COVER INFORMATION Station: NOTO (Code Nt ) Experiment: Global VLBI Observations of the Hubble Deep Field Exp. Code: GG053A Schedule Version: 1.00 Processed by SCHED version: Release of 18 Sept. 2003 PI: Mike Garrett Address: JIVE Postbus 2 7990 AA Dwingeloo Netherlands Phone: +31 521 596511 EMAIL: garrett@jive.nfra.nl Fax: +31 521 596539 Phone during observation: +31 528 220842 Observing mode: 128-4-2 Notes: N.B. Observing frequency is 20CM Phase-referencing & Wide-field Imaging Only 1 WSRT antenna please Switch the phase-cal OFF during observations Schedule for NOTO (Code Nt ) Page 2 Global VLBI Observations of the Hubble Deep Field 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 23 Feb 2004 Day 54 --- Next scan frequencies: 1412.49 1412.49 Next BBC frequencies: 613.39 613.39 Next scan bandwidths: 8.00 8.00 07 50 00 J0927+3902 19 00 12 -6.9 -27.9 9.5 D 28.8 0 1 1 0 07 50 00 07 55 00 =0923+392 19 05 12 -7.4 -27.1 9.6 D 28.0 0 F 1 2000 08 01 00 J1241+602 19 11 13 28.1 -33.8 6.5 64.0 312 1 1 2000 08 01 00 08 03 30 --- 19 13 44 27.8 -33.7 6.5 63.6 150 F 1 3000 08 03 30 HDF 19 13 44 28.1 -31.5 6.6 63.5 -5 1 1 3000 08 03 30 08 08 30 --- 19 18 45 27.6 -31.2 6.7 62.6 295 F 1 5000 08 08 30 J1241+602 19 18 45 27.2 -33.3 6.6 62.6 -5 1 1 5000 08 08 30 08 11 00 --- 19 21 15 27.0 -33.2 6.7 62.1 145 F 1 6000 08 11 00 HDF 19 21 15 27.3 -31.0 6.7 62.1 -5 1 1 6000 08 11 00 08 15 30 --- 19 25 46 26.9 -30.7 6.8 61.2 265 F 1 7800 08 15 30 J1241+602 19 25 46 26.5 -32.9 6.7 61.3 -5 1 1 7800 08 15 30 08 18 00 --- 19 28 16 26.2 -32.7 6.8 60.8 145 F 1 8800 08 20 00 J1241+602 19 30 17 26.0 -32.6 6.8 60.5 118 1 1 8800 08 20 00 08 22 00 --- 19 32 17 25.8 -32.4 6.8 60.1 120 F 1 9600 08 22 00 HDF 19 32 17 26.2 -30.3 6.9 60.0 -5 1 1 9600 08 22 00 08 26 00 --- 19 36 18 25.8 -30.1 7.0 59.2 235 F 1 11200 08 26 00 J1234+619 19 36 18 25.4 -30.1 7.0 58.6 -3 1 1 11200 08 26 00 08 29 00 --- 19 39 18 25.1 -29.9 7.1 58.0 177 F 1 12400 08 29 00 HDF 19 39 18 25.5 -29.8 7.0 58.6 -3 1 1 12400 08 29 00 08 33 00 --- 19 43 19 25.1 -29.6 7.1 57.8 237 F 1 14000 08 33 00 J1241+602 19 43 19 24.6 -31.7 7.0 58.0 -5 1 1 14000 08 33 00 08 35 30 --- 19 45 49 24.3 -31.5 7.1 57.5 145 F 1 15000 08 35 30 HDF 19 45 49 24.9 -29.4 7.1 57.4 -5 1 1 15000 08 35 30 08 39 00 --- 19 49 20 24.5 -29.2 7.2 56.7 205 F 1 16400 08 39 00 J1234+619 19 49 20 24.1 -29.2 7.2 56.1 -3 1 1 16400 08 39 00 08 42 00 --- 19 52 20 23.8 -29.0 7.3 55.5 177 F 1 17600 Schedule for NOTO (Code Nt ) Page 3 Global VLBI Observations of the Hubble Deep Field 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 23 Feb 2004 Day 54 --- 08 44 00 J1241+602 19 54 21 23.4 -30.9 7.2 55.9 115 1 2 17600 08 44 00 08 46 00 --- 19 56 21 23.2 -30.7 7.2 55.6 120 R 1 16800 08 46 00 HDF 19 56 21 23.8 -28.7 7.3 55.3 -5 1 2 16800 08 46 00 08 50 30 --- 20 00 52 23.4 -28.3 7.4 54.5 265 R 1 15000 08 50 30 J1241+602 20 00 52 22.8 -30.4 7.3 54.7 -5 1 2 15000 08 50 30 08 53 00 --- 20 03 22 22.5 -30.2 7.4 54.3 145 R 1 14000 08 53 00 HDF 20 03 22 23.2 -28.1 7.4 54.0 -5 1 2 14000 08 53 00 08 57 00 --- 20 07 23 22.8 -27.8 7.5 53.2 235 R 1 12400 08 57 00 J1241+602 20 07 23 22.1 -29.8 7.4 53.5 -5 1 2 12400 08 57 00 08 59 30 --- 20 09 53 21.9 -29.6 7.5 53.0 145 R 1 11400 08 59 30 HDF 20 09 53 22.6 -27.6 7.5 52.7 -5 1 2 11400 08 59 30 09 03 30 --- 20 13 54 22.2 -27.3 7.6 52.0 235 R 1 9800 09 03 30 J1241+602 20 13 54 21.5 -29.3 7.5 52.3 -5 1 2 9800 09 03 30 09 06 00 --- 20 16 24 21.2 -29.1 7.6 51.8 145 R 1 8800 09 08 00 J1241+602 20 18 24 21.0 -28.9 7.6 51.4 118 1 2 8800 09 08 00 09 10 00 --- 20 20 25 20.9 -28.8 7.6 51.1 120 R 1 8000 09 10 00 HDF 20 20 25 21.6 -26.8 7.7 50.7 -5 1 2 8000 09 10 00 09 14 00 --- 20 24 25 21.2 -26.5 7.8 50.0 235 R 1 6400 09 14 00 J1234+619 20 24 25 20.8 -26.5 7.8 49.4 -3 1 2 6400 09 14 00 09 17 00 --- 20 27 26 20.6 -26.3 7.9 48.8 177 R 1 5200 09 17 00 HDF 20 27 26 21.0 -26.3 7.8 49.4 -3 1 2 5200 09 17 00 09 21 00 --- 20 31 27 20.6 -25.9 7.9 48.6 237 R 1 3600 09 21 00 J1241+602 20 31 27 19.8 -27.8 7.8 49.0 -5 1 2 3600 09 21 00 09 23 30 --- 20 33 57 19.6 -27.6 7.9 48.5 145 R 1 2600 09 23 30 HDF 20 33 57 20.4 -25.7 8.0 48.1 -5 1 2 2600 09 23 30 09 27 30 --- 20 37 58 20.0 -25.4 8.0 47.4 235 R 1 1000 09 27 30 J1234+619 20 37 58 19.7 -25.4 8.1 46.8 -3 1 2 1000 09 27 30 09 30 00 --- 20 40 28 19.5 -25.2 8.1 46.3 147 R 1 0 09 32 00 J1241+602 20 42 28 18.8 -26.9 8.0 46.9 116 1 1 0 09 32 00 09 34 00 --- 20 44 29 18.6 -26.7 8.0 46.5 120 F 2 800 Schedule for NOTO (Code Nt ) Page 4 Global VLBI Observations of the Hubble Deep Field 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 23 Feb 2004 Day 54 --- 09 34 00 HDF 20 44 29 19.5 -24.8 8.1 46.1 -5 1 1 800 09 34 00 09 38 30 --- 20 49 00 19.1 -24.5 8.2 45.2 265 F 2 2600 09 38 30 J1241+602 20 49 00 18.2 -26.3 8.1 45.7 -5 1 1 2600 09 38 30 09 41 00 --- 20 51 30 18.0 -26.1 8.2 45.2 145 F 2 3600 09 41 00 HDF 20 51 30 18.9 -24.2 8.2 44.7 -5 1 1 3600 09 41 00 09 45 00 --- 20 55 31 18.6 -23.9 8.3 44.0 235 F 2 5200 09 45 00 J1241+602 20 55 31 17.6 -25.7 8.2 44.5 -5 1 1 5200 09 45 00 09 47 30 --- 20 58 01 17.4 -25.5 8.3 44.0 145 F 2 6200 09 47 30 HDF 20 58 01 18.4 -23.7 8.4 43.5 -5 1 1 6200 09 47 30 09 51 30 --- 21 02 02 18.1 -23.3 8.4 42.7 235 F 2 7800 09 51 30 J1241+602 21 02 02 17.1 -25.1 8.3 43.2 -4 1 1 7800 09 51 30 09 54 00 --- 21 04 32 16.9 -24.8 8.4 42.7 146 F 2 8800 09 56 00 J1241+602 21 06 32 16.7 -24.7 8.4 42.4 118 1 1 8800 09 56 00 09 58 00 --- 21 08 33 16.5 -24.5 8.4 42.0 120 F 2 9600 09 58 00 HDF 21 08 33 17.6 -22.7 8.5 41.5 -4 1 1 9600 09 58 00 10 02 00 --- 21 12 33 17.2 -22.3 8.6 40.7 236 F 2 11200 10 02 00 J1234+619 21 12 33 16.9 -22.3 8.6 40.1 -3 1 1 11200 10 02 00 10 05 00 --- 21 15 34 16.6 -22.0 8.7 39.6 177 F 2 12400 10 05 00 HDF 21 15 34 17.0 -22.1 8.6 40.1 -3 1 1 12400 10 05 00 10 09 00 --- 21 19 35 16.7 -21.7 8.7 39.3 237 F 2 14000 10 09 00 J1241+602 21 19 35 15.6 -23.4 8.6 39.9 -4 1 1 14000 10 09 00 10 11 30 --- 21 22 05 15.4 -23.1 8.7 39.4 146 F 2 15000 10 11 30 HDF 21 22 05 16.5 -21.4 8.8 38.8 -4 1 1 15000 10 11 30 10 15 30 --- 21 26 06 16.2 -21.1 8.8 38.1 236 F 2 16600 10 15 30 J1234+619 21 26 06 15.9 -21.0 8.9 37.5 -3 1 1 16600 10 15 30 10 18 00 --- 21 28 36 15.7 -20.7 8.9 37.0 147 F 2 17600 10 20 00 J1241+602 21 30 36 14.8 -22.3 8.8 37.8 116 1 2 17600 10 20 00 10 22 00 --- 21 32 37 14.6 -22.1 8.8 37.4 120 R 2 16800 10 22 00 HDF 21 32 37 15.8 -20.4 8.9 36.8 -4 1 2 16800 10 22 00 10 26 30 --- 21 37 07 15.5 -20.0 9.0 35.9 266 R 2 15000 Schedule for NOTO (Code Nt ) Page 5 Global VLBI Observations of the Hubble Deep Field 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 23 Feb 2004 Day 54 --- 10 26 30 J1241+602 21 37 07 14.3 -21.6 8.9 36.5 -4 1 2 15000 10 26 30 10 29 00 --- 21 39 38 14.1 -21.4 9.0 36.1 146 R 2 14000 10 29 00 HDF 21 39 38 15.3 -19.7 9.0 35.4 -4 1 2 14000 10 29 00 10 33 00 --- 21 43 38 15.0 -19.3 9.1 34.6 236 R 2 12400 10 33 00 J1241+602 21 43 38 13.8 -20.9 9.0 35.3 -4 1 2 12400 10 33 00 10 35 30 --- 21 46 09 13.6 -20.7 9.1 34.8 146 R 2 11400 10 35 30 HDF 21 46 09 14.9 -19.1 9.2 34.1 -4 1 2 11400 10 35 30 10 39 30 --- 21 50 10 14.6 -18.7 9.2 33.4 236 R 2 9800 10 39 30 J1241+602 21 50 10 13.4 -20.3 9.1 34.0 -4 1 2 9800 10 39 30 10 42 00 --- 21 52 40 13.2 -20.0 9.2 33.5 146 R 2 8800 10 44 00 J1241+602 21 54 40 13.1 -19.8 9.2 33.2 118 1 2 8800 10 44 00 10 46 00 --- 21 56 41 12.9 -19.6 9.2 32.8 120 R 2 8000 10 46 00 HDF 21 56 41 14.2 -18.0 9.3 32.1 -5 1 2 8000 10 46 00 10 50 00 --- 22 00 41 14.0 -17.6 9.4 31.3 235 R 2 6400 10 50 00 J1234+619 22 00 41 13.6 -17.5 9.4 30.8 -3 1 2 6400 10 50 00 10 53 00 --- 22 03 42 13.4 -17.2 9.5 30.2 177 R 2 5200 10 53 00 HDF 22 03 42 13.8 -17.3 9.4 30.7 -3 1 2 5200 10 53 00 10 57 00 --- 22 07 42 13.5 -16.9 9.5 29.9 237 R 2 3600 10 57 00 J1241+602 22 07 42 12.2 -18.4 9.4 30.6 -5 1 2 3600 10 57 00 10 59 30 --- 22 10 13 12.0 -18.1 9.5 30.1 145 R 2 2600 10 59 30 HDF 22 10 13 13.4 -16.6 9.6 29.4 -5 1 2 2600 10 59 30 11 03 30 --- 22 14 13 13.2 -16.2 9.6 28.6 235 R 2 1000 11 03 30 J1234+619 22 14 13 12.8 -16.1 9.7 28.1 -3 1 2 1000 11 03 30 11 06 00 --- 22 16 44 12.7 -15.8 9.7 27.6 147 R 2 0 11 08 00 J1241+602 22 18 44 11.5 -17.2 9.6 28.5 116 1 3 0 11 08 00 11 10 00 --- 22 20 45 11.4 -16.9 9.7 28.1 120 F 1 800 11 10 00 HDF 22 20 45 12.8 -15.5 9.7 27.3 -5 1 3 800 11 10 00 11 14 30 --- 22 25 15 12.6 -15.1 9.8 26.4 265 F 1 2600 11 14 30 J1241+602 22 25 15 11.2 -16.4 9.7 27.2 -5 1 3 2600 11 14 30 11 17 00 --- 22 27 46 11.0 -16.2 9.8 26.7 145 F 1 3600 Schedule for NOTO (Code Nt ) Page 6 Global VLBI Observations of the Hubble Deep Field 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 23 Feb 2004 Day 54 --- 11 17 00 HDF 22 27 46 12.4 -14.8 9.8 26.0 -5 1 3 3600 11 17 00 11 21 00 --- 22 31 46 12.2 -14.4 9.9 25.2 235 F 1 5200 11 21 00 J1241+602 22 31 46 10.8 -15.7 9.8 25.9 -5 1 3 5200 11 21 00 11 23 30 --- 22 34 17 10.7 -15.4 9.9 25.4 145 F 1 6200 11 23 30 HDF 22 34 17 12.1 -14.1 10.0 24.7 -5 1 3 6200 11 23 30 11 27 30 --- 22 38 17 11.9 -13.6 10.0 23.9 235 F 1 7800 11 27 30 J1241+602 22 38 17 10.4 -15.0 9.9 24.7 -5 1 3 7800 11 27 30 11 30 00 --- 22 40 48 10.3 -14.7 10.0 24.2 145 F 1 8800 11 32 00 J1241+602 22 42 48 10.2 -14.4 10.0 23.8 118 1 3 8800 11 32 00 11 34 00 --- 22 44 48 10.1 -14.2 10.1 23.4 120 F 1 9600 11 34 00 HDF 22 44 48 11.6 -12.9 10.1 22.6 -5 1 3 9600 11 34 00 11 38 00 --- 22 48 49 11.4 -12.5 10.2 21.8 235 F 1 11200 11 38 00 J1234+619 22 48 49 11.1 -12.3 10.2 21.3 -3 1 3 11200 11 38 00 11 41 00 --- 22 51 50 11.0 -12.0 10.3 20.7 177 F 1 12400 11 41 00 HDF 22 51 50 11.3 -12.2 10.2 21.2 -3 1 3 12400 11 41 00 11 45 00 --- 22 55 50 11.2 -11.7 10.3 20.4 237 F 1 14000 11 45 00 J1241+602 22 55 50 9.6 -12.9 10.2 21.2 -5 1 3 14000 11 45 00 11 47 30 --- 22 58 21 9.5 -12.6 10.3 20.7 145 F 1 15000 11 47 30 HDF 22 58 21 11.1 -11.4 10.4 19.9 -5 1 3 15000 11 47 30 11 51 30 --- 23 02 21 10.9 -11.0 10.4 19.1 235 F 1 16600 11 51 30 J1234+619 23 02 21 10.6 -10.8 10.5 18.6 -3 1 3 16600 11 51 30 11 54 00 --- 23 04 52 10.5 -10.5 10.5 18.1 147 F 1 17600 11 56 00 HDF 23 06 52 10.7 -10.5 10.5 18.2 117 1 4 17600 11 56 00 12 00 00 --- 23 10 53 10.6 -10.0 10.6 17.4 240 R 1 16000 12 00 00 J1241+602 23 10 53 9.0 -11.2 10.5 18.2 -5 1 4 16000 12 00 00 12 02 00 --- 23 12 53 8.9 -10.9 10.5 17.8 115 R 1 15200 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: GG053.20cm Matches group nt18+21cm in /aps3/sched/catalogs/freq.dat LO from Trigilio 26Sep96 Setup group: 10 Station: NOTO Total bit rate: 64 Format: MKIV1:4 Bits per sample: 2 Sample rate: 16.000 Number of channels: 2 Passes/head pos: 2 Speedup factor: 2.00 Tape speeds: Low density - 135.000 ips, High density - 80.00 ips Time per pass for 17600 ft, High density tapes is: 00:44:00 1st LO= 799.10 799.10 Net SB= U U Pol. = RCP LCP BBC = 1 2 BBC SB= U U IF = C A The following frequency sets based on this setup were used. Frequency Set: 10 Setup file default. Used pcal sets: 1 LO sum= 1412.49 1412.49 BBC fr= 613.39 613.39 Bandwd= 8.000 8.000 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = 1MHZ PCALXB1= S1 S1 S1 S2 S1 OFF OFF OFF PCALXB2= S2 S2 M1 M2 S2 OFF OFF OFF PCALFR1= 510 6510 0 0 1510 0 0 0 PCALFR2= 510 6510 0 0 1510 0 0 0 Track assignments are: track1= 2, 18 track2= 3, 19 barrel=roll_off SOURCE LIST -- Global VLBI Observations of the Hubble Deep Field 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). Source Source position (RA/Dec) (B1950) (J2000) (Date) * J1241+602 12 39 16.511212 * 12 41 29.590769 12 41 42.825031 60 37 07.62228 * 60 20 41.32017 60 19 08.18860 From catalog imbedded in main SCHED input file. * J1234+619 12 31 56.132262 * 12 34 11.743000 12 34 25.392770 62 15 03.88430 * 61 58 32.48000 61 56 59.59153 From catalog imbedded in main SCHED input file. * HDF 12 34 28.059876 * 12 36 42.091690 12 36 55.625125 62 30 01.18651 * 62 13 31.42640 62 11 58.45225 From catalog imbedded in main SCHED input file. * J0927+3902 09 23 55.319195 * 09 27 03.013916 09 27 19.672839 0923+392 39 15 23.56655 * 39 02 20.85195 39 01 19.45818 4C39.25 /aps3/sched/catalogs/sources.vlba J0927+39 ICRF - Ext.1 Source - 1998 IERS Annual Report J1407+2827 14 04 45.615151 * 14 07 00.394410 14 07 11.908003 1404+286 28 41 29.23495 * 28 27 14.68998 28 25 49.51151 J1407+28 /aps3/sched/catalogs/sources.vlba * OQ208 ICRF - Ext.1 Source - 1998 IERS Annual Report 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) J1241+602 123.6 J1234+619 122.9 HDF 122.5 J0927+3902 148.5 OQ208 124.6 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