  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
 Exp. Code:  EM117N  


Schedule Version:       2.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       L. Moscadelli

Address:  Osservatorio Astrofisico di Arcetri
          Via E.Fermi 5
          I-50125, Firenze
          Italy

Phone:    +39 055 2752220
EMAIL:    mosca@arcetri.astro.it
Fax:      +39 055 220039
Phone during observation: +39 055 2752220

Observing mode: Polarization observations of 1 source at 6.7 GHz (128 Mb/s

Notes:    phase-cal OFF
          source = G25.65+1.05
 
 

Schedule for HART      (Code Hh )                                   Page   2
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

 Next scan frequencies:  6665.52  6665.52  6665.52  6665.52  6669.52  6669.52  6669.52  6669.52
                         6673.52  6673.52  6673.52  6673.52  6677.52  6677.52  6677.52  6677.52
 Next BBC frequencies:    155.52   155.52   155.52   155.52   159.52   159.52   159.52   159.52
                          163.52   163.52   163.52   163.52   167.52   167.52   167.52   167.52
 Next scan bandwidths:      2.00     2.00     2.00     2.00     2.00     2.00     2.00     2.00
                            2.00     2.00     2.00     2.00     2.00     2.00     2.00     2.00

02 45 35  J1331+3030   15 19 40  28.1 333.7  1.8       0.0     0        0   02 45 35
02 50 35  =3C286       15 24 41  27.6 332.7  1.9       0.0   300        5   02 45 36

02 51 05  J1331+3030   15 25 11  27.5 332.5  1.9       0.0     9        5   02 51 05
02 59 05  =3C286       15 33 13  26.7 330.9  2.0       0.0   480       13   02 51 06

03 03 31  3C345        15 37 39  22.6  13.7 -1.1       0.0   144       13   03 03 31
03 13 31  ---          15 47 41  23.1  11.6 -0.9       0.0   600       22   03 03 32

03 30 06  J1821-0502   16 04 19  51.0  63.6 -2.3       0.0   878       22   03 30 06
03 35 06  =1818-050    16 09 20  52.0  62.4 -2.2       0.0   300       27   03 30 07

03 35 06  G25.65+1.05  16 09 20  49.9  66.6 -2.4       0.0   -33       27   No stop 
03 37 06  ---          16 11 20  50.3  66.2 -2.4       0.0    87       29   03 35 07

03 37 51  J1821-0502   16 12 05  52.6  61.7 -2.2       0.0    11       29   03 37 51
03 40 41  =1818-050    16 14 55  53.1  61.0 -2.1       0.0   170       32   03 37 52

03 40 41  G25.65+1.05  16 14 55  51.0  65.4 -2.3       0.0   -33       32   No stop 
03 42 41  ---          16 16 56  51.4  65.0 -2.3       0.0    87       34   03 40 42

03 42 41  J1821-0502   16 16 56  53.5  60.5 -2.1       0.0   -34       34   No stop 
03 45 41  =1818-050    16 19 56  54.1  59.7 -2.0       0.0   146       37   03 42 42

03 45 41  G25.65+1.05  16 19 56  52.1  64.3 -2.3       0.0   -33       37   No stop 
03 47 41  ---          16 21 57  52.5  63.8 -2.2       0.0    87       38   03 45 42

03 48 26  J1821-0502   16 22 42  54.6  59.0 -2.0       0.0    11       38   03 48 26
03 51 16  =1818-050    16 25 32  55.2  58.2 -1.9       0.0   170       41   03 48 27

03 51 16  G25.65+1.05  16 25 32  53.2  62.9 -2.2       0.0   -33       41   No stop 
03 53 16  ---          16 27 33  53.6  62.4 -2.1       0.0    87       43   03 51 17

03 53 16  J1821-0502   16 27 33  55.6  57.6 -1.9       0.0   -34       43   No stop 
03 56 16  =1818-050    16 30 33  56.1  56.8 -1.9       0.0   146       46   03 53 17

03 56 16  G25.65+1.05  16 30 33  54.2  61.7 -2.1       0.0   -33       46   No stop 
03 58 16  ---          16 32 33  54.6  61.1 -2.0       0.0    87       48   03 56 17
Schedule for HART      (Code Hh )                                   Page   3
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

03 58 16  J1821-0502   16 32 33  56.5  56.2 -1.8       0.0   -34       48   No stop 
04 01 16  =1818-050    16 35 34  57.1  55.3 -1.8       0.0   146       51   03 58 17

04 01 16  G25.65+1.05  16 35 34  55.2  60.3 -2.0       0.0   -33       51   No stop 
04 03 16  ---          16 37 34  55.6  59.8 -2.0       0.0    87       53   04 01 17

04 04 01  J1821-0502   16 38 19  57.6  54.4 -1.7       0.0    11       53   04 04 01
04 06 51  =1818-050    16 41 10  58.1  53.5 -1.7       0.0   170       56   04 04 02

04 06 51  G25.65+1.05  16 41 10  56.3  58.8 -1.9       0.0   -33       56   No stop 
04 08 51  ---          16 43 10  56.6  58.2 -1.9       0.0    87       57   04 06 52

04 08 51  J1821-0502   16 43 10  58.4  52.8 -1.6       0.0   -34       57   No stop 
04 11 51  =1818-050    16 46 11  59.0  51.8 -1.6       0.0   146       60   04 08 52

04 28 01  J1821-0502   17 02 23  61.7  45.8 -1.3       0.0   948       60   04 28 01
04 31 01  =1818-050    17 05 24  62.2  44.6 -1.3       0.0   180       63   04 28 02

04 31 01  G25.65+1.05  17 05 24  60.7  51.0 -1.5       0.0   -33       63   No stop 
04 33 01  ---          17 07 24  61.1  50.3 -1.5       0.0    87       65   04 31 02

04 33 01  J1821-0502   17 07 24  62.5  43.8 -1.2       0.0   -34       65   No stop 
04 36 01  =1818-050    17 10 25  63.0  42.5 -1.2       0.0   146       68   04 33 02

04 36 01  G25.65+1.05  17 10 25  61.6  49.2 -1.4       0.0   -33       68   No stop 
04 38 01  ---          17 12 25  61.9  48.4 -1.4       0.0    87       70   04 36 02

04 38 01  J1821-0502   17 12 25  63.3  41.6 -1.2       0.0   -34       70   No stop 
04 41 01  =1818-050    17 15 25  63.7  40.2 -1.1       0.0   146       73   04 38 02

04 41 01  G25.65+1.05  17 15 25  62.4  47.2 -1.3       0.0   -33       73   No stop 
04 43 01  ---          17 17 26  62.8  46.4 -1.3       0.0    87       75   04 41 02

04 43 46  J1821-0502   17 18 11  64.1  39.0 -1.1       0.0    11       75   04 43 46
04 46 36  =1818-050    17 21 01  64.5  37.6 -1.0       0.0   170       78   04 43 47

04 46 36  G25.65+1.05  17 21 01  63.3  44.9 -1.2       0.0   -33       78   No stop 
04 48 36  ---          17 23 02  63.7  44.0 -1.2       0.0    87       80   04 46 37

04 48 36  J1821-0502   17 23 02  64.8  36.6 -1.0       0.0   -34       80   No stop 
04 51 36  =1818-050    17 26 02  65.2  35.1 -0.9       0.0   146       82   04 48 37

04 51 36  G25.65+1.05  17 26 02  64.1  42.7 -1.2       0.0   -33       82   No stop 
04 53 36  ---          17 28 02  64.4  41.8 -1.1       0.0    87       84   04 51 37
Schedule for HART      (Code Hh )                                   Page   4
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

04 53 36  J1821-0502   17 28 02  65.4  34.1 -0.9       0.0   -34       84   No stop 
04 56 36  =1818-050    17 31 03  65.8  32.5 -0.9       0.0   146       87   04 53 37

04 56 36  G25.65+1.05  17 31 03  64.9  40.4 -1.1       0.0   -33       87   No stop 
04 58 36  ---          17 33 03  65.2  39.4 -1.0       0.0    87       89   04 56 37

04 59 21  J1821-0502   17 33 48  66.1  31.0 -0.8       0.0    11       89   04 59 21
05 02 11  =1818-050    17 36 39  66.5  29.5 -0.8       0.0   170       92   04 59 22

05 02 11  G25.65+1.05  17 36 39  65.7  37.6 -1.0       0.0   -33       92   No stop 
05 04 11  ---          17 38 39  65.9  36.6 -0.9       0.0    87       94   05 02 12

05 04 11  J1821-0502   17 38 39  66.7  28.3 -0.7       0.0   -34       94   No stop 
05 07 11  =1818-050    17 41 40  67.0  26.6 -0.7       0.0   146       97   05 04 12

05 23 46  J1821-0502   17 58 17  68.4  16.3 -0.4       0.0   973       97   05 23 46
05 26 46  =1818-050    18 01 18  68.6  14.3 -0.3       0.0   180      100   05 23 47

05 26 46  G25.65+1.05  18 01 18  68.5  23.6 -0.6       0.0   -33      100   No stop 
05 28 46  ---          18 03 18  68.7  22.4 -0.5       0.0    87      102   05 26 47

05 28 46  J1821-0502   18 03 18  68.7  13.0 -0.3       0.0   -34      102   No stop 
05 31 46  =1818-050    18 06 19  68.8  11.0 -0.3       0.0   146      105   05 28 47

05 31 46  G25.65+1.05  18 06 19  68.9  20.4 -0.5       0.0   -33      105   No stop 
05 33 46  ---          18 08 19  69.1  19.1 -0.4       0.0    87      106   05 31 47

05 33 46  J1821-0502   18 08 19  68.9   9.6 -0.2       0.0   -34      106   No stop 
05 36 46  =1818-050    18 11 20  69.0   7.5 -0.2       0.0   146      109   05 33 47

05 36 46  G25.65+1.05  18 11 20  69.3  17.1 -0.4       0.0   -33      109   No stop 
05 38 46  ---          18 13 20  69.4  15.7 -0.4       0.0    87      111   05 36 47

05 39 31  J1821-0502   18 14 05  69.1   5.6 -0.1       0.0    11      111   05 39 31
05 42 21  =1818-050    18 16 55  69.1   3.6 -0.1       0.0   170      114   05 39 32

05 42 21  G25.65+1.05  18 16 55  69.6  13.2 -0.3       0.0   -33      114   No stop 
05 44 21  ---          18 18 56  69.7  11.8 -0.3       0.0    87      116   05 42 22

05 44 21  J1821-0502   18 18 56  69.1   2.2 -0.1       0.0   -34      116   No stop 
05 47 21  =1818-050    18 21 56  69.1   0.1 -0.0       0.0   146      119   05 44 22

05 47 21  G25.65+1.05  18 21 56  69.8   9.7 -0.2       0.0   -33      119   No stop 
05 49 21  ---          18 23 57  69.9   8.2 -0.2       0.0    87      121   05 47 22
Schedule for HART      (Code Hh )                                   Page   5
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

05 49 21  J1821-0502   18 23 57  69.1 358.7  0.0       0.0   -34      121   No stop 
05 52 21  =1818-050    18 26 57  69.1 356.6  0.1       0.0   146      124   05 49 22

05 52 21  G25.65+1.05  18 26 57  70.0   6.1 -0.1       0.0   -33      124   No stop 
05 54 21  ---          18 28 57  70.0   4.6 -0.1       0.0    87      126   05 52 22

05 55 06  J1821-0502   18 29 43  69.1 354.7  0.1       0.0    11      126   05 55 06
05 57 56  =1818-050    18 32 33  69.0 352.8  0.2       0.0   170      128   05 55 07

05 57 56  G25.65+1.05  18 32 33  70.1   2.0 -0.0       0.0   -33      128   No stop 
05 59 56  ---          18 34 33  70.1   0.5 -0.0       0.0    87      130   05 57 57

05 59 56  J1821-0502   18 34 33  68.9 351.4  0.2       0.0   -34      130   No stop 
06 02 56  =1818-050    18 37 34  68.8 349.3  0.3       0.0   146      133   05 59 57

06 07 26  J2202+4216   18 42 05   7.5  35.0 -3.4  D    0.0   133      133   06 07 26
06 15 26  =VR422201    18 50 06   8.5  33.9 -3.2       0.0     0      141   06 07 27

06 20 06  J1821-0502   18 54 47  67.7 338.1  0.5       0.0   141      141   06 20 06
06 23 06  =1818-050    18 57 47  67.5 336.3  0.6       0.0   180      144   06 20 07

06 23 06  G25.65+1.05  18 57 47  69.4 343.9  0.4       0.0   -33      144   No stop 
06 25 06  ---          18 59 47  69.2 342.6  0.4       0.0    87      146   06 23 07

06 25 06  J1821-0502   18 59 47  67.3 335.1  0.6       0.0   -34      146   No stop 
06 28 06  =1818-050    19 02 48  67.0 333.3  0.7       0.0   146      149   06 25 07

06 28 06  G25.65+1.05  19 02 48  69.0 340.6  0.5       0.0   -33      149   No stop 
06 30 06  ---          19 04 48  68.9 339.2  0.5       0.0    87      151   06 28 07

06 30 06  J1821-0502   19 04 48  66.8 332.1  0.7       0.0   -34      151   No stop 
06 33 06  =1818-050    19 07 49  66.5 330.4  0.8       0.0   146      153   06 30 07

06 33 06  G25.65+1.05  19 07 49  68.6 337.3  0.5       0.0   -33      153   No stop 
06 35 06  ---          19 09 49  68.5 336.0  0.6       0.0    87      155   06 33 07

06 35 51  J1821-0502   19 10 34  66.1 328.9  0.8       0.0    11      155   06 35 51
06 38 41  =1818-050    19 13 25  65.8 327.4  0.9       0.0   170      158   06 35 52

06 38 41  G25.65+1.05  19 13 25  68.1 333.8  0.6       0.0   -33      158   No stop 
06 40 41  ---          19 15 25  67.9 332.6  0.7       0.0    87      160   06 38 42

06 40 41  J1821-0502   19 15 25  65.6 326.3  0.9       0.0   -34      160   No stop 
06 43 41  =1818-050    19 18 26  65.2 324.8  0.9       0.0   146      163   06 40 42
Schedule for HART      (Code Hh )                                   Page   6
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

06 43 41  G25.65+1.05  19 18 26  67.6 330.8  0.7       0.0   -33      163   No stop 
06 45 41  ---          19 20 26  67.4 329.6  0.8       0.0    87      165   06 43 42

06 45 41  J1821-0502   19 20 26  64.9 323.8  1.0       0.0   -34      165   No stop 
06 48 41  =1818-050    19 23 26  64.5 322.3  1.0       0.0   146      168   06 45 42

06 48 41  G25.65+1.05  19 23 26  67.0 327.9  0.8       0.0   -33      168   No stop 
06 50 41  ---          19 25 27  66.8 326.8  0.8       0.0    87      170   06 48 42

06 51 26  J1821-0502   19 26 12  64.1 321.0  1.1       0.0    11      170   06 51 26
06 54 16  =1818-050    19 29 02  63.7 319.7  1.1       0.0   170      172   06 51 27

06 54 16  G25.65+1.05  19 29 02  66.3 324.9  0.9       0.0   -33      172   No stop 
06 56 16  ---          19 31 03  66.0 323.8  0.9       0.0    87      174   06 54 17

06 56 16  J1821-0502   19 31 03  63.4 318.8  1.1       0.0   -34      174   No stop 
06 59 16  =1818-050    19 34 03  63.0 317.4  1.2       0.0   146      177   06 56 17

07 04 06  J2202+4216   19 38 54  14.0  26.7 -2.4       0.0   153      177   07 04 06
07 12 06  =VR422201    19 46 55  14.8  25.4 -2.3       0.0   480      185   07 04 07

07 17 06  J1821-0502   19 51 56  60.1 310.3  1.5       0.0   161      185   07 17 06
07 20 06  =1818-050    19 54 56  59.5 309.3  1.5       0.0   180      188   07 17 07

07 20 06  G25.65+1.05  19 54 56  62.5 312.9  1.3       0.0   -33      188   No stop 
07 22 06  ---          19 56 57  62.1 312.1  1.4       0.0    87      190   07 20 07

07 22 06  J1821-0502   19 56 57  59.2 308.6  1.6       0.0   -34      190   No stop 
07 25 06  =1818-050    19 59 57  58.7 307.6  1.6       0.0   146      193   07 22 07

07 25 06  G25.65+1.05  19 59 57  61.6 310.9  1.4       0.0   -33      193   No stop 
07 27 06  ---          20 01 58  61.3 310.2  1.4       0.0    87      195   07 25 07

07 27 06  J1821-0502   20 01 58  58.3 306.9  1.7       0.0   -34      195   No stop 
07 30 06  =1818-050    20 04 58  57.8 305.9  1.7       0.0   146      198   07 27 07

07 30 06  G25.65+1.05  20 04 58  60.8 309.1  1.5       0.0   -33      198   No stop 
07 32 06  ---          20 06 58  60.4 308.3  1.5       0.0    87      200   07 30 07

07 32 51  J1821-0502   20 07 44  57.2 305.1  1.8       0.0    11      200   07 32 51
07 35 41  =1818-050    20 10 34  56.7 304.2  1.8       0.0   170      202   07 32 52

07 35 41  G25.65+1.05  20 10 34  59.8 307.1  1.6       0.0   -33      202   No stop 
07 37 41  ---          20 12 34  59.4 306.4  1.6       0.0    87      204   07 35 42
Schedule for HART      (Code Hh )                                   Page   7
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

07 37 41  J1821-0502   20 12 34  56.3 303.6  1.8       0.0   -34      204   No stop 
07 40 41  =1818-050    20 15 35  55.8 302.7  1.9       0.0   146      207   07 37 42

07 40 41  G25.65+1.05  20 15 35  58.9 305.4  1.7       0.0   -33      207   No stop 
07 42 41  ---          20 17 35  58.5 304.8  1.7       0.0    87      209   07 40 42

07 42 41  J1821-0502   20 17 35  55.4 302.1  1.9       0.0   -34      209   No stop 
07 45 41  =1818-050    20 20 36  54.8 301.3  2.0       0.0   146      212   07 42 42

07 45 41  G25.65+1.05  20 20 36  57.9 303.8  1.8       0.0   -33      212   No stop 
07 47 41  ---          20 22 36  57.6 303.2  1.8       0.0    87      214   07 45 42

07 48 26  J1821-0502   20 23 21  54.3 300.6  2.0       0.0    11      214   07 48 26
07 51 16  =1818-050    20 26 12  53.7 299.8  2.1       0.0   170      217   07 48 27

07 51 16  G25.65+1.05  20 26 12  56.9 302.1  1.8       0.0   -33      217   No stop 
07 53 16  ---          20 28 12  56.5 301.6  1.9       0.0    87      219   07 51 17

07 53 16  J1821-0502   20 28 12  53.3 299.3  2.1       0.0   -34      219   No stop 
07 56 16  =1818-050    20 31 12  52.8 298.5  2.2       0.0   146      221   07 53 17

08 01 26  J2202+4216   20 36 23  18.9  16.8 -1.5       0.0   173      221   08 01 26
08 09 26  =VR422201    20 44 25  19.4  15.4 -1.3       0.0   480      229   08 01 27

08 14 26  J1821-0502   20 49 25  49.1 294.3  2.5       0.0   161      229   08 14 26
08 17 26  =1818-050    20 52 26  48.5 293.6  2.5       0.0   180      232   08 14 27

08 17 26  G25.65+1.05  20 52 26  51.7 295.3  2.3       0.0   -33      232   No stop 
08 19 26  ---          20 54 26  51.3 294.9  2.3       0.0    87      234   08 17 27

08 19 26  J1821-0502   20 54 26  48.1 293.2  2.5       0.0   -34      234   No stop 
08 22 26  =1818-050    20 57 27  47.4 292.6  2.6       0.0   146      237   08 19 27

08 22 26  G25.65+1.05  20 57 27  50.7 294.2  2.4       0.0   -33      237   No stop 
08 24 26  ---          20 59 27  50.3 293.7  2.4       0.0    87      239   08 22 27

08 24 26  J1821-0502   20 59 27  47.0 292.2  2.6       0.0   -34      239   No stop 
08 27 26  =1818-050    21 02 28  46.4 291.6  2.7       0.0   146      242   08 24 27

08 27 26  G25.65+1.05  21 02 28  49.6 293.1  2.5       0.0   -33      242   No stop 
08 29 26  ---          21 04 28  49.2 292.7  2.5       0.0    87      244   08 27 27

08 30 11  J1821-0502   21 05 13  45.8 291.1  2.7       0.0    11      244   08 30 11
08 33 01  =1818-050    21 08 03  45.2 290.5  2.8       0.0   170      246   08 30 12
Schedule for HART      (Code Hh )                                   Page   8
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

08 33 01  G25.65+1.05  21 08 03  48.5 291.9  2.5       0.0   -33      246   No stop 
08 35 01  ---          21 10 04  48.1 291.5  2.6       0.0    87      248   08 33 02

08 35 01  J1821-0502   21 10 04  44.8 290.1  2.8       0.0   -34      248   No stop 
08 38 01  =1818-050    21 13 04  44.2 289.6  2.8       0.0   146      251   08 35 02

08 38 01  G25.65+1.05  21 13 04  47.4 290.9  2.6       0.0   -33      251   No stop 
08 40 01  ---          21 15 05  47.0 290.5  2.7       0.0    87      253   08 38 02

08 40 01  J1821-0502   21 15 05  43.7 289.2  2.9       0.0   -34      253   No stop 
08 43 01  =1818-050    21 18 05  43.1 288.7  2.9       0.0   146      256   08 40 02

08 43 01  G25.65+1.05  21 18 05  46.4 290.0  2.7       0.0   -33      256   No stop 
08 45 01  ---          21 20 05  45.9 289.6  2.7       0.0    87      258   08 43 02

08 45 46  J1821-0502   21 20 51  42.5 288.2  3.0       0.0    11      258   08 45 46
08 48 36  =1818-050    21 23 41  41.9 287.7  3.0       0.0   170      261   08 45 47

08 48 36  G25.65+1.05  21 23 41  45.2 288.9  2.8       0.0   -33      261   No stop 
08 50 36  ---          21 25 41  44.8 288.6  2.8       0.0    87      263   08 48 37

08 50 36  J1821-0502   21 25 41  41.5 287.4  3.1       0.0   -34      263   No stop 
08 53 36  =1818-050    21 28 42  40.8 286.9  3.1       0.0   146      266   08 50 37

08 59 01  J2202+4216   21 34 08  21.4   5.8 -0.5       0.0   188      266   08 59 01
09 07 01  =VR422201    21 42 09  21.6   4.2 -0.4       0.0   480      273   08 59 02

09 12 36  J1821-0502   21 47 45  36.7 283.9  3.4       0.0   196      273   09 12 36
09 15 36  =1818-050    21 50 45  36.0 283.4  3.5       0.0   180      276   09 12 37

09 15 36  G25.65+1.05  21 50 45  39.4 284.4  3.3       0.0   -33      276   No stop 
09 17 36  ---          21 52 46  38.9 284.1  3.3       0.0    87      278   09 15 37

09 17 36  J1821-0502   21 52 46  35.6 283.1  3.5       0.0   -34      278   No stop 
09 20 36  =1818-050    21 55 46  34.9 282.7  3.6       0.0   146      281   09 17 37

09 20 36  G25.65+1.05  21 55 46  38.3 283.6  3.3       0.0   -33      281   No stop 
09 22 36  ---          21 57 47  37.8 283.3  3.4       0.0    87      283   09 20 37

09 22 36  J1821-0502   21 57 47  34.5 282.4  3.6       0.0   -34      283   No stop 
09 25 36  =1818-050    22 00 47  33.8 282.0  3.6       0.0   146      286   09 22 37

09 25 36  G25.65+1.05  22 00 47  37.2 282.9  3.4       0.0   -33      286   No stop 
09 27 36  ---          22 02 47  36.7 282.6  3.5       0.0    87      288   09 25 37
Schedule for HART      (Code Hh )                                   Page   9
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

09 28 21  J1821-0502   22 03 33  33.2 281.6  3.7       0.0    11      288   09 28 21
09 31 11  =1818-050    22 06 23  32.6 281.2  3.7       0.0   170      290   09 28 22

09 31 11  G25.65+1.05  22 06 23  35.9 282.0  3.5       0.0   -33      290   No stop 
09 33 11  ---          22 08 23  35.5 281.8  3.6       0.0    87      292   09 31 12

09 33 11  J1821-0502   22 08 23  32.1 280.9  3.8       0.0   -34      292   No stop 
09 36 11  =1818-050    22 11 24  31.5 280.5  3.8       0.0   146      295   09 33 12

09 36 11  G25.65+1.05  22 11 24  34.8 281.3  3.6       0.0   -33      295   No stop 
09 38 11  ---          22 13 24  34.4 281.1  3.6       0.0    87      297   09 36 12

09 38 11  J1821-0502   22 13 24  31.0 280.3  3.9       0.0   -34      297   No stop 
09 41 11  =1818-050    22 16 25  30.4 279.9  3.9       0.0   146      300   09 38 12

09 41 11  G25.65+1.05  22 16 25  33.7 280.6  3.7       0.0   -33      300   No stop 
09 43 11  ---          22 18 25  33.3 280.4  3.7       0.0    87      302   09 41 12

09 43 56  J1821-0502   22 19 10  29.8 279.5  4.0       0.0    11      302   09 43 56
09 46 46  =1818-050    22 22 01  29.1 279.1  4.0       0.0   170      305   09 43 57

09 46 46  G25.65+1.05  22 22 01  32.5 279.9  3.8       0.0   -33      305   No stop 
09 48 46  ---          22 24 01  32.0 279.6  3.8       0.0    87      307   09 46 47

09 48 46  J1821-0502   22 24 01  28.7 278.9  4.0       0.0   -34      307   No stop 
09 51 46  =1818-050    22 27 01  28.0 278.5  4.1       0.0   146      310   09 48 47

09 57 11  J2202+4216   22 32 27  21.4 354.2  0.5       0.0   188      310   09 57 11
10 05 11  =VR422201    22 40 29  21.2 352.7  0.6       0.0   480      317   09 57 12

10 10 41  J1821-0502   22 46 00  23.8 276.2  4.4       0.0   191      317   10 10 41
10 13 41  =1818-050    22 49 00  23.1 275.8  4.4       0.0   180      320   10 10 42

10 13 41  G25.65+1.05  22 49 00  26.5 276.4  4.2       0.0   -33      320   No stop 
10 15 41  ---          22 51 00  26.0 276.2  4.3       0.0    87      322   10 13 42

10 15 41  J1821-0502   22 51 00  22.7 275.6  4.5       0.0   -34      322   No stop 
10 18 41  =1818-050    22 54 01  22.0 275.2  4.5       0.0   146      325   10 15 42

10 18 41  G25.65+1.05  22 54 01  25.4 275.8  4.3       0.0   -33      325   No stop 
10 20 41  ---          22 56 01  24.9 275.6  4.3       0.0    87      327   10 18 42

10 20 41  J1821-0502   22 56 01  21.5 275.0  4.6       0.0   -34      327   No stop 
10 23 41  =1818-050    22 59 02  20.9 274.6  4.6       0.0   146      330   10 20 42
Schedule for HART      (Code Hh )                                   Page  10
               A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
  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
----------------------------------------------------------------------------------------

 --- Sat   3 Mar 2018   Day  62 ---

10 23 41  G25.65+1.05  22 59 02  24.2 275.2  4.4       0.0   -33      330   No stop 
10 25 41  ---          23 01 02  23.8 275.0  4.4       0.0    87      332   10 23 42

10 26 26  J1821-0502   23 01 47  20.2 274.3  4.7       0.0    11      332   10 26 26
10 29 16  =1818-050    23 04 38  19.6 274.0  4.7       0.0   170      335   10 26 27

10 29 16  G25.65+1.05  23 04 38  23.0 274.6  4.5       0.0   -33      335   No stop 
10 31 16  ---          23 06 38  22.5 274.4  4.5       0.0    87      337   10 29 17

10 31 16  J1821-0502   23 06 38  19.2 273.8  4.7       0.0   -34      337   No stop 
10 34 16  =1818-050    23 09 38  18.5 273.4  4.8       0.0   146      339   10 31 17

10 34 16  G25.65+1.05  23 09 38  21.8 274.0  4.6       0.0   -33      339   No stop 
10 36 16  ---          23 11 39  21.4 273.8  4.6       0.0    87      341   10 34 17

10 36 16  J1821-0502   23 11 39  18.0 273.2  4.8       0.0   -34      341   No stop 
10 39 16  =1818-050    23 14 39  17.4 272.8  4.9       0.0   146      344   10 36 17

10 39 16  G25.65+1.05  23 14 39  20.7 273.4  4.7       0.0   -33      344   No stop 
10 41 16  ---          23 16 40  20.3 273.2  4.7       0.0    87      346   10 39 17

10 42 01  J1821-0502   23 17 25  16.7 272.5  4.9       0.0    11      346   10 42 01
10 44 51  =1818-050    23 20 15  16.1 272.2  5.0       0.0   170      349   10 42 02

10 44 51  G25.65+1.05  23 20 15  19.5 272.8  4.7       0.0   -33      349   No stop 
10 46 51  ---          23 22 15  19.0 272.6  4.8       0.0    87      351   10 44 52

10 46 51  J1821-0502   23 22 15  15.7 272.0  5.0       0.0   -34      351   No stop 
10 49 51  =1818-050    23 25 16  15.0 271.7  5.1       0.0   146      354   10 46 52

10 54 31  J2202+4216   23 29 57  18.9 343.3  1.4       0.0   143      354   10 54 31
11 02 41  =VR422201    23 38 08  18.3 341.8  1.6       0.0   490      362   10 54 32

11 07 26  J1821-0502   23 42 54  11.0 269.7  5.3       0.0   146      362   11 07 26
11 10 26  =1818-050    23 45 54  10.3 269.4  5.4       0.0   180      365   11 07 27

11 10 26  G25.65+1.05  23 45 54  13.7 269.9  5.2       0.0   -33      365   No stop 
11 12 26  ---          23 47 55  13.2 269.7  5.2       0.0    87      366   11 10 27

11 12 51  J1821-0502   23 48 20   9.8 269.1  5.4       0.0    -9      366   11 12 51
11 17 51  =1818-050    23 53 21   8.7 268.6  5.5       0.0   291      371   11 12 52

11 22 32  J2202+4216   23 58 02  16.8 338.3  1.9       0.0   144      371   11 22 32
11 30 00  =VR422201    00 05 32  16.2 337.0  2.0       0.0   448      379   11 22 33


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


 ======== Setup file: sess118.M128
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat:
     hh5cm           Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only   16.00 of   32.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    5         Station: HART              Total bit rate:   128
   Format: VDIF              Bits per sample: 2         Sample rate:  4.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
             6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
   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:  10  Based on FREQ, BW, and/or DOPPLER in schedule.  Used with PCAL = off
    **** Warning  Only    16.00 MHz of    32.00 MHz in scheduled channels is within IFs.
   LO sum=   6665.52  6665.52  6665.52  6665.52  6669.52  6669.52  6669.52  6669.52
             6673.52  6673.52  6673.52  6673.52  6677.52  6677.52  6677.52  6677.52
   BBC fr=    155.52   155.52   155.52   155.52   159.52   159.52   159.52   159.52
              163.52   163.52   163.52   163.52   167.52   167.52   167.52   167.52
   Bandwd=      2.00     2.00     2.00     2.00     2.00     2.00     2.00     2.00
                2.00     2.00     2.00     2.00     2.00     2.00     2.00     2.00
    Matching frequency sets:  10

   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)

 * G25.65+1.05       18 31 40.145161   * 18 34 20.900000     18 35 17.910134       0.00
                    -06 02 05.96283    *-05 59 42.10000     -05 58 47.97160        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         41.60    41.60    41.60    41.60    41.60    41.60    41.60    41.60
                         41.60    41.60    41.60    41.60    41.60    41.60

   3C286             13 28 49.657758   * 13 31 08.288051     13 31 58.829871       0.18
 * J1331+3030        30 45 58.64059    * 30 30 32.95924      30 24 50.75498        0.17
   1328+307          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1331+30          GSFC 2015a astro solution, unpublished    225 observations.
                     Doppler based on other sources.

 * 3C345             16 41 17.606228   * 16 42 58.809966     16 43 34.977099       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 46 26.14472        0.52
   1641+399          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1642+39          GSFC 2015a astro solution, unpublished  53430 observations.
                     Doppler based on other sources.

   1818-050          18 18 32.138835   * 18 21 11.809558     18 22 08.506188       0.32
 * J1821-0502       -05 03 46.86946    *-05 02 20.08539     -05 01 46.63323        0.52
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished    107 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362505   * 22 02 43.291372     22 03 26.389058       0.00
 * J2202+4216        42 02 08.59077    * 42 16 39.97990      42 21 48.66404        0.00
   BLLAC             /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   2200+420          GSFC 2015a astro solution, unpublished  51226 observations.
   J2202+42          Doppler based on other sources.



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
  G25.65+1.05sess118.M128          1 2 3 4 5 6 7 8 9 10              1.900    66.385
  J1331+3030 sess118.M128          1 2 3 4 5 6 7 8 9 10              0.217     9.750
  3C345      sess118.M128          1 2 3 4 5 6 7 8 9 10              0.167     7.424
  J1821-0502 sess118.M128          1 2 3 4 5 6 7 8 9 10              3.319   135.126
  J2202+4216 sess118.M128          1 2 3 4 5 6 7 8 9 10              1.461    52.704


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) 
   G25.65+1.05         64.7
   J1331+3030         136.5
   3C345               96.7
   J1821-0502          68.1
   J2202+4216          50.6

  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 

