COVER INFORMATION Station: YEBES40M (Code Ys ) Experiment: FTP Fringe Test Exp. Code: F14K1 Schedule Version: 2.00 Processed by SCHED version: 11.00 Release of Feb. 15, 2013 PI: Ivan Agudo Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596-549 EMAIL: agudo@jive.nl Fax: Phone during observation: +31-521-596-549 Observing mode: Notes: 1.3cm FTP Fringe Test for session 1/2014 1024 Mbps, 2-bit sampling, 16 MHz filters Participation from Sr (with DBBC), and Sh65 (TIANMA65 or T6) expected Additional DBBC testing data from Mc, Tr, and Ys is also expected. COVER LETTER: Dear EVN friends, This is the schedule for the 1.3cm FTP-FT on March 10 2011, involving 22 stations: Eb Jb2 On20 Mc Nt Tr Sv Zc Bd Ur Sh Hh Ys Mh Sr Ky, Ku, Kt, as well as Md Td Yd (Mc Tr and Ys with DBBC) and Sh65. The test uses a standard setup with 1024 Mbps and consists of two ftp fringe tests, interspersed with a longer set of scans on 0234+285 (~1.5 Jy source at 22 GHz). The two ftp fringe-test scans, start at: (1) 12:07:30 UT (scan 2, 2 sec) (2) 12:56:00 UT (scan 8, 2 sec) See you on Skype group chat and Good luck with the session! Ivan Support Scientist, JIVE Skype account: JIVE.Support.Scientist Schedule for YEBES40M (Code Ys ) Page 2 FTP Fringe Test 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 10 Mar 2014 Day 69 --- 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: 637.49 637.49 637.49 637.49 669.49 669.49 669.49 669.49 701.49 701.49 701.49 701.49 733.49 733.49 733.49 733.49 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 0234+285 23 00 00 44.3 87.0 -3.6 -60.1 0 0 12 00 00 12 04 00 --- 23 04 00 45.1 87.6 -3.6 -60.1 240 31 12 00 01 12 04 30 0234+285 23 04 30 45.2 87.7 -3.6 -60.1 15 31 12 04 30 12 08 30 --- 23 08 31 45.9 88.3 -3.5 -60.2 240 62 12 04 31 12 10 30 0234+285 23 10 31 46.3 88.6 -3.5 -60.2 105 62 12 10 30 12 18 30 --- 23 18 33 47.8 89.9 -3.3 -60.2 480 123 12 10 31 12 19 00 0234+285 23 19 03 47.9 90.0 -3.3 -60.2 15 123 12 19 00 12 27 00 --- 23 27 04 49.5 91.3 -3.2 -60.2 480 185 12 19 01 12 27 30 0234+285 23 27 34 49.5 91.4 -3.2 -60.2 15 185 12 27 30 12 35 30 --- 23 35 35 51.1 92.7 -3.1 -60.1 480 246 12 27 31 12 36 00 0234+285 23 36 06 51.2 92.8 -3.0 -60.1 15 246 12 36 00 12 44 00 --- 23 44 07 52.7 94.2 -2.9 -59.9 480 308 12 36 01 12 44 30 0234+285 23 44 37 52.8 94.3 -2.9 -59.9 15 308 12 44 30 12 52 30 --- 23 52 38 54.3 95.8 -2.8 -59.7 480 369 12 44 31 12 53 00 0234+285 23 53 08 54.4 95.9 -2.8 -59.7 15 369 12 53 00 12 57 00 --- 23 57 09 55.2 96.7 -2.7 -59.5 240 400 12 53 01 12 59 00 0234+285 23 59 09 55.5 97.1 -2.7 -59.5 105 400 12 59 00 13 00 00 --- 00 00 09 55.7 97.3 -2.6 -59.4 60 408 12 59 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess114.K1024 Matching groups in ./SH65.freq.dat: ys40_1cm LO value by Francisco Colomer (21MAY08), BBC 500-1000MHz Setup group: 6 Station: YEBES40M Total bit rate: 1024 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 21550.00 Net SB= L L U U L L U U L L U U L L U U IF SB = U U U U U U U U U U U U U U 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 = A C A C A C A C A C A C A C A C The following frequency sets based on these setups were used. Frequency Set: 13 Setup file default. Used pcal sets: 1 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= 637.49 637.49 637.49 637.49 669.49 669.49 669.49 669.49 701.49 701.49 701.49 701.49 733.49 733.49 733.49 733.49 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: 13 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 S5 S6 S7 S8 PCALXB2= M1 M2 M3 M4 M5 M6 M7 M8 PCALFR1= 0 0 0 0 0 0 0 0 PCALFR2= 0 0 0 0 0 0 0 0 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) J0237+2848 02 34 55.589591 * 02 37 52.405678 02 38 42.679952 0.11 * 0234+285 28 35 11.40773 * 28 48 08.98998 28 51 46.49950 0.10 J0237+28 /usr/local/sched/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 56811 observations SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Setup file Frequency sets Observing hours (duplicates not shown) Scan Baseline 0234+285 sess114.K1024 1 2 3 4 5 6 7 10 11 12 13 1 + 0.883 204.050 EFFECT OF SOLAR CORONA 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) 0234+285 57.4 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