COVER INFORMATION Station: HART (Code Hh ) Experiment: Ftp test Exp. Code: F07L1 Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: Zsolt Paragi Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596536 EMAIL: paragi@jive.nl Fax: Phone during observation: +31-521-596536 Observing mode: Notes: L-band ftp-test (256 Mbps, 2-bit sampling, 4 MHz filters) for se Please ftp the data to JOP13 at JIVE Schedule for HART (Code Hh ) Page 2 Ftp test 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 ---------------------------------------------------------------------------------------- --- Wed 7 Mar 2007 Day 66 --- Next scan frequencies: 1641.99 1641.99 1641.99 1641.99 1649.99 1649.99 1649.99 1649.99 1657.99 1657.99 1657.99 1657.99 1665.99 1665.99 1665.99 1665.99 Next BBC frequencies: 131.99 131.99 131.99 131.99 139.99 139.99 139.99 139.99 147.99 147.99 147.99 147.99 155.99 155.99 155.99 155.99 Next scan bandwidths: 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 4.00 12 00 00 0229+131 00 50 03 43.5 35.3 -1.7 0.0 0 1 1 0 12 00 00 12 10 00 --- 01 00 05 44.8 32.4 -1.5 0.0 600 F 1 19 12 00 04 12 11 00 0235+164 01 01 05 41.2 31.9 -1.6 0.0 27 1 1 19 12 11 00 12 20 00 --- 01 10 07 42.3 29.3 -1.5 0.0 540 F 1 37 12 11 04 12 21 00 0235+164 01 11 07 42.4 29.0 -1.5 0.0 36 1 1 37 12 21 00 12 30 00 --- 01 20 08 43.3 26.4 -1.3 0.0 540 F 1 54 12 21 04 12 33 00 3C84 01 23 09 17.3 22.5 -2.0 0.0 103 1 1 54 12 33 00 12 40 00 --- 01 30 10 17.9 21.3 -1.8 0.0 420 F 1 68 12 33 04 12 41 00 3C84 01 31 10 18.0 21.1 -1.8 0.0 36 1 1 68 12 41 00 12 50 00 --- 01 40 11 18.7 19.5 -1.7 0.0 540 F 1 85 12 41 04 12 51 00 3C84 01 41 12 18.8 19.3 -1.7 0.0 36 1 1 85 12 51 00 13 00 00 --- 01 50 13 19.4 17.7 -1.5 0.0 540 F 1 103 12 51 04 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: FTP.18CM Matches group hh18cm in /aps3/sched/catalogs/freq.dat Values confirmed by E-mail Jonathan Quick 291100 (CR) Setup group: 11 Station: HART Total bit rate: 256 Format: MKIV1:1 Bits per sample: 2 Sample rate: 8.000 Number of channels: 16 Speedup factor: 1.00 Disk used to record data. 1st LO= 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 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 = 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 this setup were used. Frequency Set: 11 Setup file default. No pcal detection. LO sum= 1641.99 1641.99 1641.99 1641.99 1649.99 1649.99 1649.99 1649.99 1657.99 1657.99 1657.99 1657.99 1665.99 1665.99 1665.99 1665.99 BBC fr= 131.99 131.99 131.99 131.99 139.99 139.99 139.99 139.99 147.99 147.99 147.99 147.99 155.99 155.99 155.99 155.99 Bandwd= 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 4.000 Track assignments are: track1= 2, 6, 10, 14, 18, 22, 26, 30, 3, 7, 11, 15, 19, 23, 27, 31 barrel=roll_off SOURCE LIST -- Ftp test 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) J0231+1322 02 29 02.524208 * 02 31 45.894055 02 32 08.777216 0.31 * 0229+131 13 09 40.78813 * 13 22 54.71628 13 24 51.16415 0.20 J0231+13 /aps3/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.167 scan hours, 9.167 baseline hours above horizon. J0238+1636 02 35 52.630215 * 02 38 38.930107 02 39 02.237147 0.31 * 0235+164 16 24 04.01620 * 16 36 59.27462 16 38 54.24455 0.20 J0238+16 /aps3/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.300 scan hours, 16.500 baseline hours above horizon. J0319+4130 03 16 29.567289 * 03 19 48.160119 03 20 16.043468 0.28 0316+413 41 19 51.91677 * 41 30 42.10389 41 32 28.51390 0.41 * 3C84 /aps3/sched/catalogs/sources.vlba J0319+41 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.417 scan hours, 22.917 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) 0229+131 53.4 0235+164 56.0 3C84 73.5 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