  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 18cm global VLBI observations of the starburst galaxy Arp 220
 Exp. Code:  gv028c  


Schedule Version:       2.00
Processed by SCHED version:  11.60  Release 11.6; April 2020

PI:       Eskil Varenius

Address:  Chalmers University of Technology
          Onsala Space Observatory
          439 92 Onsala
          Sweden

Phone:    +46706755341
EMAIL:    eskil.varenius@chalmers.se
Fax:
Phone during observation: +46706755341

Observing mode: vlbi

Notes:    VLA please use all 27 stations at 18cm.
          Phase calibrator: J1532+2344
          Fringe finder: J1516+1932
          Pol. cal.: OQ208


COVER LETTER:


This is one of three .key files to observe Arp 220 at 18cm, 6cm and 3.6cm
during EVN session I 2023. Arp 220 has two nuclei 1 arcsec apart; we aim
to point right in the middle of them, to get both at the same time.

OPERATOR NOTES:
VLA27: Please use all 27 stations at 18cm.

Schedule for HART      (Code Hh )                                   Page   2
               18cm global VLBI observations of the starburst galaxy Arp 220
  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
----------------------------------------------------------------------------------------

 --- Sun  12 Mar 2023   Day  71 ---

 Next scan frequencies:  1626.00  1626.00  1626.00  1626.00  1690.00  1690.00  1690.00  1690.00
 Next BBC frequencies:    116.00   116.00   116.00   116.00   180.00   180.00   180.00   180.00
 Next scan bandwidths:     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00

22 30 00  J1516+1932   11 41 59  20.7  54.6 -3.6       0.0     0        0   22 30 00
22 35 00  =1514+197    11 47 00  21.6  53.8 -3.5       0.0   300       39   22 30 01

22 37 23  OQ208        11 49 23  26.4  34.0 -2.3       0.0    81       39   22 37 23
22 42 23  ---          11 54 24  27.0  32.9 -2.2       0.0   300       77   22 37 24

22 44 35  J1532+2344   11 56 36  17.8  51.4 -3.6       0.0    62       77   22 44 35
22 46 05  =1530+239    11 58 06  18.1  51.1 -3.6       0.0    90       89   22 44 36

22 46 31  ARP220       11 58 33  17.9  51.6 -3.6       0.0     1       89   22 46 31
22 57 01  ---          12 09 04  19.7  49.9 -3.4       0.0   630      170   22 46 32

22 57 28  J1532+2344   12 09 31  20.0  49.3 -3.4       0.0     1      170   22 57 28
22 58 58  =1530+239    12 11 02  20.3  49.1 -3.4       0.0    90      182   22 57 29

22 59 24  ARP220       12 11 28  20.2  49.5 -3.4       0.0     1      182   22 59 24
23 09 54  ---          12 22 00  21.9  47.8 -3.2       0.0   630      263   22 59 25

23 10 21  J1532+2344   12 22 27  22.2  47.2 -3.2       0.0     1      263   23 10 21
23 11 51  =1530+239    12 23 57  22.5  46.9 -3.2       0.0    90      274   23 10 22

23 12 18  ARP220       12 24 24  22.3  47.4 -3.2       0.0     1      274   23 12 18
23 22 48  ---          12 34 55  24.0  45.5 -3.0       0.0   630      356   23 12 19

23 23 15  J1532+2344   12 35 22  24.3  44.9 -3.0       0.0     1      356   23 23 15
23 24 45  =1530+239    12 36 53  24.5  44.6 -2.9       0.0    90      367   23 23 16

23 25 11  ARP220       12 37 19  24.4  45.1 -3.0       0.0     1      367   23 25 11
23 35 41  ---          12 47 51  26.1  43.2 -2.8       0.0   630      448   23 25 12

23 36 08  J1532+2344   12 48 18  26.3  42.5 -2.8       0.0     1      448   23 36 08
23 37 38  =1530+239    12 49 48  26.5  42.2 -2.7       0.0    90      460   23 36 09

23 39 54  OQ208        12 52 04  32.8  19.9 -1.3       0.0    65      460   23 39 54
23 44 54  ---          12 57 05  33.2  18.7 -1.2       0.0   300      499   23 39 55

23 47 04  J1532+2344   12 59 16  27.9  40.3 -2.6       0.0    61      499   23 47 04
23 48 34  =1530+239    13 00 46  28.2  40.0 -2.6       0.0    90      510   23 47 05

23 49 01  ARP220       13 01 13  28.1  40.6 -2.6       0.0     1      510   23 49 01
23 59 31  ---          13 11 45  29.6  38.4 -2.4       0.0   630      591   23 49 02
Schedule for HART      (Code Hh )                                   Page   3
               18cm global VLBI observations of the starburst galaxy Arp 220
  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: Sun  12 Mar 2023   Day  71 -- Stop: Mon  13 Mar 2023   Day  72 ---

23 59 58  J1532+2344   13 12 12  29.8  37.7 -2.4       0.0     1      591   23 59 58
00 01 28  =1530+239    13 13 42  30.0  37.4 -2.3       0.0    90      603   23 59 59

00 01 54  ARP220       13 14 08  29.9  37.9 -2.4       0.0     1      603   00 01 54
00 12 24  ---          13 24 40  31.3  35.6 -2.2       0.0   630      684   00 01 55

00 12 51  J1532+2344   13 25 07  31.5  34.9 -2.1       0.0     1      684   00 12 51
00 14 21  =1530+239    13 26 37  31.7  34.5 -2.1       0.0    90      696   00 12 52

00 14 47  ARP220       13 27 04  31.7  35.1 -2.1       0.0     1      696   00 14 47
00 25 17  ---          13 37 35  33.0  32.7 -2.0       0.0   630      777   00 14 48

00 25 44  J1532+2344   13 38 02  33.1  31.9 -1.9       0.0     1      777   00 25 44
00 27 14  =1530+239    13 39 33  33.3  31.6 -1.9       0.0    90      788   00 25 45

00 27 41  ARP220       13 39 59  33.3  32.1 -1.9       0.0     1      788   00 27 41
00 38 11  ---          13 50 31  34.5  29.6 -1.8       0.0   630      870   00 27 42

00 38 37  J1532+2344   13 50 58  34.6  28.8 -1.7       0.0     1      870   00 38 37
00 40 07  =1530+239    13 52 28  34.7  28.5 -1.7       0.0    90      881   00 38 38

00 42 18  OQ208        13 54 39  35.7   3.6 -0.2       0.0    60      881   00 42 18
00 47 18  ---          13 59 39  35.7   2.3 -0.1       0.0   300      920   00 42 19

00 49 23  J1532+2344   14 01 45  35.7  26.2 -1.5       0.0    56      920   00 49 23
00 50 53  =1530+239    14 03 15  35.8  25.8 -1.5       0.0    90      931   00 49 24

00 51 19  ARP220       14 03 41  35.9  26.3 -1.5       0.0     1      931   00 51 19
01 01 49  ---          14 14 13  36.9  23.6 -1.4       0.0   630     1013   00 51 20

01 02 16  J1532+2344   14 14 40  36.9  22.8 -1.3       0.0     1     1013   01 02 16
01 03 46  =1530+239    14 16 10  37.0  22.4 -1.3       0.0    90     1024   01 02 17

01 04 12  ARP220       14 16 36  37.1  23.0 -1.3       0.0     1     1024   01 04 12
01 14 42  ---          14 27 08  38.0  20.1 -1.1       0.0   630     1105   01 04 13

01 15 09  J1532+2344   14 27 35  37.9  19.3 -1.1       0.0     1     1105   01 15 09
01 16 39  =1530+239    14 29 05  38.0  18.9 -1.1       0.0    90     1117   01 15 10

01 17 05  ARP220       14 29 31  38.1  19.5 -1.1       0.0     1     1117   01 17 05
01 27 35  ---          14 40 03  38.9  16.5 -0.9       0.0   630     1198   01 17 06

01 28 01  J1532+2344   14 40 30  38.8  15.7 -0.9       0.0     1     1198   01 28 01
01 29 31  =1530+239    14 42 00  38.9  15.3 -0.9       0.0    90     1210   01 28 02
Schedule for HART      (Code Hh )                                   Page   4
               18cm global VLBI observations of the starburst galaxy Arp 220
  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
----------------------------------------------------------------------------------------

 --- Mon  13 Mar 2023   Day  72 ---

01 29 58  ARP220       14 42 26  39.0  15.9 -0.9       0.0     1     1210   01 29 58
01 40 28  ---          14 52 58  39.6  12.8 -0.7       0.0   630     1291   01 29 59

01 40 54  J1532+2344   14 53 25  39.5  12.0 -0.7       0.0     1     1291   01 40 54
01 42 24  =1530+239    14 54 55  39.6  11.6 -0.6       0.0    90     1302   01 40 55

01 44 25  OQ208        14 56 56  34.5 346.9  0.8       0.0    50     1302   01 44 25
01 49 25  ---          15 01 57  34.2 345.6  0.9       0.0   300     1341   01 44 26

01 51 24  J1532+2344   15 03 56  39.9   8.9 -0.5       0.0    50     1341   01 51 24
01 52 54  =1530+239    15 05 26  40.0   8.5 -0.5       0.0    90     1353   01 51 25

01 53 20  ARP220       15 05 53  40.2   9.0 -0.5       0.0     1     1353   01 53 20
02 03 50  ---          15 16 24  40.5   5.9 -0.3       0.0   630     1434   01 53 21

02 04 18  J1532+2344   15 16 52  40.3   5.1 -0.3       0.0     2     1434   02 04 18
02 05 48  =1530+239    15 18 23  40.3   4.6 -0.3       0.0    90     1445   02 04 19

02 06 15  ARP220       15 18 50  40.5   5.2 -0.3       0.0     1     1445   02 06 15
02 16 45  ---          15 29 21  40.7   2.0 -0.1       0.0   630     1527   02 06 16

02 17 14  J1532+2344   15 29 50  40.4   1.2 -0.1       0.0     3     1527   02 17 14
02 18 44  =1530+239    15 31 20  40.5   0.7 -0.0       0.0    90     1538   02 17 15

02 19 11  ARP220       15 31 48  40.7   1.3 -0.1       0.0     2     1538   02 19 11
02 29 41  ---          15 42 19  40.7 358.1  0.1       0.0   630     1619   02 19 12

02 30 10  J1532+2344   15 42 49  40.4 357.3  0.2       0.0     4     1619   02 30 10
02 31 40  =1530+239    15 44 19  40.4 356.8  0.2       0.0    90     1631   02 30 11

02 32 08  ARP220       15 44 47  40.6 357.3  0.1       0.0     2     1631   02 32 08
02 42 38  ---          15 55 19  40.5 354.2  0.3       0.0   630     1712   02 32 09

02 43 08  J1532+2344   15 55 49  40.2 353.4  0.4       0.0     4     1712   02 43 08
02 44 38  =1530+239    15 57 19  40.1 352.9  0.4       0.0    90     1724   02 43 09

02 47 21  OQ208        16 00 02  29.5 331.7  1.9       0.0    92     1724   02 47 21
02 52 21  ---          16 05 03  28.9 330.6  1.9       0.0   300     1762   02 47 22

02 54 59  J1532+2344   16 07 42  39.8 349.9  0.6       0.0    89     1762   02 54 59
02 56 29  =1530+239    16 09 12  39.7 349.4  0.6       0.0    90     1774   02 55 00

02 56 58  ARP220       16 09 41  40.0 349.9  0.6       0.0     4     1774   02 56 58
03 07 28  ---          16 20 13  39.5 346.8  0.7       0.0   630     1855   02 56 59
Schedule for HART      (Code Hh )                                   Page   5
               18cm global VLBI observations of the starburst galaxy Arp 220
  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
----------------------------------------------------------------------------------------

 --- Mon  13 Mar 2023   Day  72 ---

03 07 59  J1532+2344   16 20 44  39.2 346.1  0.8       0.0     6     1855   03 07 59
03 09 29  =1530+239    16 22 14  39.1 345.7  0.8       0.0    90     1867   03 08 00

03 09 59  ARP220       16 22 44  39.4 346.1  0.8       0.0     4     1867   03 09 59
03 20 29  ---          16 33 16  38.8 343.1  1.0       0.0   630     1948   03 10 00

03 21 01  J1532+2344   16 33 48  38.4 342.4  1.0       0.0     6     1948   03 21 01
03 22 31  =1530+239    16 35 18  38.3 342.0  1.0       0.0    90     1959   03 21 02

03 23 01  ARP220       16 35 48  38.6 342.4  1.0       0.0     5     1959   03 23 01
03 33 31  ---          16 46 20  37.8 339.4  1.2       0.0   630     2040   03 23 02

03 34 03  J1532+2344   16 46 52  37.4 338.8  1.2       0.0     7     2040   03 34 03
03 35 33  =1530+239    16 48 22  37.3 338.4  1.2       0.0    90     2052   03 34 04

03 36 03  ARP220       16 48 53  37.6 338.8  1.2       0.0     5     2052   03 36 03
03 46 33  ---          16 59 24  36.7 335.9  1.4       0.0   630     2133   03 36 04

03 47 06  J1532+2344   16 59 57  36.3 335.4  1.4       0.0     7     2133   03 47 06
03 48 36  =1530+239    17 01 27  36.1 335.0  1.5       0.0    90     2145   03 47 07

03 51 44  OQ208        17 04 36  21.2 318.9  2.9       0.0   117     2145   03 51 44
03 56 44  ---          17 09 36  20.4 318.0  3.0       0.0   300     2183   03 51 45

03 59 41  J1532+2344   17 12 34  35.0 332.1  1.6       0.0   108     2183   03 59 41
04 01 11  =1530+239    17 14 04  34.8 331.8  1.7       0.0    90     2195   03 59 42

04 01 42  ARP220       17 14 35  35.2 332.1  1.6       0.0     6     2195   04 01 42
04 12 12  ---          17 25 07  34.1 329.5  1.8       0.0   630     2276   04 01 43

04 12 44  J1532+2344   17 25 40  33.5 329.0  1.9       0.0     7     2276   04 12 44
04 14 14  =1530+239    17 27 10  33.4 328.6  1.9       0.0    90     2288   04 12 45

04 14 46  ARP220       17 27 41  33.8 328.9  1.9       0.0     6     2288   04 14 46
04 25 16  ---          17 38 13  32.5 326.4  2.0       0.0   630     2369   04 14 47

04 25 48  J1532+2344   17 38 46  32.0 325.9  2.1       0.0     7     2369   04 25 48
04 27 18  =1530+239    17 40 16  31.8 325.6  2.1       0.0    90     2381   04 25 49

04 27 49  ARP220       17 40 47  32.2 325.8  2.1       0.0     6     2381   04 27 49
04 38 19  ---          17 51 19  30.8 323.5  2.3       0.0   630     2462   04 27 50

04 38 52  J1532+2344   17 51 52  30.3 323.1  2.3       0.0     7     2462   04 38 52
04 40 22  =1530+239    17 53 22  30.0 322.7  2.3       0.0    90     2473   04 38 53
Schedule for HART      (Code Hh )                                   Page   6
               18cm global VLBI observations of the starburst galaxy Arp 220
  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
----------------------------------------------------------------------------------------

 --- Mon  13 Mar 2023   Day  72 ---

04 40 53  ARP220       17 53 53  30.5 322.9  2.3       0.0     6     2473   04 40 53
04 51 23  ---          18 04 25  29.0 320.7  2.5       0.0   630     2554   04 40 54

04 51 55  J1532+2344   18 04 57  28.4 320.3  2.5       0.0     7     2554   04 51 55
04 53 25  =1530+239    18 06 28  28.2 320.0  2.5       0.0    90     2566   04 51 56

04 56 16  OQ208        18 09 19  10.7 308.9  4.0       0.0   101     2566   04 56 16
04 57 16  ---          18 10 19  10.5 308.8  4.0       0.0    60     2574   04 56 17

04 57 16  OQ208        18 10 19  10.5 308.8  4.0       0.0   -20     2574   No stop 
05 01 16  ---          18 14 20   9.8 308.2  4.1       0.0   220     2605   04 57 17

05 03 55  J1532+2344   18 16 59  26.7 318.0  2.7       0.0    90     2605   05 03 55
05 04 55  =1530+239    18 17 59  26.5 317.8  2.7       0.0    60     2612   05 03 56

05 04 55  J1532+2344   18 17 59  26.5 317.8  2.7       0.0   -20     2612   No stop 
05 05 25  =1530+239    18 18 29  26.4 317.7  2.7       0.0    10     2616   05 04 56

05 05 56  ARP220       18 19 00  26.9 317.8  2.7       0.0     5     2616   05 05 56
05 16 26  ---          18 29 32  25.2 315.8  2.9       0.0   630     2697   05 05 57

05 16 58  J1532+2344   18 30 04  24.6 315.5  2.9       0.0     6     2697   05 16 58
05 17 58  =1530+239    18 31 04  24.5 315.3  3.0       0.0    60     2705   05 16 59

05 17 58  J1532+2344   18 31 04  24.5 315.3  3.0       0.0   -20     2705   No stop 
05 18 28  =1530+239    18 31 34  24.4 315.2  3.0       0.0    10     2709   05 17 59

05 18 58  ARP220       18 32 04  24.8 315.4  2.9       0.0     5     2709   05 18 58
05 29 28  ---          18 42 36  23.1 313.5  3.1       0.0   630     2790   05 18 59

05 30 00  J1532+2344   18 43 08  22.5 313.2  3.2       0.0     6     2790   05 30 00
05 31 00  =1530+239    18 44 08  22.4 313.0  3.2       0.0    60     2798   05 30 01

05 31 00  J1532+2344   18 44 08  22.4 313.0  3.2       0.0   -20     2798   No stop 
05 31 30  =1530+239    18 44 38  22.3 312.9  3.2       0.0    10     2802   05 31 01

05 32 00  ARP220       18 45 08  22.7 313.0  3.2       0.0     5     2802   05 32 00
05 42 30  ---          18 55 40  21.0 311.2  3.3       0.0   630     2883   05 32 01

05 43 01  J1532+2344   18 56 11  20.4 311.0  3.4       0.0     5     2883   05 43 01
05 44 01  =1530+239    18 57 11  20.2 310.8  3.4       0.0    60     2891   05 43 02

05 44 01  J1532+2344   18 57 11  20.2 310.8  3.4       0.0   -20     2891   No stop 
05 44 31  =1530+239    18 57 41  20.1 310.7  3.4       0.0    10     2895   05 44 02
Schedule for HART      (Code Hh )                                   Page   7
               18cm global VLBI observations of the starburst galaxy Arp 220
  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
----------------------------------------------------------------------------------------

 --- Mon  13 Mar 2023   Day  72 ---

05 45 01  ARP220       18 58 11  20.5 310.8  3.4       0.0     4     2895   05 45 01
05 55 31  ---          19 08 43  18.7 309.1  3.5       0.0   630     2976   05 45 02

05 56 01  J1532+2344   19 09 14  18.1 308.9  3.6       0.0     5     2976   05 56 01
05 57 31  =1530+239    19 10 44  17.8 308.7  3.6       0.0    90     2987   05 56 02


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


 ======== Setup file: sess123.L1024glob
   Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat:
     hh18cm          Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  122.00 of  256.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:   16         Station: HART              Total bit rate:  1024
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels:  8    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
   Net SB=         L         L         U         U         L         L         U         U
   IF SB =         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         2        10         2        10
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        A1        C1        A1        C1        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  10  Setup file default.  Used with PCAL = off
   LO sum=   1626.00  1626.00  1626.00  1626.00  1690.00  1690.00  1690.00  1690.00
   BBC fr=    116.00   116.00   116.00   116.00   180.00   180.00   180.00   180.00
   Bandwd=     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
    Matching frequency sets:  10

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8
    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 57.940194       0.00
                     23 40 07.75728    * 23 30 11.33000      23 25 18.96580        0.00
                     From catalog imbedded in main SCHED input file.

 * 3C286             13 28 49.657769   * 13 31 08.288061     13 32 13.487531       0.17
   J1331+3030        30 45 58.64066    * 30 30 32.95930      30 23 13.19246        0.16
   1328+307          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J1331+30          GSFC 2016a X/S astro solution,    269 observations.

 * OQ208             14 04 45.615156   * 14 07 00.394415     14 08 03.650024       0.24
   J1407+2827        28 41 29.23515    * 28 27 14.69019      28 20 26.03181        0.35
   1404+286          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J1407+28          GSFC 2016a X/S astro solution,  68278 observations.

   1514+197          15 14 40.985841   * 15 16 56.796164     15 18 00.065612       0.01
 * J1516+1932        19 43 10.94247    * 19 32 12.99203      19 26 53.79356        0.02
   J1516+19          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,   4472 observations.

   1530+239          15 30 36.092759   * 15 32 46.345214     15 33 47.008502       0.08
 * J1532+2344        23 54 09.32913    * 23 44 05.26796      23 39 09.39949        0.14
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    171 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     sess123.L1024glob     1 2 3 4 5 6 7 8 9 10 11 17  +    12.250  1600.189
  3C286      sess123.L1024glob     17                                0.133     0.000
  OQ208      sess123.L1024glob     1 2 3 4 5 6 7 8 9 10 11 17  +     1.500   188.550
  J1516+1932 sess123.L1024glob     1 2 3 4 5 6 7 8 9 10 11           0.083    10.000
  J1532+2344 sess123.L1024glob     1 2 3 4 5 6 7 8 9 10 11 17  +     2.183   275.621


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             117.8
   3C286              140.6
   OQ208              135.1
   J1516+1932         122.6
   J1532+2344         118.2

  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 

