COVER INFORMATION Station: EFLSBERG (Code Ef ) Experiment: 3.6cm NME and ftp fringe-test experiment Exp. Code: N11X1 Schedule Version: 1.00 Processed by SCHED version: 9.30 Release near March 23, 2010 PI: Jun Yang Address: JIVE Postbus 2, 7990 AA Dwingeloo The Netherlands Phone: +31 521 596 507 EMAIL: yang@jive.nl Fax: +353 91 750501 Phone during observation: Observing mode: (1) 512-16-2, RCP & LCP. (2) 1024-16-2, RCP only. Notes: See my cover letter. COVER LETTER: Dear EVN friends, N11X1 is 3.6cm (8.4GHz) NME and ftp fringe-test experiment. (1) Make sure that your auto-ftp setting is OK, please. (2) A test mode is used in last scan. The mode is: 1024 Mbps, RCP ONLY,8 BBCs, USB & LSB, 16 MHz filter, 2 bit sampling. Before the scan, I leave a long gap for ONSALA60 to insert attenuators for several BBCs. Furthermore, ZELENCHK and SVETLOE need to reconnect IF cables. (3) Note that the next user experiment EM085 will use both RCP and LCP to observe at 1 Gbps recording rate. If you reconnect IF cables because of the above test mode, you may need to get them back after N11X1. (4) The Kunming 40m radio telescope will participate in N11X1 to test its MK4 backend. Via the backend donated by the Westerbork Observatory and a new MK5B recorder, the new Chinese station is fully compatible with the EVN and other VLBI networks now. Four ftp tests are scheduled: ~12:07 UT (scan 1, 2 sec, J0237+2848) ~13:09 UT (scan 7, 2 sec, J0530+1331) ~14:09 UT (scan 13, 2 sec, J0530+1331) ~15:59 UT (scan 18, 2 sec, J0530+1331) See you in skype group chat! Jun Yang skype account: uaoagn Schedule for EFLSBERG (Code Ef ) Page 2 3.6cm NME and ftp fringe-test experiment 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 ---------------------------------------------------------------------------------------- --- Mon 14 Mar 2011 Day 73 --- Next scan frequencies: 8391.49 8391.49 8391.49 8391.49 8407.49 8407.49 8407.49 8407.49 8423.49 8423.49 8423.49 8423.49 8439.49 8439.49 8439.49 8439.49 Next BBC frequencies: 131.49 131.49 131.49 131.49 147.49 147.49 147.49 147.49 163.49 163.49 163.49 163.49 179.49 179.49 179.49 179.49 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 12 00 00 J0237+2848 23 54 34 52.4 109.5 -2.7 -43.2 0 1 1 0 12 00 00 12 08 00 =0234+285 00 02 35 53.6 111.6 -2.6 -42.4 480 F 1 31 12 00 04 12 10 00 J0237+2848 00 04 36 53.9 112.2 -2.6 -42.2 101 1 1 31 12 10 00 12 18 00 =0234+285 00 12 37 55.1 114.5 -2.4 -41.4 480 F 1 62 12 10 04 12 20 00 J0237+2848 00 14 37 55.4 115.0 -2.4 -41.1 100 1 1 62 12 20 00 12 28 00 =0234+285 00 22 39 56.5 117.4 -2.3 -40.1 480 F 1 93 12 20 04 12 30 00 J0237+2848 00 24 39 56.8 118.0 -2.2 -39.8 100 1 1 93 12 30 00 12 38 00 =0234+285 00 32 40 57.9 120.6 -2.1 -38.7 480 F 1 124 12 30 04 12 40 00 J0237+2848 00 34 41 58.2 121.2 -2.1 -38.4 100 1 1 124 12 40 00 12 48 00 =0234+285 00 42 42 59.3 123.9 -1.9 -37.1 480 F 1 155 12 40 04 12 50 00 J0237+2848 00 44 42 59.5 124.6 -1.9 -36.7 99 1 1 155 12 50 00 12 58 00 =0234+285 00 52 44 60.6 127.4 -1.8 -35.2 480 F 1 186 12 50 04 13 02 00 J0530+1331 00 56 44 23.9 97.8 -4.6 -40.4 72 1 1 186 13 02 00 13 10 00 =0528+134 01 04 46 25.2 99.4 -4.4 -40.2 480 F 1 217 13 02 04 13 12 00 J0530+1331 01 06 46 25.5 99.8 -4.4 -40.1 102 1 1 217 13 12 00 13 20 00 =0528+134 01 14 47 26.7 101.5 -4.3 -39.9 480 F 1 248 13 12 04 13 22 00 J0530+1331 01 16 48 27.0 101.9 -4.2 -39.8 102 1 1 248 13 22 00 13 30 00 =0528+134 01 24 49 28.3 103.6 -4.1 -39.5 480 F 1 279 13 22 04 13 32 00 J0530+1331 01 26 49 28.6 104.0 -4.1 -39.4 102 1 1 279 13 32 00 13 40 00 =0528+134 01 34 50 29.8 105.8 -3.9 -39.0 480 F 1 310 13 32 04 13 42 00 J0530+1331 01 36 51 30.1 106.2 -3.9 -38.9 102 1 1 310 13 42 00 13 50 00 =0528+134 01 44 52 31.3 108.0 -3.8 -38.5 480 F 1 341 13 42 04 Schedule for EFLSBERG (Code Ef ) Page 3 3.6cm NME and ftp fringe-test experiment 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 ---------------------------------------------------------------------------------------- --- Mon 14 Mar 2011 Day 73 --- 13 52 00 J0530+1331 01 46 52 31.6 108.4 -3.7 -38.3 102 1 1 341 13 52 00 14 00 00 =0528+134 01 54 54 32.9 110.2 -3.6 -37.9 480 F 1 372 13 52 04 14 02 00 J0530+1331 01 56 54 33.2 110.7 -3.6 -37.7 101 1 1 372 14 02 00 14 10 00 =0528+134 02 04 55 34.3 112.5 -3.4 -37.2 480 F 1 403 14 02 04 14 12 00 J0530+1331 02 06 56 34.6 113.0 -3.4 -37.0 101 1 1 403 14 12 00 14 20 00 =0528+134 02 14 57 35.8 114.9 -3.3 -36.4 480 F 1 434 14 12 04 14 22 00 J0530+1331 02 16 57 36.1 115.4 -3.2 -36.2 101 1 1 434 14 22 00 14 30 00 =0528+134 02 24 59 37.2 117.4 -3.1 -35.5 480 F 1 464 14 22 04 14 32 00 J0530+1331 02 26 59 37.5 117.9 -3.1 -35.3 101 1 1 464 14 32 00 14 40 00 =0528+134 02 35 00 38.6 119.9 -2.9 -34.5 480 F 1 495 14 32 04 Next scan frequencies: 8340.49 8340.49 8372.49 8372.49 8404.49 8404.49 8436.49 8436.49 8468.49 8468.49 8500.49 8500.49 8532.49 8532.49 8564.49 8564.49 Next BBC frequencies: 230.49 230.49 262.49 262.49 294.49 294.49 326.49 326.49 358.49 358.49 390.49 390.49 422.49 422.49 454.49 454.49 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 14 52 00 J0530+1331 02 47 02 40.3 123.1 -2.7 -33.2 686 1 1 495 14 52 00 15 00 00 =0528+134 02 55 04 41.3 125.2 -2.6 -32.3 480 F 1 557 14 52 28 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: kvsr.X512 Matching groups in ./n11x1_freq.dat: ef_x Setup group: 2 Station: EFLSBERG Total bit rate: 512 Format: MKIV1:2 Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 Speedup factor: 1.00 Disk used to record data. 1st LO= 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 8260.00 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 = 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 = 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N The following frequency sets based on this setup were used. Frequency Set: 2 Setup file default. LO sum= 8391.49 8391.49 8391.49 8391.49 8407.49 8407.49 8407.49 8407.49 8423.49 8423.49 8423.49 8423.49 8439.49 8439.49 8439.49 8439.49 BBC fr= 131.49 131.49 131.49 131.49 147.49 147.49 147.49 147.49 163.49 163.49 163.49 163.49 179.49 179.49 179.49 179.49 Bandwd= 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91 barrel=roll_off Setup file: X1024rcp Matching groups in ./n11x1_freq.dat: efgeosx special setup for Geodesy, contact friend of VLBI Setup group: 14 Station: EFLSBERG Total bit rate: 1024 Format: MKIV1:2 Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 Speedup factor: 0.50 Disk used to record data. 1st LO= 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 8110.00 Net SB= L U L U L U L U L U L U L U L U Pol. = RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP RCP BBC = 1 1 2 2 3 3 4 4 5 5 6 6 7 7 8 8 BBC SB= L U L U L U L U L U L U L U L U IF = 1N 1N 2A 2A 1N 1N 2A 2A 1N 1N 2A 2A 1N 1N 2A 2A The following frequency sets based on this setup were used. Frequency Set: 14 Setup file default. LO sum= 8340.49 8340.49 8372.49 8372.49 8404.49 8404.49 8436.49 8436.49 8468.49 8468.49 8500.49 8500.49 8532.49 8532.49 8564.49 8564.49 BBC fr= 230.49 230.49 262.49 262.49 294.49 294.49 326.49 326.49 358.49 358.49 390.49 390.49 422.49 422.49 454.49 454.49 Bandwd= 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91 barrel=roll_off SOURCE LIST -- 3.6cm NME and ftp fringe-test experiment 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) * J0237+2848 02 34 55.589591 * 02 37 52.405678 02 38 32.350636 0.01 0234+285 28 35 11.40782 * 28 48 08.99007 28 51 07.31079 0.01 J0237+28 /aps3/sched9.3/catalogs/sources.vlba GSFC Nov. 2009 Solution 2009a 53148 Observations 0.800 scan hours, 52.800 baseline hours above horizon. * J0530+1331 05 28 06.759217 * 05 30 56.416747 05 31 35.639390 0.00 0528+134 13 29 42.28889 * 13 31 55.14955 13 32 20.95310 0.01 J0530+13 /aps3/sched9.3/catalogs/sources.vlba GSFC Nov. 2009 Solution 2009a 129534 Observations 1.467 scan hours, 96.299 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) J0237+2848 53.7 J0530+1331 89.4 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