  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: OH outburst in a proto-planetary nebula
 Exp. Code:  es057a  


Schedule Version:       1.00                                              
Processed by SCHED version:   6.04  March 2006                            

PI:       M. Szymczak                                                     

Address:  Torun Centre for Astronomy                                      
          ul. Gagarina 11, Torun, PL-87100                                
          Poland                                                          
                                                                          

Phone:    +48 56 6113029                                                  
EMAIL:    msz@astro.uni.torun.pl                                          
Fax:      +48 56 6113009                                                  
Phone during observation: +48 56 6113010                                  

Observing mode: VLBA/MKIV                                                 

Notes:    Please, make sure PHASE CAL is OFF.                             
          0.5MHz filters                                                  
                                                                          
                                                                          

Schedule for HART      (Code Hh )                                   Page   2
               OH outburst in a proto-planetary nebula
  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
----------------------------------------------------------------------------------------

 --- Tue   5 Jun 2007   Day 156 ---

 Next scan frequencies:  1611.79  1611.79  1611.79  1611.79
 Next BBC frequencies:    101.79   101.79   101.79   101.79
 Next scan bandwidths:      0.50     0.50     0.50     0.50

19 00 00  3C286        13 46 02  33.5 356.2  0.2       0.0     0   1  1      0  19 00 00
19 10 00  ---          13 56 04  33.3 353.7  0.4       0.0   600   F  1      2  19 00 04

19 12 00  3C286        13 58 04  33.3 353.2  0.4       0.0    95   1  1      2  19 12 00
19 22 00  ---          14 08 06  33.0 350.6  0.6       0.0   600   F  1      5  19 12 04

19 24 00  3C286        14 10 06  32.9 350.1  0.6       0.0    95   1  1      5  19 24 00
19 34 00  ---          14 20 08  32.5 347.6  0.8       0.0   600   F  1      7  19 24 04

19 34 00  3C345        14 20 08  16.3  27.9 -2.4       0.0  -123   1  1      7  19 34 00
19 44 00  ---          14 30 09  17.4  26.2 -2.2       0.0   477   F  1     10  19 34 04

19 44 00  3C345        14 30 09  17.4  26.2 -2.2       0.0   -20   1  1     10  19 44 00
19 48 00  ---          14 34 10  17.8  25.5 -2.2       0.0   220   F  1     11  19 44 04

19 48 00  3C286        14 34 10  31.7 344.1  1.0       0.0  -123   1  1     11  19 48 00
19 58 00  ---          14 44 12  31.0 341.7  1.2       0.0   477   F  1     13  19 48 04

20 00 00  3C286        14 46 12  30.9 341.2  1.2       0.0    95   1  1     13  20 00 00
20 10 00  ---          14 56 14  30.1 338.9  1.4       0.0   600   F  1     15  20 00 04

20 12 00  3C286        14 58 14  29.9 338.4  1.4       0.0    95   1  1     15  20 12 00
20 22 00  ---          15 08 16  29.1 336.2  1.6       0.0   600   F  1     18  20 12 04

20 22 00  3C345        15 08 16  20.7  19.3 -1.6       0.0  -123   1  1     18  20 22 00
20 32 00  ---          15 18 17  21.4  17.4 -1.4       0.0   477   F  1     20  20 22 04

20 32 00  3C345        15 18 17  21.4  17.4 -1.4       0.0   -20   1  1     20  20 32 00
20 36 00  ---          15 22 18  21.7  16.6 -1.3       0.0   220   F  1     21  20 32 04

20 36 00  3C286        15 22 18  27.7 333.1  1.8       0.0  -123   1  1     21  20 36 00
20 46 00  ---          15 32 20  26.7 331.0  2.0       0.0   477   F  1     24  20 36 04

20 48 00  3C286        15 34 20  26.4 330.6  2.0       0.0    95   1  1     24  20 48 00
20 58 00  ---          15 44 22  25.3 328.5  2.2       0.0   600   F  1     26  20 48 04

21 00 00  3C286        15 46 22  25.1 328.1  2.2       0.0    95   1  1     26  21 00 00
21 10 00  ---          15 56 24  23.8 326.2  2.4       0.0   600   F  1     29  21 00 04
Schedule for HART      (Code Hh )                                   Page   3
               OH outburst in a proto-planetary nebula
  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
----------------------------------------------------------------------------------------

 --- Tue   5 Jun 2007   Day 156 ---

21 10 00  3C345        15 56 24  23.4   9.8 -0.8       0.0  -123   1  1     29  21 10 00
21 20 00  ---          16 06 25  23.8   7.7 -0.6       0.0   477   F  1     31  21 10 04

21 20 00  3C345        16 06 25  23.8   7.7 -0.6       0.0   -20   1  1     31  21 20 00
21 24 00  ---          16 10 26  23.9   6.9 -0.5       0.0   220   F  1     32  21 20 04

21 25 30  OH17.7-2.0   16 11 56  55.6  77.5 -2.3       0.0   -46   1  1     32  21 25 30
21 35 30  ---          16 21 58  57.8  75.6 -2.1       0.0   554   F  1     34  21 25 34

21 37 00  OH17.7-2.0   16 23 28  58.1  75.3 -2.1       0.0    65   1  1     34  21 37 00
21 47 00  ---          16 33 30  60.3  73.2 -2.0       0.0   600   F  1     37  21 37 04

21 47 00  OH17.7-2.0   16 33 30  60.3  73.2 -2.0       0.0   -20   1  1     37  21 47 00
21 57 00  ---          16 43 31  62.4  70.8 -1.8       0.0   580   F  1     39  21 47 04

21 58 30  OH17.7-2.0   16 45 02  62.7  70.4 -1.8       0.0    65   1  1     39  21 58 30
22 06 30  ---          16 53 03  64.4  68.3 -1.6       0.0   480   F  1     41  21 58 34

22 08 00  J1733-1304   16 54 33  74.3  37.4 -0.6       0.0    33   1  1     41  22 08 00
22 14 00  =1730-130    17 00 34  75.0  32.7 -0.5       0.0   360   F  1     43  22 08 04

22 15 30  OH17.7-2.0   17 02 04  66.3  65.6 -1.5       0.0    35   1  1     43  22 15 30
22 25 30  ---          17 12 06  68.3  62.1 -1.3       0.0   600   F  1     45  22 15 34

22 27 00  OH17.7-2.0   17 13 36  68.6  61.5 -1.3       0.0    65   1  1     45  22 27 00
22 37 00  ---          17 23 38  70.5  57.3 -1.1       0.0   600   F  1     47  22 27 04

22 37 00  OH17.7-2.0   17 23 38  70.5  57.3 -1.1       0.0   -20   1  1     47  22 37 00
22 47 00  ---          17 33 39  72.4  52.4 -1.0       0.0   580   F  1     50  22 37 04

22 48 30  OH17.7-2.0   17 35 10  72.7  51.5 -0.9       0.0    65   1  1     50  22 48 30
22 56 30  ---          17 43 11  74.0  46.7 -0.8       0.0   480   F  1     52  22 48 34

22 58 00  J1733-1304   17 44 41  76.9 347.9  0.2       0.0    33   1  1     52  22 58 00
23 04 00  =1730-130    17 50 42  76.6 341.7  0.3       0.0   360   F  1     53  22 58 04

23 05 30  OH17.7-2.0   17 52 13  75.4  40.3 -0.6       0.0    35   1  1     53  23 05 30
23 15 30  ---          18 02 14  76.8  31.9 -0.5       0.0   600   F  1     56  23 05 34

23 17 00  OH17.7-2.0   18 03 44  76.9  30.5 -0.5       0.0    65   1  1     56  23 17 00
23 27 00  ---          18 13 46  77.9  20.3 -0.3       0.0   600   F  1     58  23 17 04

23 27 00  OH17.7-2.0   18 13 46  77.9  20.3 -0.3       0.0   -20   1  1     58  23 27 00
23 37 00  ---          18 23 48  78.5   8.7 -0.1       0.0   580   F  1     60  23 27 04
Schedule for HART      (Code Hh )                                   Page   4
               OH outburst in a proto-planetary nebula
  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
----------------------------------------------------------------------------------------

 --- Tue   5 Jun 2007   Day 156 ---

23 38 30  OH17.7-2.0   18 25 18  78.5   6.9 -0.1       0.0    65   1  1     60  23 38 30
23 46 30  ---          18 33 19  78.6 357.1  0.0       0.0   480   F  1     62  23 38 34

23 48 00  J1733-1304   18 34 50  70.7 308.7  1.0       0.0    33   1  1     62  23 48 00
23 54 00  =1730-130    18 40 50  69.6 305.8  1.1       0.0   360   F  1     64  23 48 04

 --- Start: Tue   5 Jun 2007   Day 156 -- Stop: Wed   6 Jun 2007   Day 157 ---

23 55 30  OH17.7-2.0   18 42 21  78.3 346.3  0.2       0.0    35   1  1     64  23 55 30
00 05 30  ---          18 52 22  77.5 335.3  0.4       0.0   600   F  1     66  23 55 34

00 07 00  OH17.7-2.0   18 53 53  77.4 333.7  0.4       0.0    65   1  1     66  00 07 00
00 17 00  ---          19 03 54  76.2 324.4  0.5       0.0   600   F  1     69  00 07 04

00 17 00  OH17.7-2.0   19 03 54  76.2 324.4  0.5       0.0   -20   1  1     69  00 17 00
00 27 00  ---          19 13 56  74.8 316.5  0.7       0.0   580   F  1     71  00 17 04

00 28 30  OH17.7-2.0   19 15 26  74.6 315.5  0.7       0.0    65   1  1     71  00 28 30
00 36 30  ---          19 23 27  73.2 310.4  0.9       0.0   480   F  1     73  00 28 34

00 38 00  J1733-1304   19 24 58  60.9 290.7  1.9       0.0    33   1  1     73  00 38 00
00 44 00  =1730-130    19 30 59  59.6 289.3  2.0       0.0   360   F  1     75  00 38 04

00 45 30  OH17.7-2.0   19 32 29  71.6 305.4  1.0       0.0    35   1  1     75  00 45 30
00 55 30  ---          19 42 31  69.7 300.8  1.2       0.0   600   F  1     77  00 45 34

00 57 00  OH17.7-2.0   19 44 01  69.4 300.2  1.2       0.0    65   1  1     77  00 57 00
01 07 00  ---          19 54 02  67.5 296.4  1.4       0.0   600   F  1     79  00 57 04

01 07 00  OH17.7-2.0   19 54 02  67.5 296.4  1.4       0.0   -20   1  1     79  01 07 00
01 17 00  ---          20 04 04  65.4 293.1  1.6       0.0   580   F  1     82  01 07 04

01 18 30  OH17.7-2.0   20 05 34  65.1 292.7  1.6       0.0    65   1  1     82  01 18 30
01 26 30  ---          20 13 36  63.4 290.4  1.7       0.0   480   F  1     84  01 18 34

01 28 00  J1733-1304   20 15 06  50.0 280.8  2.7       0.0    33   1  1     84  01 28 00
01 34 00  =1730-130    20 21 07  48.7 279.8  2.8       0.0   360   F  1     85  01 28 04

01 35 30  OH17.7-2.0   20 22 37  61.5 288.2  1.9       0.0    35   1  1     85  01 35 30
01 45 30  ---          20 32 39  59.4 285.9  2.0       0.0   600   F  1     88  01 35 34

01 47 00  OH17.7-2.0   20 34 09  59.0 285.6  2.1       0.0    65   1  1     88  01 47 00
01 57 00  ---          20 44 11  56.8 283.6  2.2       0.0   600   F  1     90  01 47 04
Schedule for HART      (Code Hh )                                   Page   5
               OH outburst in a proto-planetary nebula
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

01 57 00  OH17.7-2.0   20 44 11  56.8 283.6  2.2       0.0   -20   1  1     90  01 57 00
02 07 00  ---          20 54 12  54.6 281.8  2.4       0.0   580   F  1     92  01 57 04

02 08 30  OH17.7-2.0   20 55 43  54.3 281.5  2.4       0.0    65   1  1     92  02 08 30
02 16 30  ---          21 03 44  52.5 280.2  2.5       0.0   480   F  1     94  02 08 34

02 18 00  J1733-1304   21 05 14  38.8 273.9  3.5       0.0    33   1  1     94  02 18 00
02 24 00  =1730-130    21 11 15  37.5 273.2  3.6       0.0   360   F  1     96  02 18 04

02 25 30  OH17.7-2.0   21 12 45  50.5 278.8  2.7       0.0    35   1  1     96  02 25 30
02 35 30  ---          21 22 47  48.3 277.3  2.9       0.0   600   F  1     98  02 25 34

02 37 00  OH17.7-2.0   21 24 17  48.0 277.1  2.9       0.0    65   1  1     98  02 37 00
02 47 00  ---          21 34 19  45.7 275.7  3.1       0.0   600   F  1    101  02 37 04

02 47 00  OH17.7-2.0   21 34 19  45.7 275.7  3.1       0.0   -20   1  1    101  02 47 00
02 57 00  ---          21 44 21  43.5 274.4  3.2       0.0   580   F  1    103  02 47 04

02 58 30  OH17.7-2.0   21 45 51  43.1 274.2  3.2       0.0    65   1  1    103  02 58 30
03 06 30  ---          21 53 52  41.3 273.3  3.4       0.0   480   F  1    105  02 58 34

03 08 00  J1733-1304   21 55 22  27.6 268.2  4.4       0.0    33   1  1    105  03 08 00
03 14 00  =1730-130    22 01 23  26.2 267.6  4.5       0.0   360   F  1    106  03 08 04

03 15 30  OH17.7-2.0   22 02 54  39.3 272.2  3.5       0.0    35   1  1    106  03 15 30
03 25 30  ---          22 12 55  37.1 271.0  3.7       0.0   600   F  1    109  03 15 34

03 27 00  OH17.7-2.0   22 14 25  36.7 270.9  3.7       0.0    65   1  1    109  03 27 00
03 37 00  ---          22 24 27  34.5 269.8  3.9       0.0   600   F  1    111  03 27 04

03 37 00  OH17.7-2.0   22 24 27  34.5 269.8  3.9       0.0   -20   1  1    111  03 37 00
03 47 00  ---          22 34 29  32.2 268.7  4.1       0.0   580   F  1    114  03 37 04

03 48 30  OH17.7-2.0   22 35 59  31.9 268.5  4.1       0.0    65   1  1    114  03 48 30
03 56 30  ---          22 44 00  30.1 267.7  4.2       0.0   480   F  1    116  03 48 34

03 58 00  J1733-1304   22 45 31  16.3 263.1  5.2       0.0    33   1  1    116  03 58 00
04 04 00  =1730-130    22 51 32  15.0 262.5  5.3       0.0   360   F  1    117  03 58 04

04 05 30  OH17.7-2.0   22 53 02  28.0 266.8  4.4       0.0    35   1  1    117  04 05 30
04 15 30  ---          23 03 03  25.8 265.8  4.5       0.0   600   F  1    120  04 05 34

04 17 00  OH17.7-2.0   23 04 34  25.5 265.6  4.6       0.0    65   1  1    120  04 17 00
04 27 00  ---          23 14 35  23.2 264.6  4.7       0.0   600   F  1    122  04 17 04
Schedule for HART      (Code Hh )                                   Page   6
               OH outburst in a proto-planetary nebula
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

04 27 00  OH17.7-2.0   23 14 35  23.2 264.6  4.7       0.0   -20   1  1    122  04 27 00
04 37 00  ---          23 24 37  21.0 263.6  4.9       0.0   580   F  1    124  04 27 04

04 38 30  OH17.7-2.0   23 26 07  20.6 263.4  4.9       0.0    65   1  1    124  04 38 30
04 46 30  ---          23 34 09  18.8 262.6  5.1       0.0   480   F  1    126  04 38 34

04 48 30  J2253+1608   23 36 09  46.7 345.3  0.7       0.0   -38   1  1    126  04 48 30
04 58 30  =2251+158    23 46 11  46.1 341.9  0.9       0.0   562   F  1    129  04 48 34

04 58 30  J2253+1608   23 46 11  46.1 341.9  0.9       0.0   -20   1  1    129  04 58 30
05 12 30  =2251+158    00 00 13  45.0 337.4  1.1       0.0   820   F  1    132  04 58 34

05 14 30  J2253+1608   00 02 13  44.8 336.7  1.1       0.0    95   1  1    132  05 14 30
05 29 30  =2251+158    00 17 16  43.3 332.1  1.4       0.0   900   F  1    136  05 14 34

05 31 30  J2253+1608   00 19 16  43.1 331.5  1.4       0.0    95   1  1    136  05 31 30
05 46 30  =2251+158    00 34 18  41.4 327.3  1.7       0.0   900   F  1    139  05 31 34

05 48 30  J2253+1608   00 36 19  41.2 326.7  1.7       0.0    95   1  1    139  05 48 30
05 58 30  =2251+158    00 46 20  39.9 324.0  1.9       0.0   600   F  1    142  05 48 34


SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


 Setup file: es057.set
   Matches group hh18cm in /usr/local/sched/catalogs/freq.dat
    Values confirmed by E-mail Jonathan Quick 291100 (CR)

   Setup group:    7         Station: HART              Total bit rate:   32
   Format: MKIV1:1           Bits per sample: 2         Sample rate:  4.000
   Number of channels:  4                               Speedup factor:   2.00

   Disk used to record data.

   1st LO=   1510.00   1510.00   1510.00   1510.00
   Net SB=         U         U         U         U
   Pol.  =      LCP       RCP       LCP       RCP 
   BBC   =         1         2         3         4
   BBC SB=         U         U         U         U
   IF    =        1N        2N        1N        2N

  The following frequency sets based on this setup were used.

  Frequency Set:   7  Based on FREQ, BW, and/or DOPPLER in schedule.  No pcal detection.
   LO sum=    1611.79   1611.79   1611.79   1611.79
   BBC fr=     101.79    101.79    101.79    101.79
   Bandwd=      0.500     0.500     0.500     0.500

   Track assignments are: 
    track1=   2,  6, 10, 14
    barrel=roll_off 
 SOURCE LIST -- OH outburst in a proto-planetary nebula
     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)

 * OH17.7-2.0        18 27 39.767201   * 18 30 30.695000     18 30 57.703990       0.00
                    -14 31 03.68772    *-14 28 56.82000     -14 28 44.96006        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         61.60    61.60    61.60    61.60
                        5.700 scan hours,    149.283 baseline hours above horizon.

   J1331+3030        13 28 49.657756   * 13 31 08.288048     13 31 30.366413       0.37
   1328+307          30 45 58.64060    * 30 30 32.95924      30 28 17.00085        0.47
 * 3C286             /usr/local/sched/catalogs/sources.vlba
   J1331+30          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        1.500 scan hours,     38.381 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 15.921781       0.26
   1641+399          39 54 10.81494    * 39 48 36.99400      39 47 39.01090        0.40
 * 3C345             /usr/local/sched/catalogs/sources.vlba
   J1642+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.700 scan hours,     13.751 baseline hours above horizon.

 * J1733-1304        17 30 13.535187   * 17 33 02.705785     17 33 29.510354       0.21
   1730-130         -13 02 45.83975    *-13 04 49.54823     -13 05 16.71233        0.30
   J1733-13          /usr/local/sched/catalogs/sources.vlba
   NRAO530           VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.900 scan hours,     20.600 baseline hours above horizon.

 * J2253+1608        22 51 29.519744   * 22 53 57.747943     22 54 19.955266       0.31
   2251+158          15 52 54.34806    * 16 08 53.56089      16 11 08.19784        0.20
   3C454.3           /usr/local/sched/catalogs/sources.vlba
   J2253+16          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        1.067 scan hours,     29.119 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) 
   OH17.7-2.0         155.8
   3C286              107.9
   3C345              117.6
   J1733-1304         166.8
   J2253+1608          83.9

  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 

