  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 6cm global VLBI observations of Arp220
 Exp. Code:  GV022B  


Schedule Version:       3.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       Eskil Varenius

Address:  Department of Earth and Space Sciences, Chalmers University of T
          Onsala Space Observatory
          439 92 Onsala
          Sweden

Phone:    +46 31 772 55 45
EMAIL:    varenius@chalmers.se
Fax:      +46(0)31 772 5590
Phone during observation: +46 31 772 55 45

Observing mode: 6cm 2Gbps global VLBI with phased C-array VLA

Notes:    Phase calibrator: J1532+2344
          Fringe finder / pol. cal / bandpass cal: J1516+1932
          VLA phase-up calibrator: J1516+1932
 

Schedule for HART      (Code Hh )                                   Page   2
               6cm global VLBI observations of Arp220
  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
----------------------------------------------------------------------------------------

 --- Wed   7 Jun 2017   Day 158 ---

 ---------- pre-VLA block ----------

 Next scan frequencies:  4772.25  4772.25  4772.25  4772.25  4836.25  4836.25  4836.25  4836.25
                         4900.25  4900.25  4900.25  4900.25  4964.25  4964.25  4964.25  4964.25
 Next BBC frequencies:    172.25   172.25   172.25   172.25   236.25   236.25   236.25   236.25
                          300.25   300.25   300.25   300.25   364.25   364.25   364.25   364.25
 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

21 00 00  J1516+1932   15 56 32  43.7 347.3  0.6       0.0     0        0   21 00 00
21 03 00  =1514+197    15 59 32  43.5 346.4  0.7       0.0   180       46   21 00 01

21 04 01  J1532+2344   16 00 34  40.0 351.9  0.5       0.0    26       46   21 04 01
21 05 31  =1530+239    16 02 14  39.9 351.4  0.5       0.0    90       70   21 04 02

21 05 57  ARP220       16 02 29  40.2 351.9  0.4       0.0     0       70   21 05 57
21 10 27  ---          16 07 00  40.1 350.6  0.5       0.0   270      139   21 05 58

21 11 02  J1532+2344   16 07 36  39.8 349.8  0.6       0.0    10      139   21 11 02
21 12 32  =1530+239    16 09 16  39.7 349.4  0.6       0.0    90      162   21 11 03

21 12 58  ARP220       16 09 32  40.0 349.9  0.6       0.0     0      162   21 12 58
21 17 28  ---          16 14 03  39.8 348.5  0.6       0.0   270      232   21 12 59

21 18 04  J1532+2344   16 14 38  39.4 347.8  0.7       0.0    10      232   21 18 04
21 19 34  =1530+239    16 16 19  39.4 347.3  0.7       0.0    90      255   21 18 05

21 19 59  ARP220       16 16 34  39.7 347.8  0.7       0.0     0      255   21 19 59
21 24 29  ---          16 21 05  39.5 346.5  0.8       0.0   270      325   21 20 00

21 25 05  J1532+2344   16 21 41  39.1 345.8  0.8       0.0    10      325   21 25 05
21 26 35  =1530+239    16 23 21  39.0 345.3  0.8       0.0    90      348   21 25 06

21 27 01  ARP220       16 23 37  39.3 345.8  0.8       0.0     0      348   21 27 01
21 31 31  ---          16 28 08  39.1 344.5  0.9       0.0   270      417   21 27 02

21 32 06  J1532+2344   16 28 43  38.7 343.8  0.9       0.0    10      417   21 32 06
21 33 36  =1530+239    16 30 24  38.6 343.3  0.9       0.0    90      441   21 32 07

21 34 02  ARP220       16 30 39  38.9 343.7  0.9       0.0     0      441   21 34 02
21 38 32  ---          16 35 10  38.6 342.5  1.0       0.0   270      510   21 34 03

21 39 08  J1532+2344   16 35 46  38.2 341.8  1.0       0.0    10      510   21 39 08
21 40 38  =1530+239    16 37 26  38.1 341.3  1.1       0.0    90      533   21 39 09
Schedule for HART      (Code Hh )                                   Page   3
               6cm global VLBI observations of Arp220
  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
----------------------------------------------------------------------------------------

 --- Wed   7 Jun 2017   Day 158 ---

21 41 03  ARP220       16 37 42  38.4 341.8  1.0       0.0     0      533   21 41 03
21 45 33  ---          16 42 12  38.1 340.5  1.1       0.0   270      603   21 41 04

21 46 09  J1532+2344   16 42 48  37.7 339.9  1.2       0.0    10      603   21 46 09
21 47 39  =1530+239    16 44 29  37.5 339.4  1.2       0.0    90      626   21 46 10

21 48 05  ARP220       16 44 44  37.9 339.8  1.2       0.0     0      626   21 48 05
21 52 35  ---          16 49 15  37.6 338.6  1.2       0.0   270      696   21 48 06

 ---------- 2nd rpt7 (6+1) + rpt5 (1+2+2) ----------

21 53 36  J1516+1932   16 50 16  39.4 331.4  1.5       0.0    25      696   21 53 36
21 56 26  =1514+197    16 53 17  39.0 330.6  1.6       0.0   170      739   21 53 37

21 57 23  J1532+2344   16 54 04  36.7 336.8  1.3       0.0    21      739   21 57 23
21 58 53  =1530+239    16 55 44  36.6 336.4  1.4       0.0    90      763   21 57 24

21 59 18  ARP220       16 56 00  37.0 336.8  1.3       0.0     0      763   21 59 18
22 03 18  ---          17 00 00  36.6 335.7  1.4       0.0   240      824   21 59 19

22 03 54  J1532+2344   17 00 36  36.1 335.1  1.5       0.0    10      824   22 03 54
22 05 24  =1530+239    17 02 17  36.0 334.7  1.5       0.0    90      848   22 03 55

22 05 50  ARP220       17 02 32  36.4 335.1  1.4       0.0     0      848   22 05 50
22 09 50  ---          17 06 33  36.0 334.0  1.5       0.0   240      909   22 05 51

22 10 25  J1532+2344   17 07 09  35.5 333.5  1.6       0.0    10      909   22 10 25
22 11 55  =1530+239    17 08 49  35.3 333.0  1.6       0.0    90      933   22 10 26

22 12 21  ARP220       17 09 05  35.7 333.4  1.6       0.0     0      933   22 12 21
22 16 21  ---          17 13 05  35.3 332.4  1.6       0.0   240      994   22 12 22

22 16 57  J1532+2344   17 13 41  34.8 331.8  1.7       0.0    10      994   22 16 57
22 18 27  =1530+239    17 15 21  34.6 331.4  1.7       0.0    90     1018   22 16 58

22 18 52  ARP220       17 15 37  35.1 331.8  1.7       0.0     0     1018   22 18 52
22 22 52  ---          17 19 38  34.6 330.8  1.7       0.0   240     1080   22 18 53

22 23 28  J1532+2344   17 20 13  34.1 330.2  1.8       0.0    10     1080   22 23 28
22 24 58  =1530+239    17 21 54  33.9 329.8  1.8       0.0    90     1103   22 23 29

22 25 23  ARP220       17 22 09  34.3 330.2  1.8       0.0     0     1103   22 25 23
22 29 23  ---          17 26 10  33.9 329.2  1.8       0.0   240     1165   22 25 24
Schedule for HART      (Code Hh )                                   Page   4
               6cm global VLBI observations of Arp220
  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
----------------------------------------------------------------------------------------

 --- Wed   7 Jun 2017   Day 158 ---

22 29 59  J1532+2344   17 26 46  33.4 328.7  1.9       0.0    10     1165   22 29 59
22 31 29  =1530+239    17 28 26  33.2 328.3  1.9       0.0    90     1188   22 30 00

22 31 55  ARP220       17 28 42  33.6 328.6  1.9       0.0     0     1188   22 31 55
22 35 55  ---          17 32 42  33.1 327.6  1.9       0.0   240     1250   22 31 56

22 36 30  J1532+2344   17 33 18  32.6 327.1  2.0       0.0    10     1250   22 36 30
22 38 00  =1530+239    17 34 58  32.4 326.8  2.0       0.0    90     1273   22 36 31

22 38 26  ARP220       17 35 14  32.8 327.1  2.0       0.0     0     1273   22 38 26
22 42 26  ---          17 39 15  32.3 326.1  2.1       0.0   240     1335   22 38 27

22 43 02  J1532+2344   17 39 50  31.8 325.7  2.1       0.0    10     1335   22 43 02
22 44 32  =1530+239    17 41 31  31.6 325.3  2.1       0.0    90     1358   22 43 03

22 44 57  ARP220       17 41 46  32.0 325.6  2.1       0.0     0     1358   22 44 57
22 48 57  ---          17 45 47  31.5 324.7  2.2       0.0   240     1420   22 44 58

22 49 33  J1532+2344   17 46 23  30.9 324.2  2.2       0.0    10     1420   22 49 33
22 51 03  =1530+239    17 48 03  30.7 323.9  2.2       0.0    90     1443   22 49 34

22 51 29  ARP220       17 48 19  31.1 324.1  2.2       0.0     0     1443   22 51 29
22 55 29  ---          17 52 19  30.6 323.2  2.3       0.0   240     1505   22 51 30

22 56 04  J1532+2344   17 52 55  30.1 322.8  2.3       0.0    10     1505   22 56 04
22 57 34  =1530+239    17 54 35  29.8 322.5  2.4       0.0    90     1528   22 56 05

22 58 00  ARP220       17 54 51  30.3 322.7  2.3       0.0     0     1528   22 58 00
23 02 00  ---          17 58 52  29.7 321.9  2.4       0.0   240     1590   22 58 01

23 02 36  J1532+2344   17 59 28  29.2 321.4  2.4       0.0    10     1590   23 02 36
23 04 06  =1530+239    18 01 08  28.9 321.1  2.5       0.0    90     1613   23 02 37

23 04 31  ARP220       18 01 23  29.4 321.3  2.4       0.0     0     1613   23 04 31
23 08 31  ---          18 05 24  28.8 320.5  2.5       0.0   240     1675   23 04 32

23 09 07  J1532+2344   18 06 00  28.2 320.1  2.5       0.0    10     1675   23 09 07
23 10 37  =1530+239    18 07 40  28.0 319.8  2.6       0.0    90     1698   23 09 08

23 11 03  ARP220       18 07 56  28.4 320.0  2.5       0.0     0     1698   23 11 03
23 15 03  ---          18 11 57  27.9 319.2  2.6       0.0   240     1760   23 11 04
Schedule for HART      (Code Hh )                                   Page   5
               6cm global VLBI observations of Arp220
  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
----------------------------------------------------------------------------------------

 --- Wed   7 Jun 2017   Day 158 ---

 ---------- 1st post-VLA block (no Yy) ----------

23 15 56  J1516+1932   18 12 50  27.8 312.5  2.9       0.0    17     1760   23 15 56
23 18 46  =1514+197    18 15 50  27.3 311.9  3.0       0.0   170     1803   23 15 57

23 19 38  J1532+2344   18 16 33  26.7 318.0  2.7       0.0    17     1803   23 19 38
23 21 08  =1530+239    18 18 13  26.4 317.7  2.7       0.0    90     1827   23 19 39

23 21 34  ARP220       18 18 29  26.9 317.9  2.7       0.0     0     1827   23 21 34
23 25 34  ---          18 22 30  26.3 317.1  2.8       0.0   240     1888   23 21 35

23 26 10  J1532+2344   18 23 05  25.7 316.8  2.8       0.0    10     1888   23 26 10
23 27 40  =1530+239    18 24 46  25.4 316.5  2.9       0.0    90     1912   23 26 11

23 28 05  ARP220       18 25 01  25.9 316.6  2.8       0.0     0     1912   23 28 05
23 32 05  ---          18 29 02  25.3 315.9  2.9       0.0   240     1974   23 28 06

 ---------- 2nd post-VLA block ----------

23 32 41  J1532+2344   18 29 38  24.6 315.6  2.9       0.0    10     1974   23 32 41
23 34 11  =1530+239    18 31 18  24.4 315.2  3.0       0.0    90     1997   23 32 42

23 34 37  ARP220       18 31 34  24.9 315.4  2.9       0.0     0     1997   23 34 37
23 38 37  ---          18 35 34  24.2 314.7  3.0       0.0   240     2059   23 34 38

23 39 12  J1532+2344   18 36 10  23.6 314.4  3.0       0.0    10     2059   23 39 12
23 40 32  =1530+239    18 37 40  23.4 314.1  3.1       0.0    80     2079   23 39 13

23 40 58  ARP220       18 37 56  23.8 314.3  3.0       0.0     0     2079   23 40 58
23 44 58  ---          18 41 57  23.2 313.6  3.1       0.0   240     2141   23 40 59

23 45 34  J1532+2344   18 42 33  22.6 313.3  3.2       0.0    10     2141   23 45 34
23 46 54  =1530+239    18 44 03  22.3 313.0  3.2       0.0    80     2162   23 45 35

23 47 19  ARP220       18 44 18  22.8 313.1  3.1       0.0     0     2162   23 47 19
23 51 19  ---          18 48 19  22.1 312.5  3.2       0.0   240     2223   23 47 20

23 52 13  J1516+1932   18 49 13  21.5 306.1  3.5       0.0    18     2223   23 52 13
23 53 13  =1514+197    18 50 24  21.3 305.9  3.5       0.0    60     2239   23 52 14

23 53 45  J1516+1932   18 50 45  21.2 305.9  3.6       0.0    10     2239   23 53 45
23 55 35  =1514+197    18 52 45  20.8 305.6  3.6       0.0   110     2267   23 53 46

23 56 28  J1532+2344   18 53 29  20.8 311.4  3.3       0.0    18     2267   23 56 28
23 57 58  =1530+239    18 55 09  20.5 311.1  3.4       0.0    90     2290   23 56 29
Schedule for HART      (Code Hh )                                   Page   6
               6cm global VLBI observations of Arp220
  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
----------------------------------------------------------------------------------------

 --- Start: Wed   7 Jun 2017   Day 158 -- Stop: Thu   8 Jun 2017   Day 159 ---

23 58 24  ARP220       18 55 25  21.0 311.3  3.3       0.0     0     2290   23 58 24
00 02 24  ---          18 59 25  20.3 310.6  3.4       0.0   240     2352   23 58 25

00 02 59  J1532+2344   19 00 01  19.6 310.3  3.4       0.0    10     2352   00 02 59
00 04 29  =1530+239    19 01 41  19.4 310.1  3.5       0.0    90     2375   00 03 00

00 04 55  ARP220       19 01 57  19.8 310.2  3.4       0.0     0     2375   00 04 55
00 08 55  ---          19 05 58  19.1 309.5  3.5       0.0   240     2437   00 04 56

00 09 31  J1532+2344   19 06 34  18.5 309.3  3.6       0.0    10     2437   00 09 31
00 11 01  =1530+239    19 08 14  18.2 309.0  3.6       0.0    90     2460   00 09 32

00 11 26  ARP220       19 08 29  18.7 309.1  3.5       0.0     0     2460   00 11 26
00 15 26  ---          19 12 30  18.0 308.5  3.6       0.0   240     2522   00 11 27

00 16 02  J1532+2344   19 13 06  17.4 308.3  3.7       0.0    10     2522   00 16 02
00 17 32  =1530+239    19 14 46  17.1 308.0  3.7       0.0    90     2545   00 16 03

00 17 58  ARP220       19 15 02  17.6 308.1  3.7       0.0     0     2545   00 17 58
00 21 58  ---          19 19 02  16.8 307.5  3.7       0.0   240     2607   00 17 59

00 22 33  J1532+2344   19 19 38  16.2 307.3  3.8       0.0    10     2607   00 22 33
00 24 03  =1530+239    19 21 19  15.9 307.0  3.8       0.0    90     2630   00 22 34

00 24 29  ARP220       19 21 34  16.4 307.1  3.8       0.0     0     2630   00 24 29
00 28 29  ---          19 25 35  15.7 306.6  3.8       0.0   240     2692   00 24 30

00 29 23  J1516+1932   19 26 30  14.5 300.5  4.1       0.0    18     2692   00 29 23
00 30 23  =1514+197    19 27 40  14.3 300.4  4.2       0.0    60     2708   00 29 24

00 30 55  J1516+1932   19 28 01  14.2 300.3  4.2       0.0    10     2708   00 30 55
00 32 45  =1514+197    19 30 02  13.8 300.1  4.2       0.0   110     2736   00 30 56

00 33 38  J1532+2344   19 30 45  14.2 305.7  4.0       0.0    18     2736   00 33 38
00 34 58  =1530+239    19 32 15  13.9 305.5  4.0       0.0    80     2757   00 33 39

00 35 24  ARP220       19 32 31  14.4 305.5  3.9       0.0     0     2757   00 35 24
00 39 24  ---          19 36 32  13.7 305.0  4.0       0.0   240     2819   00 35 25

00 40 00  J1532+2344   19 37 08  13.0 304.8  4.1       0.0    10     2819   00 40 00
00 41 20  =1530+239    19 38 38  12.7 304.6  4.1       0.0    80     2839   00 40 01

00 41 45  ARP220       19 38 53  13.2 304.7  4.1       0.0     0     2839   00 41 45
00 45 45  ---          19 42 54  12.5 304.1  4.1       0.0   240     2901   00 41 46
Schedule for HART      (Code Hh )                                   Page   7
               6cm global VLBI observations of Arp220
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2017   Day 159 ---

00 46 21  J1532+2344   19 43 30  11.8 303.9  4.2       0.0    10     2901   00 46 21
00 47 51  =1530+239    19 45 10  11.5 303.7  4.2       0.0    90     2924   00 46 22

00 48 17  ARP220       19 45 26  12.0 303.8  4.2       0.0     0     2924   00 48 17
00 52 17  ---          19 49 27  11.3 303.2  4.2       0.0   240     2986   00 48 18

00 52 52  J1532+2344   19 50 02  10.6 303.0  4.3       0.0    10     2986   00 52 52
00 54 22  =1530+239    19 51 43  10.3 302.8  4.3       0.0    90     3009   00 52 53

00 54 48  ARP220       19 51 58  10.8 302.9  4.3       0.0     0     3009   00 54 48
00 58 48  ---          19 55 59  10.0 302.3  4.3       0.0   240     3071   00 54 49

00 59 24  J1532+2344   19 56 35   9.4 302.2  4.4       0.0    10     3071   00 59 24
01 00 54  =1530+239    19 58 15   9.1 302.0  4.4       0.0    90     3094   00 59 25

01 01 15  ARP220       19 58 26   9.6 302.0  4.4       0.0    -4     3094   01 01 15
01 05 15  ---          20 02 27   8.8 301.5  4.4  H    0.0     0     3156   01 01 16


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


 ======== Setup file: sess217.C2048glob
   Matching groups in /home/guest/rmc/SCHED/sched11.4/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:   18         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         3        11         3        11
                   5        13         5        13         7        15         7        15
   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
                  B2        C1        B2        C1        B2        C1        B2        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  13  Setup file default.  Used with PCAL = off
   LO sum=   4772.25  4772.25  4772.25  4772.25  4836.25  4836.25  4836.25  4836.25
             4900.25  4900.25  4900.25  4900.25  4964.25  4964.25  4964.25  4964.25
   BBC fr=    172.25   172.25   172.25   172.25   236.25   236.25   236.25   236.25
              300.25   300.25   300.25   300.25   364.25   364.25   364.25   364.25
   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:  13

   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)

 * ARP220            15 32 46.905485   * 15 34 57.250000     15 35 43.359734       0.00
                     23 40 07.75728    * 23 30 11.33000      23 26 55.86293        0.00
                     From catalog imbedded in main SCHED input file.
                     Pos. from Batejat. et al 2011

 * 3C286             13 28 49.657758   * 13 31 08.288051     13 31 56.602521       0.18
   J1331+3030        30 45 58.64059    * 30 30 32.95924      30 25 24.79116        0.17
   1328+307          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1331+30          GSFC 2015a astro solution, unpublished    225 observations.

   1514+197          15 14 40.985840   * 15 16 56.796162     15 17 44.720916       0.01
 * J1516+1932        19 43 10.94252    * 19 32 12.99209      19 28 35.77580        0.02
   J1516+19          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished   2699 observations.

   1530+239          15 30 36.092767   * 15 32 46.345222     15 33 32.415948       0.10
 * J1532+2344        23 54 09.32921    * 23 44 05.26804      23 40 47.21139        0.17
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished     90 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
  ARP220     sess217.C2048glob     1 2 3 4 5 6 7 8 9 10 13 15  +     6.750   962.311
  3C286      sess217.C2048glob     22                                0.067     0.000
  J1516+1932 sess217.C2048glob     1 2 3 4 5 6 7 8 9 10 13 15  +     1.456   115.850
  J1532+2344 sess217.C2048glob     1 2 3 4 5 6 7 8 9 10 13 15  +     2.541   356.089


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) 
   ARP220             128.8
   3C286              106.0
   J1516+1932         130.1
   J1532+2344         128.3

  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 

