COVER INFORMATION Station: VLBA_FD (Code Fd ) Experiment: 3mm observing with autopeak Exp. Code: BJ045D Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: Bill Junor Address: ISR-1, Space & Atmospheric Sciences MS D466, LANL, P.O. Box 1663 Los Alamos, New Mexico, 87545 U.S.A. Phone: 505 667 0788 EMAIL: bjunor@lanl.gov Fax: 505 665 7395 Phone during observation: 505 699 7692 Observing mode: 3mm 512-8-2 Notes: Will use reference pointing. COVER LETTER: BJ045 SUMMARY: This project needs about 40 hours times 28 baselines to meet the sensitivity requirements. This time can be accumulated in many separated sessions but MK should appear in all sessions. Each session should be a full track with all antennas to set the calibration and ensure full uv coverage. Tropospheric weather is the problem for these 3mm observations. 3C274 is mostly a night-time object now. 2 tapes per station. -------------------------------------------------------------------- Here is the official dynamic scheduling sheet: ================================================================ Preferred Dynamic Contraints. Alter [defaults] as desired. ================================================================ Equipment constraints: Stations. Below each station code, the "o" indicates an [optional] station that is to be used if it is available. Change "o" to "r" if the station is required or change "o" to "n" if the station is not to be used. SC HN NL FD LA PT KP OV BR MK n o o o o o o o n r Minimum number of stations [7]: May we swap PT for a single VLA antenna? [no] Consult http://www.aoc.nrao.edu/~gtaylor/y1gotcha.html to decide. If you adopt the default, then both PT and VLA1 must be in the stations list in the keyin file. Bands and polarizations. Below each band code, insert "R" if the righthand polarization is to be used, "L" if the lefthand polarization is to be used, "d" if dual polarizations are to be used, or "o" if the band is in your setups but scheduling should not be constrained by its availability. 90cm 50cm 20cm 13cm 6cm 4cm 2cm 1cm 7mm 3mm d Weather constraints: [appropriate for bands marked "L", "R", or "d" above and for at least the minimum number of stations] Best tropospheric conditions for 3mm. Date constraints: Preferred date(s), usually a series start [none]: Excluded dates plus reason [none]: Preferred interval between segments in days [none]: Special conditions (e.g., a series with different spacings in time) [See the comments at the top.]: Must include MK Schedule for VLBA_FD (Code Fd ) Page 2 3mm observing with autopeak 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sat 26 Aug 2006 Day 238 --- Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 17 23 12 3C273 08 46 42 30.2 107.3 -3.7 -55.3 0 1 1 0 Stopped 17 28 11 --- 08 51 42 31.2 108.1 -3.6 -54.9 299 S 1 0 Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 17 28 41 3C273 08 52 12 31.3 108.2 -3.6 -54.9 25 1 1 0 17 28 41 17 34 40 --- 08 58 12 32.5 109.2 -3.5 -54.4 359 F 1 23 17 28 59 17 36 40 3C274 09 00 12 38.2 98.6 -3.5 -60.6 102 1 1 23 17 36 40 17 47 38 --- 09 11 12 40.5 100.3 -3.3 -60.1 658 F 1 66 17 36 58 17 48 08 3C274 09 11 42 40.6 100.4 -3.3 -60.0 25 1 1 66 17 48 08 17 59 06 --- 09 22 42 42.9 102.2 -3.1 -59.4 658 F 1 108 17 48 26 18 01 06 3C274 09 24 42 43.3 102.5 -3.1 -59.3 113 1 1 108 18 01 06 18 12 04 --- 09 35 42 45.6 104.5 -2.9 -58.5 658 F 1 151 18 01 24 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 18 12 34 3C273 09 36 12 40.1 116.4 -2.9 -50.5 13 1 1 151 Stopped 18 17 33 --- 09 41 12 41.0 117.5 -2.8 -49.8 299 S 1 151 Schedule for VLBA_FD (Code Fd ) Page 3 3mm observing with autopeak 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sat 26 Aug 2006 Day 238 --- Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 18 18 03 3C273 09 41 42 41.1 117.6 -2.8 -49.8 25 1 1 151 18 18 03 18 24 02 --- 09 47 42 42.3 118.9 -2.7 -48.9 359 F 1 174 18 18 21 18 26 02 3C274 09 49 42 48.5 107.1 -2.7 -57.3 101 1 1 174 18 26 02 18 37 00 --- 10 00 42 50.8 109.4 -2.5 -56.2 658 F 1 216 18 26 20 18 37 30 3C274 10 01 12 50.9 109.5 -2.5 -56.1 25 1 1 216 18 37 30 18 48 28 --- 10 12 12 53.1 112.0 -2.3 -54.8 658 F 1 259 18 37 48 18 50 28 3C274 10 14 12 53.5 112.5 -2.3 -54.5 113 1 1 259 18 50 28 19 01 26 --- 10 25 12 55.7 115.2 -2.1 -52.8 658 F 1 301 18 50 46 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 19 01 56 3C273 10 25 42 49.1 128.4 -2.1 -42.5 11 1 1 301 Stopped 19 06 55 --- 10 30 42 49.9 129.8 -2.0 -41.4 299 S 1 301 Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 19 07 25 3C273 10 31 12 50.0 129.9 -2.0 -41.3 25 1 1 301 19 07 25 19 13 24 --- 10 37 12 51.0 131.7 -1.9 -40.0 359 F 1 324 19 07 43 19 15 24 3C274 10 39 12 58.3 119.1 -1.9 -50.3 99 1 1 324 19 15 24 19 26 22 --- 10 50 12 60.4 122.6 -1.7 -47.9 658 F 1 367 19 15 42 Schedule for VLBA_FD (Code Fd ) Page 4 3mm observing with autopeak 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sat 26 Aug 2006 Day 238 --- 19 26 52 3C274 10 50 42 60.5 122.7 -1.7 -47.8 25 1 1 367 19 26 52 19 37 50 --- 11 01 42 62.4 126.6 -1.5 -45.0 658 F 1 409 19 27 10 19 39 50 3C274 11 03 42 62.8 127.4 -1.5 -44.4 113 1 1 409 19 39 50 19 50 48 --- 11 14 42 64.6 131.8 -1.3 -41.0 658 F 1 452 19 40 08 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 19 51 18 3C273 11 15 12 56.4 144.9 -1.2 -29.7 8 1 1 452 Stopped 19 56 17 --- 11 20 12 57.0 146.9 -1.2 -28.1 299 S 1 452 Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 19 56 47 3C273 11 20 42 57.1 147.1 -1.1 -27.9 25 1 1 452 19 56 47 20 02 46 --- 11 26 42 57.8 149.6 -1.0 -25.9 359 F 1 475 19 57 05 20 04 45 3C274 11 28 42 66.7 138.3 -1.0 -35.9 96 1 1 475 20 04 45 20 15 44 --- 11 39 42 68.2 144.2 -0.9 -31.0 658 F 1 517 20 05 03 20 16 14 3C274 11 40 12 68.3 144.4 -0.8 -30.8 25 1 1 517 20 16 14 20 27 12 --- 11 51 12 69.5 151.0 -0.7 -25.2 658 F 1 560 20 16 32 20 29 11 3C274 11 53 12 69.7 152.3 -0.6 -24.2 113 1 1 560 20 29 11 20 40 10 --- 12 04 12 70.7 159.7 -0.4 -17.8 658 F 1 602 20 29 29 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 20 40 40 3C273 12 04 42 60.8 167.3 -0.4 -10.9 4 1 1 602 Stopped 20 45 39 --- 12 09 42 61.0 169.8 -0.3 -8.8 299 S 1 602 Schedule for VLBA_FD (Code Fd ) Page 5 3mm observing with autopeak 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sat 26 Aug 2006 Day 238 --- Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 20 46 09 3C273 12 10 12 61.0 170.0 -0.3 -8.6 25 1 1 602 20 46 09 20 52 08 --- 12 16 12 61.2 173.1 -0.2 -5.9 359 F 1 625 20 46 27 20 54 07 3C274 12 18 12 71.5 170.0 -0.2 -8.8 93 1 1 625 20 54 07 21 05 06 --- 12 29 12 71.7 178.5 0.0 -1.3 658 F 1 668 20 54 25 21 05 35 3C274 12 29 42 71.7 178.9 0.0 -1.0 24 1 1 668 21 05 35 21 16 34 --- 12 40 42 71.6 187.4 0.2 6.5 658 F 1 710 21 05 53 21 18 33 3C274 12 42 42 71.5 188.9 0.2 7.9 113 1 1 710 21 18 33 21 29 32 --- 12 53 42 71.0 197.1 0.4 15.0 658 F 1 753 21 18 51 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 21 30 01 3C273 12 54 12 60.8 192.8 0.4 11.0 4 1 1 753 Stopped 21 35 01 --- 12 59 12 60.5 195.2 0.5 13.1 299 S 1 753 Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 21 35 31 3C273 12 59 42 60.5 195.5 0.5 13.3 25 1 1 753 21 35 31 21 41 30 --- 13 05 42 60.1 198.4 0.6 15.8 359 F 1 776 21 35 49 21 43 29 3C274 13 07 42 69.9 206.8 0.6 23.4 94 1 1 776 21 43 29 21 54 27 --- 13 18 42 68.7 213.6 0.8 29.2 658 F 1 818 21 43 47 Schedule for VLBA_FD (Code Fd ) Page 6 3mm observing with autopeak 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sat 26 Aug 2006 Day 238 --- 21 54 57 3C274 13 19 12 68.6 213.9 0.8 29.4 25 1 1 818 21 54 57 22 05 56 --- 13 30 12 67.2 219.9 1.0 34.4 658 F 1 861 21 55 15 22 07 55 3C274 13 32 12 66.9 221.0 1.0 35.3 113 1 1 861 22 07 55 22 18 53 --- 13 43 12 65.3 226.2 1.2 39.5 658 F 1 903 22 08 13 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 22 19 23 3C273 13 43 42 56.4 215.1 1.2 29.7 6 1 1 903 Stopped 22 24 22 --- 13 48 42 55.8 217.0 1.3 31.2 299 S 1 903 Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 22 24 52 3C273 13 49 12 55.7 217.2 1.3 31.4 25 1 1 903 22 24 52 22 30 51 --- 13 55 12 54.9 219.5 1.4 33.2 359 F 1 926 22 25 10 22 32 51 3C274 13 57 12 63.0 232.1 1.4 44.0 98 1 1 926 22 32 51 22 43 49 --- 14 08 12 61.1 236.1 1.6 47.0 658 F 1 969 22 33 09 22 44 19 3C274 14 08 42 61.0 236.3 1.6 47.1 25 1 1 969 22 44 19 22 55 17 --- 14 19 42 59.0 239.8 1.8 49.6 658 F 1 1011 22 44 37 22 57 17 3C274 14 21 42 58.6 240.5 1.8 50.0 113 1 1 1011 22 57 17 23 08 15 --- 14 32 42 56.5 243.6 2.0 52.1 658 F 1 1054 22 57 35 Next scan frequencies: 43115.99 43115.99 43215.99 43215.99 Next BBC frequencies: 715.99 715.99 815.99 815.99 Next scan bandwidths: 16.00 16.00 16.00 16.00 23 08 45 3C273 14 33 12 49.1 231.7 2.1 42.5 9 1 1 1054 Stopped 23 13 44 --- 14 38 12 48.2 233.0 2.1 43.5 299 S 1 1054 Schedule for VLBA_FD (Code Fd ) Page 7 3mm observing with autopeak 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sat 26 Aug 2006 Day 238 --- Next scan frequencies: 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 Next BBC frequencies: 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 23 14 14 3C273 14 38 42 48.1 233.2 2.2 43.6 25 1 1 1054 23 14 14 23 20 13 --- 14 44 42 47.1 234.8 2.3 44.7 359 F 1 1077 23 14 32 23 22 13 3C274 14 46 42 53.8 247.2 2.3 54.3 100 1 1 1077 23 22 13 23 33 11 --- 14 57 42 51.6 249.7 2.4 55.7 658 F 1 1119 23 22 31 23 33 41 3C274 14 58 12 51.5 249.8 2.5 55.8 25 1 1 1119 23 33 41 23 44 39 --- 15 09 12 49.2 252.2 2.6 57.0 658 F 1 1162 23 33 59 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: /home/filehost/cwalker/sched/setups/pt7mm.set Matches group v7mm_c8 in /home/filehost/cwalker/sched/catalogs/freq.dat Setup group: 11 Station: VLBA_FD Total bit rate: 256 Format: NONE Bits per sample: 2 Sample rate: 32.000 Number of channels: 4 Setup not used for recording data. 1st LO= 42400.00 42400.00 42400.00 42400.00 Net SB= U U U U Pol. = RCP LCP RCP LCP BBC = 1 2 3 4 BBC SB= U U U U IF = A C A C VLBA FE= 7mm omit 7mm omit VLBA Synth= 15.4 7.6 11.6 The following frequency sets based on this setup were used. Frequency Set: 3 Setup file default. Used pcal sets: 1 LO sum= 43115.99 43115.99 43215.99 43215.99 BBC fr= 715.99 715.99 815.99 815.99 Bandwd= 16.000 16.000 16.000 16.000 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 OFF OFF OFF OFF PCALXB2= M1 M2 M3 M4 OFF OFF OFF OFF PCALFR1= 0 0 0 0 0 0 0 0 PCALFR2= 0 0 0 0 0 0 0 0 Setup file: v3mm-512-8-2.set Matches group v3mm_ff in /home/filehost/cwalker/sched/catalogs/freq.dat Setup group: 3 Station: VLBA_FD Total bit rate: 512 Format: VLBA1:4 Bits per sample: 2 Sample rate: 32.000 Number of channels: 8 Speedup factor: 1.00 Disk used to record data. 1st LO= 85500.00 85500.00 85500.00 85500.00 85500.00 85500.00 85500.00 85500.00 Net SB= U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 2 3 4 5 6 7 8 BBC SB= U U U U U U U U IF = B D B D B D B D VLBA FE= omit 3mm omit 3mm VLBA Synth= 12.9 15.4 12.1 The following frequency sets based on this setup were used. Frequency Set: 10 Setup file default. Used pcal sets: 2 LO sum= 86212.49 86212.49 86228.49 86228.49 86244.49 86244.49 86260.49 86260.49 BBC fr= 712.49 712.49 728.49 728.49 744.49 744.49 760.49 760.49 Bandwd= 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 The following pulse cal sets were used with this setup: Pulse cal detection set: 2 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, 18, 3, 19, 66, 82, 67, 83 barrel=roll_off SOURCE LIST -- 3mm observing with autopeak 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) J1229+0203 12 26 33.245836 * 12 29 06.699732 12 29 26.217370 0.30 1226+023 02 19 43.30565 * 02 03 08.59815 02 01 02.05249 0.20 * 3C273 /home/filehost/cwalker/sched/catalogs/sources.vlba 3C273B VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro J1229+02 0.798 scan hours, 20.245 baseline hours above horizon. J1230+1223 12 28 17.569279 * 12 30 49.423381 12 31 08.814772 0.31 1228+126 12 40 01.74901 * 12 23 28.04383 12 21 23.37736 0.20 * 3C274 /home/filehost/cwalker/sched/catalogs/sources.vlba J1230+12 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 4.205 scan hours, 110.065 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) 3C273 32.8 3C274 31.8 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