COVER INFORMATION Station: MEDICINA (Code Mc ) Experiment: K-band Ftp test F13K2 Exp. Code: F13K2 Schedule Version: 1.00 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: K-band ftp test for session 3/2013 1 Gbps, 2-bit sampling, 16 MHz filters COVER LETTER: Dear EVN friends, This is the schedule for the K-band ftp fringe-test on 16 October 2013, involving 15 antennas: Eb Jb2 On20 Mc Nt Tr Mh Sv Zc Bd Ur Sh KVNYS KVNUS KVNTN. Stations testing their new DBBC backends are also included, with different names: MC_DBBC and TR_DBBC. The ftp test uses a setup with 1 Gbps and consists of long integrations on standard fringe finder calibrators: 3C345 (2 Jy at 22 GHz) and J1800+3848 (0.6 Jy at 22 GHz). There are two ftp fringe-test scans (1) 12:09:00 UT (scan 2, 2 sec, 3C345) (2) 12:45:00 UT (scan 6, 4 sec, J1800+3848) 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 MEDICINA (Code Mc ) Page 2 K-band Ftp test F13K2 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 ---------------------------------------------------------------------------------------- --- Wed 16 Oct 2013 Day 289 --- Next scan frequencies: 22187.49 22187.49 22187.49 22187.49 22219.49 22219.49 22219.49 22219.49 22251.49 22251.49 22251.49 22251.49 22283.49 22283.49 22283.49 22283.49 Next BBC frequencies: 223.49 223.49 223.49 223.49 255.49 255.49 255.49 255.49 287.49 287.49 287.49 287.49 319.49 319.49 319.49 319.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 12 00 00 3C345 14 27 15 64.5 448.7 -2.3 -68.1 0 0 12 00 00 12 04 00 --- 14 31 16 65.2 449.4 -2.2 -68.1 240 15 12 00 04 12 06 00 3C345 14 33 16 65.6 449.7 -2.2 -68.1 117 15 12 06 00 12 10 00 --- 14 37 17 66.3 450.4 -2.1 -68.1 240 31 12 06 04 12 12 00 3C345 14 39 17 66.7 450.8 -2.1 -68.1 117 31 12 12 00 12 22 00 --- 14 49 19 68.4 452.7 -1.9 -68.0 600 70 12 12 04 12 24 00 3C345 14 51 19 68.8 453.1 -1.9 -67.9 117 70 12 24 00 12 34 00 --- 15 01 21 70.6 455.2 -1.7 -67.5 600 108 12 24 04 12 38 00 J1800+3848 15 05 21 57.1 444.4 -2.9 -65.6 207 108 12 38 00 12 41 00 =1758+388 15 08 22 57.7 444.8 -2.9 -65.7 180 120 12 38 04 12 43 00 J1800+3848 15 10 22 58.0 445.1 -2.8 -65.8 117 120 12 43 00 12 47 00 =1758+388 15 14 23 58.7 445.7 -2.8 -65.9 240 135 12 43 04 12 50 00 J1800+3848 15 17 23 59.3 446.2 -2.7 -65.9 177 135 12 50 00 13 00 00 =1758+388 15 27 25 61.1 447.8 -2.6 -66.1 600 174 12 50 04 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess313.K1024 Matching groups in /aps3/sched10.2/catalogs/freq.dat: mc13mm values confirmed Maccaferri (CR 30Nov00) Setup group: 17 Station: MEDICINA Total bit rate: 512 Format: MKIV1:4 Bits per sample: 1 Sample rate: 32.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 21964.00 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 these setups were used. Frequency Set: 4 Setup file default. LO sum= 22187.49 22187.49 22187.49 22187.49 22219.49 22219.49 22219.49 22219.49 22251.49 22251.49 22251.49 22251.49 22283.49 22283.49 22283.49 22283.49 BBC fr= 223.49 223.49 223.49 223.49 255.49 255.49 255.49 255.49 287.49 287.49 287.49 287.49 319.49 319.49 319.49 319.49 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 4 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91 barrel=roll_off SOURCES USED IN RECORDING SCANS -- K-band Ftp test F13K2 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) J1642+3948 16 41 17.606228 * 16 42 58.809965 16 43 25.812651 0.77 * 3C345 39 54 10.81496 * 39 48 36.99402 39 47 25.57562 0.52 1641+399 /aps3/sched10.2/catalogs/sources.vlba J1642+39 GSFC 2011A astro solution 52621 Observations 0.467 scan and 56.000 baseline hours in setup: sess313.K1024 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 11 12 13 16 17 * J1800+3848 17 58 44.703952 * 18 00 24.765361 18 00 52.029998 0.13 1758+388 38 48 32.47341 * 38 48 30.69739 38 48 54.85660 0.10 J1800+38 /aps3/sched10.2/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 2965 observations 0.283 scan and 35.867 baseline hours in setup: sess313.K1024 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 11 12 13 16 17 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) 3C345 66.8 J1800+3848 79.5 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