COVER INFORMATION Station: HART (Code Hh ) Experiment: 6cm FTP Fringe Test F14C2 Exp. Code: F14C2 Schedule Version: 2.00 Processed by SCHED version: 10.20 Release of about July 12, 2012 PI: Ciriaco GODDI Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596548 EMAIL: goddi@jive.nl Fax: Phone during observation: +31-521-596548 Observing mode: Notes: 6cm FTP Fringe Test for Session 2/2014 512 Mbps, L+R, 2-bit sampling, 16 MHz filters (USB-only mode) Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 6cm ftp fringe-test F14C2 on 09 June 2014 involving 14 antennas: Eb Wb Jb1 Cm On25 Nt Tr Sv Zc Bd Sh T6 Hh Ys (Yd, Td). Stations testing their new DBBC backends are also included: YS_DBBC (Yd) and TM_DBBC (Td). The ftp test uses a USB-only/16MHz setup with 512 Mbps. The schedule consists of long integrations on QSO J0559+2353 (1 Jy at 5 GHz) and standard fringe finder DA193 (5 Jy at 5 GHz). There are two ftp fringe-test scans (1) 10:39:00 UT (scan 2, 2 sec, J0559+2353) (2) 11:15:00 UT (scan 6, 2 sec, DA193) Please make sure that the autoftp is set up correctly. See you on Skype group chat and Good luck with the session! Ciriaco Goddi Support Scientist, JIVE Skype account: ciriaco.goddi Schedule for HART (Code Hh ) Page 2 6cm FTP Fringe Test F14C2 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 ---------------------------------------------------------------------------------------- --- Mon 9 Jun 2014 Day 160 --- Next scan frequencies: 4958.49 4958.49 4974.49 4974.49 4990.49 4990.49 5006.49 5006.49 Next BBC frequencies: 358.49 358.49 374.49 374.49 390.49 390.49 406.49 406.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 10 30 00 J0559+2353 05 31 37 39.7 8.6 -0.5 0.0 0 0 10 30 00 10 34 00 =0556+238 05 35 37 39.9 7.4 -0.4 0.0 240 15 10 30 01 10 36 00 J0559+2353 05 37 38 39.9 6.8 -0.4 0.0 99 15 10 36 00 10 40 00 =0556+238 05 41 38 40.0 5.6 -0.3 0.0 240 31 10 36 01 10 42 00 J0559+2353 05 43 39 40.0 5.0 -0.3 0.0 99 31 10 42 00 10 52 00 =0556+238 05 53 40 40.2 2.0 -0.1 0.0 600 70 10 42 01 10 54 00 J0559+2353 05 55 41 40.2 1.4 -0.1 0.0 99 70 10 54 00 11 04 00 =0556+238 06 05 42 40.2 358.4 0.1 0.0 600 108 10 54 01 11 08 00 DA193 06 09 43 24.2 357.2 0.2 0.0 181 108 11 08 00 11 11 00 --- 06 12 43 24.2 356.6 0.3 0.0 180 120 11 08 01 11 13 00 DA193 06 14 44 24.2 356.2 0.3 0.0 99 120 11 13 00 11 17 00 --- 06 18 44 24.1 355.3 0.4 0.0 240 135 11 13 01 11 20 00 DA193 06 21 45 24.0 354.7 0.4 0.0 159 135 11 20 00 11 30 00 --- 06 31 47 23.8 352.6 0.6 0.0 600 174 11 20 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess214.C512 --- WARNING --- This group does not match an entry in the frequency catalog. This might be ok because the catalog is not complete. But be very careful to be sure that the setup is correct. Setup group: 10 Station: HART Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 8 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 Net SB= U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 5 2 6 3 7 4 8 BBC SB= U U U U U U U U IF = A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 13 Setup file default. LO sum= 4958.49 4958.49 4974.49 4974.49 4990.49 4990.49 5006.49 5006.49 BBC fr= 358.49 358.49 374.49 374.49 390.49 390.49 406.49 406.49 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 13 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16 barrel=roll_off SOURCES USED IN RECORDING SCANS -- 6cm FTP Fringe Test F14C2 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) J0555+3948 05 52 01.407174 * 05 55 30.805616 05 56 30.144399 0.13 0552+398 39 48 21.94578 * 39 48 49.16493 39 48 46.39656 0.10 * DA193 /aps3/sched10.2/catalogs/sources.vlba J0555+39 rfc_2012b Petrov, 2012, unpublished 376994 observations 0.283 scan and 31.500 baseline hours in setup: sess214.C512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 11 12 13 14 15 16 * J0559+2353 05 56 28.691736 * 05 59 32.033135 06 00 24.043242 0.11 0556+238 23 53 45.20881 * 23 53 53.92668 23 53 45.16862 0.10 J0559+23 /aps3/sched10.2/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 14595 observations 0.467 scan and 56.000 baseline hours in setup: sess214.C512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 11 12 13 14 15 16 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) DA193 19.5 J0559+2353 11.5 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