COVER INFORMATION Station: HART (Code Hh ) Experiment: Ftp test Exp. Code: F07M2 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: C-band (5cm) ftp-test (256 Mbps, 2-bit sampling, 4 MHz filters) 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 ---------------------------------------------------------------------------------------- --- Tue 12 Jun 2007 Day 163 --- Next scan frequencies: 6653.99 6653.99 6653.99 6653.99 6661.99 6661.99 6661.99 6661.99 6669.99 6669.99 6669.99 6669.99 6677.99 6677.99 6677.99 6677.99 Next BBC frequencies: 143.99 143.99 143.99 143.99 151.99 151.99 151.99 151.99 159.99 159.99 159.99 159.99 167.99 167.99 167.99 167.99 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 16 00 00 4C39.25 11 13 09 20.6 338.3 1.8 0.0 0 1 1 0 16 00 00 16 10 00 --- 11 23 10 19.7 336.5 1.9 0.0 600 F 1 19 16 00 04 16 12 00 4C39.25 11 25 10 19.5 336.1 2.0 0.0 95 1 1 19 16 12 00 16 20 00 --- 11 33 12 18.8 334.7 2.1 0.0 480 F 1 35 16 12 04 16 26 00 3C273B 11 39 13 59.6 25.4 -0.8 0.0 245 1 1 35 16 26 00 16 33 00 --- 11 46 14 60.2 22.2 -0.7 0.0 420 F 1 48 16 26 04 16 35 00 3C273B 11 48 14 60.4 21.2 -0.7 0.0 95 1 1 48 16 35 00 16 40 00 --- 11 53 15 60.8 18.8 -0.6 0.0 300 F 1 58 16 35 04 16 41 00 3C273B 11 54 15 60.8 18.3 -0.6 0.0 36 1 1 58 16 41 00 16 50 00 --- 12 03 17 61.4 13.8 -0.4 0.0 540 F 1 75 16 41 04 16 52 00 3C273B 12 05 17 61.5 12.8 -0.4 0.0 95 1 1 75 16 52 00 17 00 00 --- 12 13 18 61.8 8.6 -0.3 0.0 480 F 1 91 16 52 04 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: FTP.5CM Matches group hh4.5cm_S2 in /aps3/sched/catalogs/freq.dat Values confirmed by E-mail Jonathan Quick 291100 (CR) ****** Only 63.98 of 64.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. Setup group: 9 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= 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 6510.00 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: 9 Setup file default. No pcal detection. LO sum= 6653.99 6653.99 6653.99 6653.99 6661.99 6661.99 6661.99 6661.99 6669.99 6669.99 6669.99 6669.99 6677.99 6677.99 6677.99 6677.99 BBC fr= 143.99 143.99 143.99 143.99 151.99 151.99 151.99 151.99 159.99 159.99 159.99 159.99 167.99 167.99 167.99 167.99 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) J0927+3902 09 23 55.319213 * 09 27 03.013934 09 27 30.735702 0.26 0923+392 39 15 23.56648 * 39 02 20.85188 39 00 37.04423 0.40 * 4C39.25 /aps3/sched/catalogs/sources.vlba J0927+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.300 scan hours, 10.800 baseline hours above horizon. J1229+0203 12 26 33.245836 * 12 29 06.699732 12 29 30.225579 0.30 1226+023 02 19 43.30565 * 02 03 08.59815 02 00 37.07111 0.20 3C273 /aps3/sched/catalogs/sources.vlba * 3C273B VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro J1229+02 0.483 scan hours, 17.400 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) 4C39.25 53.8 3C273B 104.6 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