COVER INFORMATION Station: HART (Code Hh ) Experiment: Studying the feasibility of high-precision VLBI astrometry on M60 Exp. Code: RSY12 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Jun Yang Address: Onsala Space Observatory SE-439 92 Onsala Sweden Phone: +46 31 7725531 EMAIL: jun.yang@chalmers.se Fax: +46 31 7725590 Phone during observation: +46 31 7725531 Observing mode: 2048-16-2 Notes: 2048 Mbps, 16x32 MHz, RCP & LCP, 2 bit sampling Short phase-referencing observations at 5 GHz Schedule for HART (Code Hh ) Page 2 Studying the feasibility of high-precision VLBI astrometry on M60 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 ---------------------------------------------------------------------------------------- --- Tue 11 Mar 2025 Day 70 --- Next scan frequencies: 4830.49 4830.49 4830.49 4830.49 4894.49 4894.49 4894.49 4894.49 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 Next BBC frequencies: 230.49 230.49 230.49 230.49 294.49 294.49 294.49 294.49 358.49 358.49 358.49 358.49 422.49 422.49 422.49 422.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 20 30 00 J1250+1343 09 39 45 28.9 55.6 -3.2 0.0 0 0 20 30 00 20 33 30 =1247+139 09 43 15 29.5 54.9 -3.1 0.0 210 54 20 30 01 20 34 30 B1239+1110 09 44 16 33.1 55.6 -3.0 0.0 27 54 20 34 30 20 35 30 --- 09 45 16 33.3 55.4 -3.0 0.0 60 70 20 34 31 20 35 55 M60 09 45 41 32.6 55.1 -3.0 0.0 -1 70 20 35 55 20 37 55 --- 09 47 41 33.0 54.7 -3.0 0.0 119 100 20 35 56 20 38 20 J124353 09 48 06 33.0 54.6 -3.0 0.0 3 100 20 38 20 20 39 30 --- 09 49 16 33.2 54.4 -2.9 0.0 70 119 20 38 21 20 39 55 M60 09 49 41 33.4 54.3 -2.9 0.0 3 119 20 39 55 20 41 55 --- 09 51 42 33.7 54.0 -2.9 0.0 120 149 20 39 56 20 42 20 J124353 09 52 07 33.7 53.8 -2.9 0.0 3 149 20 42 20 20 43 30 --- 09 53 17 33.9 53.6 -2.9 0.0 70 167 20 42 21 20 43 55 M60 09 53 42 34.1 53.6 -2.9 0.0 3 167 20 43 55 20 45 55 --- 09 55 42 34.5 53.2 -2.8 0.0 120 198 20 43 56 20 46 20 J124353 09 56 07 34.4 53.0 -2.8 0.0 3 198 20 46 20 20 47 30 --- 09 57 18 34.6 52.8 -2.8 0.0 70 216 20 46 21 20 47 55 M60 09 57 43 34.8 52.7 -2.8 0.0 3 216 20 47 55 20 49 55 --- 09 59 43 35.2 52.3 -2.8 0.0 120 247 20 47 56 20 50 20 J124353 10 00 08 35.1 52.2 -2.8 0.0 3 247 20 50 20 20 51 30 --- 10 01 18 35.3 52.0 -2.7 0.0 70 265 20 50 21 20 51 55 M60 10 01 43 35.5 51.9 -2.7 0.0 3 265 20 51 55 20 53 55 --- 10 03 44 35.9 51.5 -2.7 0.0 120 296 20 51 56 20 54 20 J1241+1141 10 04 09 36.2 50.9 -2.6 0.0 0 296 20 54 20 20 55 30 --- 10 05 19 36.4 50.6 -2.6 0.0 70 314 20 54 21 20 55 55 M60 10 05 44 36.2 51.1 -2.7 0.0 0 314 20 55 55 20 57 55 --- 10 07 44 36.6 50.6 -2.6 0.0 120 345 20 55 56 Schedule for HART (Code Hh ) Page 3 Studying the feasibility of high-precision VLBI astrometry on M60 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 ---------------------------------------------------------------------------------------- --- Tue 11 Mar 2025 Day 70 --- 20 58 20 J124353 10 08 09 36.5 50.5 -2.6 0.0 3 345 20 58 20 20 59 30 --- 10 09 20 36.8 50.3 -2.6 0.0 70 363 20 58 21 20 59 55 M60 10 09 45 36.9 50.2 -2.6 0.0 3 363 20 59 55 21 01 55 --- 10 11 45 37.3 49.8 -2.6 0.0 120 394 20 59 56 21 02 20 J124353 10 12 10 37.2 49.7 -2.6 0.0 3 394 21 02 20 21 03 30 --- 10 13 20 37.4 49.4 -2.5 0.0 70 412 21 02 21 21 03 55 M60 10 13 45 37.6 49.3 -2.5 0.0 3 412 21 03 55 21 05 55 --- 10 15 46 38.0 48.9 -2.5 0.0 120 443 21 03 56 21 06 20 J124353 10 16 11 37.9 48.8 -2.5 0.0 3 443 21 06 20 21 07 30 --- 10 17 21 38.1 48.5 -2.5 0.0 70 461 21 06 21 21 07 55 M60 10 17 46 38.3 48.4 -2.5 0.0 3 461 21 07 55 21 09 55 --- 10 19 46 38.6 48.0 -2.4 0.0 120 492 21 07 56 21 10 20 J124353 10 20 11 38.6 47.9 -2.4 0.0 3 492 21 10 20 21 11 30 --- 10 21 22 38.8 47.6 -2.4 0.0 70 510 21 10 21 21 11 55 M60 10 21 47 39.0 47.5 -2.4 0.0 3 510 21 11 55 21 13 55 --- 10 23 47 39.3 47.0 -2.4 0.0 120 541 21 11 56 21 14 20 J1241+1141 10 24 12 39.6 46.4 -2.3 0.0 0 541 21 14 20 21 15 30 --- 10 25 22 39.8 46.1 -2.3 0.0 70 559 21 14 21 21 15 55 M60 10 25 47 39.6 46.6 -2.3 0.0 0 559 21 15 55 21 17 55 --- 10 27 48 40.0 46.1 -2.3 0.0 120 590 21 15 56 21 18 20 J124353 10 28 13 39.9 46.0 -2.3 0.0 3 590 21 18 20 21 19 30 --- 10 29 23 40.1 45.7 -2.3 0.0 70 608 21 18 21 21 19 55 M60 10 29 48 40.3 45.6 -2.3 0.0 3 608 21 19 55 21 21 55 --- 10 31 48 40.6 45.1 -2.2 0.0 120 639 21 19 56 21 22 20 J124353 10 32 13 40.6 45.0 -2.2 0.0 3 639 21 22 20 21 23 30 --- 10 33 24 40.7 44.7 -2.2 0.0 70 657 21 22 21 21 23 55 M60 10 33 49 40.9 44.6 -2.2 0.0 3 657 21 23 55 21 25 55 --- 10 35 49 41.2 44.1 -2.2 0.0 120 688 21 23 56 21 26 20 J124353 10 36 14 41.2 44.0 -2.1 0.0 3 688 21 26 20 21 27 30 --- 10 37 24 41.4 43.7 -2.1 0.0 70 706 21 26 21 Schedule for HART (Code Hh ) Page 4 Studying the feasibility of high-precision VLBI astrometry on M60 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 ---------------------------------------------------------------------------------------- --- Tue 11 Mar 2025 Day 70 --- 21 27 55 M60 10 37 49 41.5 43.6 -2.1 0.0 3 706 21 27 55 21 29 55 --- 10 39 50 41.9 43.1 -2.1 0.0 120 737 21 27 56 21 30 20 J124353 10 40 15 41.8 43.0 -2.1 0.0 3 737 21 30 20 21 31 30 --- 10 41 25 42.0 42.7 -2.1 0.0 70 755 21 30 21 21 31 55 M60 10 41 50 42.2 42.6 -2.1 0.0 3 755 21 31 55 21 33 55 --- 10 43 50 42.5 42.1 -2.0 0.0 120 786 21 31 56 21 34 20 J1241+1141 10 44 15 42.7 41.3 -2.0 0.0 0 786 21 34 20 21 35 30 --- 10 45 26 42.9 41.0 -2.0 0.0 70 804 21 34 21 21 35 55 M60 10 45 51 42.8 41.5 -2.0 0.0 0 804 21 35 55 21 37 55 --- 10 47 51 43.1 41.0 -2.0 0.0 120 835 21 35 56 21 38 20 J124353 10 48 16 43.0 40.9 -1.9 0.0 3 835 21 38 20 21 39 30 --- 10 49 26 43.2 40.6 -1.9 0.0 70 853 21 38 21 21 39 55 M60 10 49 51 43.4 40.5 -1.9 0.0 3 853 21 39 55 21 41 55 --- 10 51 52 43.6 39.9 -1.9 0.0 120 884 21 39 56 21 42 20 J124353 10 52 17 43.6 39.8 -1.9 0.0 3 884 21 42 20 21 43 30 --- 10 53 27 43.8 39.5 -1.9 0.0 70 902 21 42 21 21 43 55 M60 10 53 52 43.9 39.4 -1.9 0.0 3 902 21 43 55 21 45 55 --- 10 55 52 44.2 38.8 -1.8 0.0 120 933 21 43 56 21 46 20 J124353 10 56 17 44.2 38.7 -1.8 0.0 3 933 21 46 20 21 47 30 --- 10 57 28 44.3 38.4 -1.8 0.0 70 951 21 46 21 21 47 55 M60 10 57 53 44.5 38.2 -1.8 0.0 3 951 21 47 55 21 49 55 --- 10 59 53 44.8 37.7 -1.8 0.0 120 982 21 47 56 21 50 20 J124353 11 00 18 44.7 37.6 -1.7 0.0 3 982 21 50 20 21 51 30 --- 11 01 28 44.9 37.2 -1.7 0.0 70 1000 21 50 21 21 51 55 M60 11 01 53 45.1 37.1 -1.7 0.0 3 1000 21 51 55 21 53 55 --- 11 03 54 45.3 36.5 -1.7 0.0 120 1031 21 51 56 21 54 20 J1241+1141 11 04 19 45.5 35.7 -1.6 0.0 0 1031 21 54 20 21 55 30 --- 11 05 29 45.7 35.4 -1.6 0.0 70 1049 21 54 21 21 55 55 M60 11 05 54 45.6 35.9 -1.7 0.0 0 1049 21 55 55 21 57 55 --- 11 07 54 45.9 35.3 -1.6 0.0 120 1080 21 55 56 Schedule for HART (Code Hh ) Page 5 Studying the feasibility of high-precision VLBI astrometry on M60 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 ---------------------------------------------------------------------------------------- --- Tue 11 Mar 2025 Day 70 --- 21 58 20 J124353 11 08 19 45.8 35.2 -1.6 0.0 3 1080 21 58 20 21 59 30 --- 11 09 29 46.0 34.9 -1.6 0.0 70 1098 21 58 21 21 59 55 M60 11 09 55 46.1 34.7 -1.6 0.0 3 1098 21 59 55 22 01 55 --- 11 11 55 46.4 34.1 -1.6 0.0 120 1128 21 59 56 22 02 20 J124353 11 12 20 46.3 34.0 -1.5 0.0 3 1128 22 02 20 22 03 30 --- 11 13 30 46.5 33.6 -1.5 0.0 70 1146 22 02 21 22 03 55 M60 11 13 55 46.6 33.5 -1.5 0.0 3 1146 22 03 55 22 05 55 --- 11 15 56 46.9 32.9 -1.5 0.0 120 1177 22 03 56 22 06 20 J124353 11 16 21 46.8 32.8 -1.5 0.0 3 1177 22 06 20 22 07 30 --- 11 17 31 47.0 32.4 -1.5 0.0 70 1195 22 06 21 22 07 55 M60 11 17 56 47.1 32.3 -1.5 0.0 3 1195 22 07 55 22 09 55 --- 11 19 56 47.3 31.6 -1.4 0.0 120 1226 22 07 56 22 10 20 J124353 11 20 21 47.3 31.5 -1.4 0.0 3 1226 22 10 20 22 11 30 --- 11 21 31 47.4 31.1 -1.4 0.0 70 1244 22 10 21 22 11 55 M60 11 21 57 47.6 31.0 -1.4 0.0 3 1244 22 11 55 22 13 55 --- 11 23 57 47.8 30.3 -1.4 0.0 120 1275 22 11 56 22 14 20 J1241+1141 11 24 22 48.0 29.5 -1.3 0.0 0 1275 22 14 20 22 15 30 --- 11 25 32 48.1 29.1 -1.3 0.0 70 1293 22 14 21 22 15 55 M60 11 25 57 48.0 29.7 -1.3 0.0 0 1293 22 15 55 22 17 55 --- 11 27 57 48.3 29.0 -1.3 0.0 120 1324 22 15 56 22 18 20 J124353 11 28 23 48.2 28.9 -1.3 0.0 3 1324 22 18 20 22 19 30 --- 11 29 33 48.3 28.5 -1.3 0.0 70 1342 22 18 21 22 19 55 M60 11 29 58 48.5 28.4 -1.2 0.0 3 1342 22 19 55 22 21 55 --- 11 31 58 48.7 27.7 -1.2 0.0 120 1373 22 19 56 22 22 20 J124353 11 32 23 48.6 27.6 -1.2 0.0 3 1373 22 22 20 22 23 30 --- 11 33 33 48.7 27.2 -1.2 0.0 70 1391 22 22 21 22 23 55 M60 11 33 58 48.9 27.0 -1.2 0.0 3 1391 22 23 55 22 25 55 --- 11 35 59 49.1 26.3 -1.1 0.0 120 1422 22 23 56 22 26 20 J124353 11 36 24 49.0 26.2 -1.1 0.0 3 1422 22 26 20 22 27 30 --- 11 37 34 49.1 25.8 -1.1 0.0 70 1440 22 26 21 Schedule for HART (Code Hh ) Page 6 Studying the feasibility of high-precision VLBI astrometry on M60 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 ---------------------------------------------------------------------------------------- --- Tue 11 Mar 2025 Day 70 --- 22 27 55 M60 11 37 59 49.3 25.7 -1.1 0.0 3 1440 22 27 55 22 29 55 --- 11 39 59 49.5 25.0 -1.1 0.0 120 1471 22 27 56 22 30 20 J124353 11 40 25 49.4 24.8 -1.1 0.0 3 1471 22 30 20 22 31 30 --- 11 41 35 49.5 24.4 -1.1 0.0 70 1489 22 30 21 22 31 55 M60 11 42 00 49.7 24.3 -1.0 0.0 3 1489 22 31 55 22 33 55 --- 11 44 00 49.9 23.6 -1.0 0.0 120 1520 22 31 56 22 34 20 J1241+1141 11 44 25 49.9 22.6 -1.0 0.0 0 1520 22 34 20 22 35 30 --- 11 45 35 50.0 22.2 -1.0 0.0 70 1538 22 34 21 22 35 55 M60 11 46 00 50.0 22.8 -1.0 0.0 0 1538 22 35 55 22 37 55 --- 11 48 01 50.2 22.1 -0.9 0.0 120 1569 22 35 56 22 38 20 J124353 11 48 26 50.1 22.0 -0.9 0.0 3 1569 22 38 20 22 39 30 --- 11 49 36 50.2 21.6 -0.9 0.0 70 1587 22 38 21 22 39 55 M60 11 50 01 50.4 21.4 -0.9 0.0 3 1587 22 39 55 22 41 55 --- 11 52 01 50.5 20.7 -0.9 0.0 120 1618 22 39 56 22 42 20 J124353 11 52 27 50.5 20.6 -0.9 0.0 3 1618 22 42 20 22 43 30 --- 11 53 37 50.6 20.1 -0.9 0.0 70 1636 22 42 21 22 43 55 M60 11 54 02 50.7 19.9 -0.8 0.0 3 1636 22 43 55 22 45 55 --- 11 56 02 50.8 19.2 -0.8 0.0 120 1667 22 43 56 22 46 20 J124353 11 56 27 50.8 19.1 -0.8 0.0 3 1667 22 46 20 22 47 30 --- 11 57 37 50.9 18.7 -0.8 0.0 70 1685 22 46 21 22 47 55 M60 11 58 02 51.0 18.5 -0.8 0.0 3 1685 22 47 55 22 49 55 --- 12 00 03 51.1 17.7 -0.7 0.0 120 1716 22 47 56 22 50 20 J124353 12 00 28 51.1 17.6 -0.7 0.0 3 1716 22 50 20 22 51 30 --- 12 01 38 51.1 17.2 -0.7 0.0 70 1734 22 50 21 22 51 55 M60 12 02 03 51.3 17.0 -0.7 0.0 3 1734 22 51 55 22 53 55 --- 12 04 03 51.4 16.2 -0.7 0.0 120 1765 22 51 56 22 54 20 J1241+1141 12 04 28 51.4 15.2 -0.6 0.0 0 1765 22 54 20 22 55 30 --- 12 05 39 51.5 14.8 -0.6 0.0 70 1783 22 54 21 22 56 30 J1250+1343 12 06 39 49.0 16.9 -0.8 0.0 29 1783 22 56 30 23 00 00 =1247+139 12 10 09 49.2 15.6 -0.7 0.0 210 1837 22 56 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess125.C2048 Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat: hh6cm Values confirmed by E-mail Jonathan Quick 20140219 (CR) ****** Only 256.00 of 512.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. Setup group: 4 Station: HART Total bit rate: 2048 Format: VDIF Bits per sample: 2 Sample rate: 64.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 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 9 1 9 2 10 2 10 3 11 3 11 4 12 4 12 BBC SB= L L U U L L U U L L U U L L U U IF = A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 The following frequency sets based on these setups were used. Frequency Set: 9 Setup file default. Used with PCAL = off LO sum= 4830.49 4830.49 4830.49 4830.49 4894.49 4894.49 4894.49 4894.49 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 BBC fr= 230.49 230.49 230.49 230.49 294.49 294.49 294.49 294.49 358.49 358.49 358.49 358.49 422.49 422.49 422.49 422.49 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 9 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * M60 12 41 08.749622 * 12 43 39.971500 12 44 57.539389 0.00 11 49 34.61513 * 11 33 09.68800 11 24 42.47089 0.00 From catalog imbedded in main SCHED input file. * J124353 12 41 22.732369 * 12 43 53.920000 12 45 11.471242 0.00 11 55 02.09886 * 11 38 37.36000 11 30 10.22017 0.00 From catalog imbedded in main SCHED input file. * J1241+1141 12 39 08.335748 * 12 41 39.647000 12 42 57.264691 0.00 11 57 52.34245 * 11 41 25.84000 11 32 57.89411 0.00 From catalog imbedded in main SCHED input file. * B1239+1110 12 39 21.961908 * 12 41 53.428100 12 43 11.114991 0.00 11 10 35.84335 * 10 54 09.51200 10 45 41.71636 0.00 From catalog imbedded in main SCHED input file. 1247+139 12 47 57.966311 * 12 50 28.218043 12 51 45.309972 0.09 * J1250+1343 13 59 59.38502 * 13 43 40.38467 13 35 15.67349 0.20 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 81 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 M60 sess125.C2048 1 2 3 4 5 6 7 8 9 10 1.167 52.479 J124353 sess125.C2048 1 2 3 4 5 6 7 8 9 10 0.544 20.825 J1241+1141 sess125.C2048 2 3 4 5 6 7 8 9 10 0.136 4.874 B1239+1110 sess125.C2048 2 3 4 5 6 7 8 9 10 0.017 0.600 J1250+1343 sess125.C2048 1 2 3 4 5 6 7 8 9 10 0.117 5.250 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) M60 159.5 J124353 159.5 J1241+1141 159.9 B1239+1110 160.2 J1250+1343 157.2 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