COVER INFORMATION Station: VLBA_KP (Code Kp ) Experiment: 3mm observing with autopeak Exp. Code: BJ045E 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_KP (Code Kp ) 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 ---------------------------------------------------------------------------------------- --- Thu 24 Aug 2006 Day 236 --- 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 31 04 3C273 08 16 02 23.5 103.1 -4.2 -55.8 0 1 1 0 Stopped 17 36 03 --- 08 21 02 24.5 103.8 -4.1 -55.5 299 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 36 33 3C273 08 21 32 24.6 103.9 -4.1 -55.5 25 1 1 0 17 36 33 17 42 32 --- 08 27 32 25.9 104.9 -4.0 -55.1 359 F 1 23 17 36 51 17 44 32 3C274 08 29 32 31.5 95.0 -4.0 -59.9 102 1 1 23 17 44 32 17 55 30 --- 08 40 32 33.8 96.6 -3.8 -59.6 658 F 1 66 17 44 50 17 56 00 3C274 08 41 02 33.9 96.6 -3.8 -59.6 25 1 1 66 17 56 00 18 06 58 --- 08 52 02 36.2 98.3 -3.7 -59.3 658 F 1 108 17 56 18 18 08 58 3C274 08 54 02 36.7 98.6 -3.6 -59.2 113 1 1 108 18 08 58 18 19 56 --- 09 05 02 39.0 100.4 -3.4 -58.7 658 F 1 151 18 09 16 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 20 26 3C273 09 05 32 33.5 111.3 -3.4 -52.3 13 1 1 151 Stopped 18 25 25 --- 09 10 32 34.5 112.3 -3.3 -51.8 299 S 1 151 Schedule for VLBA_KP (Code Kp ) 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 ---------------------------------------------------------------------------------------- --- Thu 24 Aug 2006 Day 236 --- 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 25 55 3C273 09 11 02 34.6 112.4 -3.3 -51.7 25 1 1 151 18 25 55 18 31 54 --- 09 17 02 35.8 113.5 -3.2 -51.1 359 F 1 174 18 26 13 18 33 53 3C274 09 19 02 41.9 102.7 -3.2 -57.9 102 1 1 174 18 33 53 18 44 52 --- 09 30 02 44.1 104.7 -3.0 -57.2 658 F 1 216 18 34 11 18 45 22 3C274 09 30 32 44.2 104.8 -3.0 -57.1 25 1 1 216 18 45 22 18 56 20 --- 09 41 32 46.5 106.9 -2.8 -56.2 658 F 1 259 18 45 40 18 58 19 3C274 09 43 32 46.9 107.3 -2.8 -56.0 113 1 1 259 18 58 19 19 09 18 --- 09 54 32 49.1 109.6 -2.6 -54.9 658 F 1 301 18 58 37 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 09 48 3C273 09 55 02 42.9 121.6 -2.6 -46.3 12 1 1 301 Stopped 19 14 47 --- 10 00 02 43.8 122.8 -2.5 -45.5 299 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 15 17 3C273 10 00 32 43.9 122.9 -2.5 -45.5 25 1 1 301 19 15 17 19 21 16 --- 10 06 32 45.0 124.4 -2.4 -44.5 359 F 1 324 19 15 35 19 23 15 3C274 10 08 32 51.9 112.7 -2.4 -53.2 100 1 1 324 19 23 15 19 34 14 --- 10 19 32 54.0 115.4 -2.2 -51.7 658 F 1 367 19 23 33 Schedule for VLBA_KP (Code Kp ) 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 ---------------------------------------------------------------------------------------- --- Thu 24 Aug 2006 Day 236 --- 19 34 43 3C274 10 20 02 54.1 115.6 -2.2 -51.6 25 1 1 367 19 34 43 19 45 42 --- 10 31 02 56.2 118.6 -2.0 -49.7 658 F 1 409 19 35 01 19 47 41 3C274 10 33 02 56.6 119.1 -2.0 -49.4 113 1 1 409 19 47 41 19 58 40 --- 10 44 02 58.6 122.5 -1.8 -47.1 658 F 1 452 19 47 59 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 59 09 3C273 10 44 32 51.2 135.2 -1.7 -36.7 9 1 1 452 Stopped 20 04 09 --- 10 49 32 51.9 136.8 -1.7 -35.5 299 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 20 04 39 3C273 10 50 02 52.0 137.0 -1.7 -35.4 25 1 1 452 20 04 39 20 10 38 --- 10 56 02 52.9 139.0 -1.6 -33.8 359 F 1 475 20 04 57 20 12 37 3C274 10 58 02 61.0 127.2 -1.6 -43.8 97 1 1 475 20 12 37 20 23 35 --- 11 09 02 62.8 131.5 -1.4 -40.6 658 F 1 517 20 12 55 20 24 05 3C274 11 09 32 62.9 131.7 -1.4 -40.5 25 1 1 517 20 24 05 20 35 04 --- 11 20 32 64.6 136.4 -1.2 -36.8 658 F 1 560 20 24 23 20 37 03 3C274 11 22 32 64.8 137.3 -1.1 -36.1 113 1 1 560 20 37 03 20 48 01 --- 11 33 32 66.3 142.7 -1.0 -31.7 658 F 1 602 20 37 21 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 48 31 3C273 11 34 02 57.3 153.7 -0.9 -22.1 6 1 1 602 Stopped 20 53 31 --- 11 39 02 57.8 155.9 -0.8 -20.3 299 S 1 602 Schedule for VLBA_KP (Code Kp ) 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 ---------------------------------------------------------------------------------------- --- Thu 24 Aug 2006 Day 236 --- 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 54 00 3C273 11 39 32 57.8 156.1 -0.8 -20.1 25 1 1 602 20 54 00 20 59 59 --- 11 45 32 58.3 158.8 -0.7 -17.9 359 F 1 625 20 54 18 21 01 59 3C274 11 47 32 68.0 150.5 -0.7 -25.4 94 1 1 625 21 01 59 21 12 57 --- 11 58 32 69.0 157.2 -0.5 -19.6 658 F 1 668 21 02 17 21 13 27 3C274 11 59 02 69.1 157.6 -0.5 -19.4 25 1 1 668 21 13 27 21 24 25 --- 12 10 02 69.8 164.9 -0.4 -13.1 658 F 1 710 21 13 45 21 26 25 3C274 12 12 02 69.9 166.3 -0.3 -11.9 113 1 1 710 21 26 25 21 37 23 --- 12 23 02 70.3 174.1 -0.1 -5.1 658 F 1 753 21 26 43 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 37 53 3C273 12 23 32 60.0 177.0 -0.1 -2.5 3 1 1 753 Stopped 21 42 52 --- 12 28 32 60.1 179.5 0.0 -0.4 299 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 43 22 3C273 12 29 02 60.1 179.8 0.0 -0.2 25 1 1 753 21 43 22 21 49 21 --- 12 35 02 60.0 182.8 0.1 2.4 359 F 1 776 21 43 40 21 51 21 3C274 12 37 02 70.4 184.3 0.1 3.7 93 1 1 776 21 51 21 22 02 19 --- 12 48 02 70.0 192.1 0.3 10.5 658 F 1 818 21 51 39 Schedule for VLBA_KP (Code Kp ) 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 ---------------------------------------------------------------------------------------- --- Thu 24 Aug 2006 Day 236 --- 22 02 49 3C274 12 48 32 70.0 192.5 0.3 10.8 25 1 1 818 22 02 49 22 13 47 --- 12 59 32 69.3 200.0 0.5 17.3 658 F 1 861 22 03 07 22 15 47 3C274 13 01 32 69.2 201.3 0.5 18.4 113 1 1 861 22 15 47 22 26 45 --- 13 12 32 68.2 208.2 0.7 24.2 658 F 1 903 22 16 05 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 27 15 3C273 13 13 02 58.3 201.1 0.7 17.8 4 1 1 903 Stopped 22 32 14 --- 13 18 02 57.9 203.3 0.8 19.7 299 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 32 44 3C273 13 18 32 57.9 203.6 0.8 19.8 25 1 1 903 22 32 44 22 38 43 --- 13 24 32 57.4 206.2 0.9 22.0 359 F 1 926 22 33 02 22 40 43 3C274 13 26 32 66.6 216.1 0.9 30.8 95 1 1 926 22 40 43 22 51 41 --- 13 37 32 65.2 221.6 1.1 35.2 658 F 1 969 22 41 01 22 52 11 3C274 13 38 02 65.1 221.9 1.1 35.4 25 1 1 969 22 52 11 23 03 09 --- 13 49 02 63.5 226.8 1.3 39.3 658 F 1 1011 22 52 29 23 05 09 3C274 13 51 02 63.2 227.6 1.3 39.9 113 1 1 1011 23 05 09 23 16 07 --- 14 02 02 61.4 231.9 1.5 43.2 658 F 1 1054 23 05 27 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 16 37 3C273 14 02 32 52.9 220.9 1.6 33.8 7 1 1 1054 Stopped 23 21 36 --- 14 07 32 52.2 222.6 1.6 35.1 299 S 1 1054 Schedule for VLBA_KP (Code Kp ) 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 ---------------------------------------------------------------------------------------- --- Thu 24 Aug 2006 Day 236 --- 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 22 06 3C273 14 08 02 52.1 222.7 1.6 35.2 25 1 1 1054 23 22 06 23 28 05 --- 14 14 02 51.2 224.7 1.7 36.7 359 F 1 1077 23 22 24 23 30 05 3C274 14 16 02 59.0 236.8 1.7 46.6 98 1 1 1077 23 30 05 23 41 03 --- 14 27 02 57.0 240.2 1.9 48.9 658 F 1 1119 23 30 23 23 41 33 3C274 14 27 32 56.9 240.4 1.9 49.0 25 1 1 1119 23 41 33 23 52 31 --- 14 38 32 54.8 243.4 2.1 51.0 658 F 1 1162 23 41 51 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: 14 Station: VLBA_KP 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: 6 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: 6 Station: VLBA_KP 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: 13 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 26.240492 0.30 1226+023 02 19 43.30565 * 02 03 08.59815 02 01 01.96093 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 08.838164 0.31 1228+126 12 40 01.74901 * 12 23 28.04383 12 21 23.38997 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 34.7 3C274 33.5 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