2.9 -53.5 63 F 1 372 13 52 31 13 55 00 4C39.25 06 34 55 57.6 456.6 -2.9 -51.6 32 1 1 372 13 55 00 13 56 30 --- 06 36 25 57.8 456.9 -2.9 -51.6 90 F 1 377 13 55 01 13 56 30 J0926+4029 06 36 25 58.9 455.0 -2.8 -53.4 -27 1 1 377 No stop 13 58 00 =0922+407 06 37 55 59.1 455.3 -2.8 -53.4 63 F 1 383 13 56 31 13 58 00 4C39.25 06 37 55 58.1 457.3 -2.8 -51.5 -27 1 1 383 No stop 13 59 30 --- 06 39 26 58.3 457.6 -2.8 -51.5 63 F 1 389 13 58 01 13 59 30 J0926+4029 06 39 26 59.4 455.6 -2.8 -53.3 -28 1 1 389 No stop 14 01 00 =0922+407 06 40 56 59.6 456.0 -2.8 -53.3 62 F 1 395 13 59 31 14 01 00 4C39.25 06 40 56 58.5 458.0 -2.8 -51.4 -28 1 1 395 No stop 14 02 30 --- 06 42 26 58.8 458.3 -2.8 -51.3 62 F 1 401 14 01 01 14 02 30 J0926+4029 06 42 26 59.8 456.3 -2.7 -53.2 -28 1 1 401 No stop 14 04 00 =0922+407 06 43 56 60.0 456.6 -2.7 -53.2 62 F 1 406 14 02 31 14 05 00 4C39.25 06 44 57 59.1 458.9 -2.7 -51.2 31 1 1 406 14 05 00 14 06 30 --- 06 46 27 59.4 459.3 -2.7 -51.2 90 F 1 412 14 05 01 14 06 30 J0926+4029 06 46 27 60.4 457.2 -2.7 -53.1 -28 1 1 412 No stop 14 08 00 =0922+407 06 47 57 60.7 457.6 -2.6 -53.0 62 F 1 418 14 06 31 14 08 00 4C39.25 06 47 57 59.6 459.6 -2.7 -51.1 -28 1 1 418 No stop 14 09 30 --- 06 49 27 59.8 460.0 -2.6 -51.0 62 F 1 424 14 08 01 Schedule for CAMBG32M (Code Cm ) Page 4 Network Monitoring Experiment UP: D => Below limits; H => Below horizon mask. blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Tapes: Drive, Index, Start footage / Direction, Head Group, End footage. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Tue 1 Jun 2010 Day 152 --- 14 09 30 J0926+4029 06 49 27 60.9 457.9 -2.6 -53.0 -28 1 1 424 No stop 14 11 00 =0922+407 06 50 58 61.1 458.3 -2.6 -52.9 62 F 1 430 14 09 31 14 11 00 4C39.25 06 50 58 60.1 460.4 -2.6 -50.9 -28 1 1 430 No stop 14 12 30 --- 06 52 28 60.3 460.7 -2.6 -50.8 62 F 1 435 14 11 01 14 12 30 J0926+4029 06 52 28 61.3 458.6 -2.6 -52.8 -28 1 1 435 No stop 14 14 00 =0922+407 06 53 58 61.6 459.0 -2.5 -52.8 62 F 1 441 14 12 31 14 15 00 4C39.25 06 54 58 60.7 461.4 -2.5 -50.7 31 1 1 441 14 15 00 14 25 00 --- 07 05 00 62.2 464.0 -2.4 -50.0 600 F 1 480 14 15 01 14 26 00 4C39.25 07 06 00 62.3 464.2 -2.4 -49.9 44 1 1 480 14 26 00 14 34 00 --- 07 14 01 63.5 466.4 -2.2 -49.2 480 F 1 511 14 26 01 14 35 00 4C39.25 07 15 02 63.6 466.7 -2.2 -49.1 43 1 1 511 14 35 00 14 40 00 --- 07 20 02 64.4 468.2 -2.1 -48.6 300 F 1 530 14 35 01 14 41 00 4C39.25 07 21 03 64.5 468.5 -2.1 -48.5 43 1 1 530 14 41 00 14 51 00 --- 07 31 04 66.0 471.6 -1.9 -47.2 600 F 1 569 14 41 01 14 55 00 4C39.25 07 35 05 66.5 472.9 -1.9 -46.6 216 1 1 569 14 55 00 15 00 00 --- 07 40 06 67.2 474.7 -1.8 -45.8 300 F 1 588 14 55 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: nme.5cm Matching groups in ./n10m2_freq.dat: cm5cm MK2 LO setting-400MHz, P. Burgess (JFD 15Oct01) Setup group: 1 Station: CAMBG32M Total bit rate: 512 Format: MKIV1:2 Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 Speedup factor: 1.00 Disk used to record data. 1st LO= 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 6120.00 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 this setup were used. Frequency Set: 1 Setup file default. Used pcal sets: 1 LO sum= 6636.52 6636.52 6636.52 6636.52 6652.52 6652.52 6652.52 6652.52 6668.52 6668.52 6668.52 6668.52 6684.52 6684.52 6684.52 6684.52 BBC fr= 516.52 516.52 516.52 516.52 532.52 532.52 532.52 532.52 548.52 548.52 548.52 548.52 564.52 564.52 564.52 564.52 Bandwd= 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = 1MHZ PCALXB1= S1 S3 S5 S7 S9 S11 S13 S15 PCALXB2= S2 S4 S6 S8 S10 S12 S14 S16 PCALFR1= 520 480 520 480 520 480 520 480 PCALFR2= 520 480 520 480 520 480 520 480 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91 barrel=roll_off SOURCE LIST -- 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) * J0926+4029 09 22 50.724315 * 09 26 00.426850 09 26 40.518519 0.31 0922+407 40 42 49.48298 * 40 29 49.67273 40 27 12.32593 0.48 /aps3/sched/catalogs/sources.vlba Petrov Dec. 2009 Solution 2009c_astro 90 Observations 0.225 scan hours, 6.099 baseline hours above horizon. J0927+3902 09 23 55.319215 * 09 27 03.013936 09 27 42.696749 0.01 0923+392 39 15 23.56644 * 39 02 20.85184 38 59 42.50175 0.01 * 4C39.25 /aps3/sched/catalogs/sources.vlba J0927+39 GSFC Nov. 2009 Solution 2009a 226075 Observations 1.975 scan hours, 69.766 baseline hours above horizon. * J0958+4725 09 55 08.528426 * 09 58 19.671641 09 59 00.258331 0.01 0955+476 47 39 28.28174 * 47 25 07.84243 47 22 15.60754 0.01 J0958+47 /aps3/sched/catalogs/sources.vlba GSFC Nov. 2009 Solution 2009a 138317 Observations 0.333 scan hours, 12.000 baseline hours above horizon. 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) J0926+4029 62.7 4C39.25 63.1 J0958+4725 67.6 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