  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
 Exp. Code:  EM117P  


Schedule Version:       2.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

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 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

 Next scan frequencies:  6661.54  6661.54  6661.54  6661.54  6665.54  6665.54  6665.54  6665.54
                         6669.54  6669.54  6669.54  6669.54  6673.54  6673.54  6673.54  6673.54
 Next BBC frequencies:    151.54   151.54   151.54   151.54   155.54   155.54   155.54   155.54
                          159.54   159.54   159.54   159.54   163.54   163.54   163.54   163.54
 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 15 35  J1331+3030   15 11 20  28.9 335.6  1.7       0.0     0        0   02 15 35
02 20 35  =3C286       15 16 21  28.4 334.5  1.7       0.0   300        5   02 15 36

02 21 05  J1331+3030   15 16 51  28.4 334.4  1.7       0.0     9        5   02 21 05
02 31 05  =3C286       15 26 53  27.4 332.2  1.9       0.0   600       14   02 21 06

02 35 51  3C345        15 31 40  22.2  14.9 -1.2       0.0   164       14   02 35 51
02 43 51  ---          15 39 41  22.7  13.3 -1.1       0.0   480       22   02 35 52

03 00 31  J1821-0502   15 56 24  49.4  65.4 -2.4       0.0   883       22   03 00 31
03 05 31  =1818-050    16 01 24  50.4  64.3 -2.3       0.0   300       27   03 00 32

03 05 31  G25.65+1.05  16 01 24  48.2  68.3 -2.6       0.0   -33       27   No stop 
03 07 31  ---          16 03 25  48.6  67.9 -2.5       0.0    87       29   03 05 32

03 08 16  J1821-0502   16 04 10  51.0  63.7 -2.3       0.0    11       29   03 08 16
03 11 06  =1818-050    16 07 00  51.5  63.0 -2.3       0.0   170       32   03 08 17

03 11 06  G25.65+1.05  16 07 00  49.4  67.2 -2.5       0.0   -33       32   No stop 
03 13 06  ---          16 09 01  49.8  66.7 -2.4       0.0    87       34   03 11 07

03 13 06  J1821-0502   16 09 01  51.9  62.5 -2.2       0.0   -34       34   No stop 
03 16 06  =1818-050    16 12 01  52.5  61.8 -2.2       0.0   146       37   03 13 07

03 16 06  G25.65+1.05  16 12 01  50.4  66.1 -2.4       0.0   -33       37   No stop 
03 18 06  ---          16 14 01  50.8  65.6 -2.4       0.0    87       38   03 16 07

03 18 51  J1821-0502   16 14 47  53.1  61.1 -2.1       0.0    11       38   03 18 51
03 21 41  =1818-050    16 17 37  53.6  60.4 -2.1       0.0   170       41   03 18 52

03 21 41  G25.65+1.05  16 17 37  51.6  64.8 -2.3       0.0   -33       41   No stop 
03 23 41  ---          16 19 37  52.0  64.4 -2.3       0.0    87       43   03 21 42

03 23 41  J1821-0502   16 19 37  54.0  59.8 -2.0       0.0   -34       43   No stop 
03 26 41  =1818-050    16 22 38  54.6  59.0 -2.0       0.0   146       46   03 23 42

03 26 41  G25.65+1.05  16 22 38  52.6  63.7 -2.2       0.0   -33       46   No stop 
03 28 41  ---          16 24 38  53.0  63.2 -2.2       0.0    87       48   03 26 42
Schedule for HART      (Code Hh )                                   Page   3
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

03 28 41  J1821-0502   16 24 38  55.0  58.5 -2.0       0.0   -34       48   No stop 
03 31 41  =1818-050    16 27 39  55.6  57.6 -1.9       0.0   146       51   03 28 42

03 31 41  G25.65+1.05  16 27 39  53.6  62.4 -2.1       0.0   -33       51   No stop 
03 33 41  ---          16 29 39  54.0  61.9 -2.1       0.0    87       53   03 31 42

03 34 26  J1821-0502   16 30 24  56.1  56.8 -1.9       0.0    11       53   03 34 26
03 37 16  =1818-050    16 33 15  56.6  56.0 -1.8       0.0   170       56   03 34 27

03 37 16  G25.65+1.05  16 33 15  54.7  61.0 -2.0       0.0   -33       56   No stop 
03 39 16  ---          16 35 15  55.1  60.5 -2.0       0.0    87       57   03 37 17

03 39 16  J1821-0502   16 35 15  57.0  55.4 -1.8       0.0   -34       57   No stop 
03 42 16  =1818-050    16 38 15  57.5  54.4 -1.7       0.0   146       60   03 39 17

03 58 26  J1821-0502   16 54 28  60.4  48.9 -1.5       0.0   948       60   03 58 26
04 01 26  =1818-050    16 57 29  60.9  47.8 -1.4       0.0   180       63   03 58 27

04 01 26  G25.65+1.05  16 57 29  59.3  53.8 -1.6       0.0   -33       63   No stop 
04 03 26  ---          16 59 29  59.7  53.1 -1.6       0.0    87       65   04 01 27

04 03 26  J1821-0502   16 59 29  61.2  47.0 -1.4       0.0   -34       65   No stop 
04 06 26  =1818-050    17 02 29  61.7  45.8 -1.3       0.0   146       68   04 03 27

04 06 26  G25.65+1.05  17 02 29  60.2  52.1 -1.5       0.0   -33       68   No stop 
04 08 26  ---          17 04 30  60.5  51.4 -1.5       0.0    87       70   04 06 27

04 08 26  J1821-0502   17 04 30  62.1  45.0 -1.3       0.0   -34       70   No stop 
04 11 26  =1818-050    17 07 30  62.5  43.8 -1.2       0.0   146       73   04 08 27

04 11 26  G25.65+1.05  17 07 30  61.1  50.3 -1.5       0.0   -33       73   No stop 
04 13 26  ---          17 09 31  61.4  49.6 -1.4       0.0    87       75   04 11 27

04 14 11  J1821-0502   17 10 16  63.0  42.6 -1.2       0.0    11       75   04 14 11
04 17 01  =1818-050    17 13 06  63.4  41.3 -1.2       0.0   170       78   04 14 12

04 17 01  G25.65+1.05  17 13 06  62.0  48.2 -1.4       0.0   -33       78   No stop 
04 19 01  ---          17 15 06  62.4  47.4 -1.3       0.0    87       80   04 17 02

04 19 01  J1821-0502   17 15 06  63.7  40.4 -1.1       0.0   -34       80   No stop 
04 22 01  =1818-050    17 18 07  64.1  39.0 -1.1       0.0   146       82   04 19 02

04 22 01  G25.65+1.05  17 18 07  62.9  46.2 -1.3       0.0   -33       82   No stop 
04 24 01  ---          17 20 07  63.2  45.3 -1.3       0.0    87       84   04 22 02
Schedule for HART      (Code Hh )                                   Page   4
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

04 24 01  J1821-0502   17 20 07  64.4  38.1 -1.0       0.0   -34       84   No stop 
04 27 01  =1818-050    17 23 08  64.8  36.6 -1.0       0.0   146       87   04 24 02

04 27 01  G25.65+1.05  17 23 08  63.7  44.0 -1.2       0.0   -33       87   No stop 
04 29 01  ---          17 25 08  64.0  43.1 -1.2       0.0    87       89   04 27 02

04 29 46  J1821-0502   17 25 53  65.2  35.3 -0.9       0.0    11       89   04 29 46
04 32 36  =1818-050    17 28 44  65.5  33.8 -0.9       0.0   170       92   04 29 47

04 32 36  G25.65+1.05  17 28 44  64.5  41.5 -1.1       0.0   -33       92   No stop 
04 34 36  ---          17 30 44  64.8  40.6 -1.1       0.0    87       94   04 32 37

04 34 36  J1821-0502   17 30 44  65.8  32.8 -0.9       0.0   -34       94   No stop 
04 37 36  =1818-050    17 33 45  66.1  31.1 -0.8       0.0   146       97   04 34 37

04 54 16  J1821-0502   17 50 27  67.8  21.4 -0.5       0.0   978       97   04 54 16
04 57 16  =1818-050    17 53 28  68.0  19.5 -0.5       0.0   180      100   04 54 17

04 57 16  G25.65+1.05  17 53 28  67.7  28.5 -0.7       0.0   -33      100   No stop 
04 59 16  ---          17 55 28  67.9  27.3 -0.7       0.0    87      102   04 57 17

04 59 16  J1821-0502   17 55 28  68.2  18.2 -0.4       0.0   -34      102   No stop 
05 02 16  =1818-050    17 58 29  68.4  16.3 -0.4       0.0   146      105   04 59 17

05 02 16  G25.65+1.05  17 58 29  68.2  25.5 -0.6       0.0   -33      105   No stop 
05 04 16  ---          18 00 29  68.4  24.2 -0.6       0.0    87      106   05 02 17

05 04 16  J1821-0502   18 00 29  68.5  14.9 -0.4       0.0   -34      106   No stop 
05 07 16  =1818-050    18 03 29  68.7  12.9 -0.3       0.0   146      109   05 04 17

05 07 16  G25.65+1.05  18 03 29  68.7  22.3 -0.5       0.0   -33      109   No stop 
05 09 16  ---          18 05 30  68.8  21.0 -0.5       0.0    87      111   05 07 17

05 10 01  J1821-0502   18 06 15  68.8  11.1 -0.3       0.0    11      111   05 10 01
05 12 51  =1818-050    18 09 05  68.9   9.1 -0.2       0.0   170      114   05 10 02

05 12 51  G25.65+1.05  18 09 05  69.1  18.6 -0.4       0.0   -33      114   No stop 
05 14 51  ---          18 11 06  69.3  17.3 -0.4       0.0    87      116   05 12 52

05 14 51  J1821-0502   18 11 06  69.0   7.8 -0.2       0.0   -34      116   No stop 
05 17 51  =1818-050    18 14 06  69.0   5.7 -0.1       0.0   146      119   05 14 52

05 17 51  G25.65+1.05  18 14 06  69.5  15.2 -0.4       0.0   -33      119   No stop 
05 19 51  ---          18 16 06  69.6  13.9 -0.3       0.0    87      121   05 17 52
Schedule for HART      (Code Hh )                                   Page   5
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

05 19 51  J1821-0502   18 16 06  69.1   4.3 -0.1       0.0   -34      121   No stop 
05 22 51  =1818-050    18 19 07  69.1   2.2 -0.1       0.0   146      124   05 19 52

05 22 51  G25.65+1.05  18 19 07  69.7  11.8 -0.3       0.0   -33      124   No stop 
05 24 51  ---          18 21 07  69.8  10.3 -0.2       0.0    87      126   05 22 52

05 25 36  J1821-0502   18 21 52  69.1   0.3 -0.0       0.0    11      126   05 25 36
05 28 26  =1818-050    18 24 43  69.1 358.3  0.0       0.0   170      128   05 25 37

05 28 26  G25.65+1.05  18 24 43  69.9   7.8 -0.2       0.0   -33      128   No stop 
05 30 26  ---          18 26 43  70.0   6.3 -0.1       0.0    87      130   05 28 27

05 30 26  J1821-0502   18 26 43  69.1 356.9  0.1       0.0   -34      130   No stop 
05 33 26  =1818-050    18 29 44  69.1 354.8  0.1       0.0   146      133   05 30 27

05 50 36  J1821-0502   18 46 57  68.3 343.1  0.4       0.0  1008      133   05 50 36
05 53 36  =1818-050    18 49 57  68.1 341.2  0.5       0.0   180      136   05 50 37

05 53 36  G25.65+1.05  18 49 57  69.8 349.5  0.2       0.0   -33      136   No stop 
05 55 36  ---          18 51 57  69.7 348.1  0.3       0.0    87      138   05 53 37

05 55 36  J1821-0502   18 51 57  68.0 339.9  0.5       0.0   -34      138   No stop 
05 58 36  =1818-050    18 54 58  67.7 338.0  0.5       0.0   146      141   05 55 37

05 58 36  G25.65+1.05  18 54 58  69.5 346.0  0.3       0.0   -33      141   No stop 
06 00 36  ---          18 56 58  69.4 344.6  0.4       0.0    87      143   05 58 37

06 00 36  J1821-0502   18 56 58  67.5 336.8  0.6       0.0   -34      143   No stop 
06 03 36  =1818-050    18 59 59  67.3 335.0  0.6       0.0   146      146   06 00 37

06 03 36  G25.65+1.05  18 59 59  69.2 342.5  0.4       0.0   -33      146   No stop 
06 05 36  ---          19 01 59  69.1 341.2  0.4       0.0    87      148   06 03 37

06 06 21  J1821-0502   19 02 44  67.0 333.4  0.7       0.0    11      148   06 06 21
06 09 11  =1818-050    19 05 35  66.7 331.7  0.7       0.0   170      150   06 06 22

06 09 11  G25.65+1.05  19 05 35  68.8 338.8  0.5       0.0   -33      150   No stop 
06 11 11  ---          19 07 35  68.7 337.5  0.5       0.0    87      152   06 09 12

06 11 11  J1821-0502   19 07 35  66.5 330.6  0.8       0.0   -34      152   No stop 
06 14 11  =1818-050    19 10 35  66.1 328.9  0.8       0.0   146      155   06 11 12

06 14 11  G25.65+1.05  19 10 35  68.4 335.6  0.6       0.0   -33      155   No stop 
06 16 11  ---          19 12 36  68.2 334.4  0.6       0.0    87      157   06 14 12
Schedule for HART      (Code Hh )                                   Page   6
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

06 16 11  J1821-0502   19 12 36  65.9 327.9  0.8       0.0   -34      157   No stop 
06 19 11  =1818-050    19 15 36  65.5 326.3  0.9       0.0   146      160   06 16 12

06 19 11  G25.65+1.05  19 15 36  67.9 332.5  0.7       0.0   -33      160   No stop 
06 21 11  ---          19 17 37  67.7 331.3  0.7       0.0    87      162   06 19 12

06 21 56  J1821-0502   19 18 22  65.2 324.9  0.9       0.0    11      162   06 21 56
06 24 46  =1818-050    19 21 12  64.8 323.4  1.0       0.0   170      165   06 21 57

06 24 46  G25.65+1.05  19 21 12  67.3 329.3  0.8       0.0   -33      165   No stop 
06 26 46  ---          19 23 12  67.0 328.1  0.8       0.0    87      167   06 24 47

06 26 46  J1821-0502   19 23 12  64.5 322.5  1.0       0.0   -34      167   No stop 
06 29 46  =1818-050    19 26 13  64.1 321.0  1.1       0.0   146      170   06 26 47

06 34 36  J2202+4216   19 31 04  13.2  27.9 -2.5       0.0   153      170   06 34 36
06 42 36  =VR422201    19 39 05  14.0  26.7 -2.4       0.0   480      177   06 34 37

06 47 36  J1821-0502   19 44 06  61.4 313.3  1.4       0.0   161      177   06 47 36
06 50 36  =1818-050    19 47 06  60.9 312.2  1.4       0.0   180      180   06 47 37

06 50 36  G25.65+1.05  19 47 06  63.7 316.2  1.2       0.0   -33      180   No stop 
06 52 36  ---          19 49 07  63.4 315.4  1.2       0.0    87      182   06 50 37

06 52 36  J1821-0502   19 49 07  60.6 311.4  1.4       0.0   -34      182   No stop 
06 55 36  =1818-050    19 52 07  60.0 310.3  1.5       0.0   146      185   06 52 37

06 55 36  G25.65+1.05  19 52 07  62.9 314.1  1.3       0.0   -33      185   No stop 
06 57 36  ---          19 54 08  62.6 313.3  1.3       0.0    87      187   06 55 37

06 57 36  J1821-0502   19 54 08  59.7 309.6  1.5       0.0   -34      187   No stop 
07 00 36  =1818-050    19 57 08  59.2 308.5  1.6       0.0   146      190   06 57 37

07 00 36  G25.65+1.05  19 57 08  62.1 312.1  1.4       0.0   -33      190   No stop 
07 02 36  ---          19 59 08  61.8 311.3  1.4       0.0    87      192   07 00 37

07 03 21  J1821-0502   19 59 53  58.7 307.6  1.6       0.0    11      192   07 03 21
07 06 11  =1818-050    20 02 44  58.2 306.7  1.7       0.0   170      195   07 03 22

07 06 11  G25.65+1.05  20 02 44  61.2 309.9  1.5       0.0   -33      195   No stop 
07 08 11  ---          20 04 44  60.8 309.2  1.5       0.0    87      196   07 06 12

07 08 11  J1821-0502   20 04 44  57.8 306.0  1.7       0.0   -34      196   No stop 
07 11 11  =1818-050    20 07 45  57.3 305.1  1.8       0.0   146      199   07 08 12
Schedule for HART      (Code Hh )                                   Page   7
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

07 11 11  G25.65+1.05  20 07 45  60.3 308.1  1.5       0.0   -33      199   No stop 
07 13 11  ---          20 09 45  59.9 307.4  1.6       0.0    87      201   07 11 12

07 13 11  J1821-0502   20 09 45  56.9 304.5  1.8       0.0   -34      201   No stop 
07 16 11  =1818-050    20 12 46  56.3 303.6  1.8       0.0   146      204   07 13 12

07 16 11  G25.65+1.05  20 12 46  59.4 306.4  1.6       0.0   -33      204   No stop 
07 18 11  ---          20 14 46  59.0 305.7  1.7       0.0    87      206   07 16 12

07 18 56  J1821-0502   20 15 31  55.8 302.8  1.9       0.0    11      206   07 18 56
07 21 46  =1818-050    20 18 22  55.3 301.9  1.9       0.0   170      209   07 18 57

07 21 46  G25.65+1.05  20 18 22  58.4 304.6  1.7       0.0   -33      209   No stop 
07 23 46  ---          20 20 22  58.0 303.9  1.7       0.0    87      211   07 21 47

07 23 46  J1821-0502   20 20 22  54.9 301.4  2.0       0.0   -34      211   No stop 
07 26 46  =1818-050    20 23 22  54.3 300.6  2.0       0.0   146      214   07 23 47

07 31 56  J2202+4216   20 28 33  18.3  18.3 -1.6       0.0   173      214   07 31 56
07 39 56  =VR422201    20 36 34  18.9  16.8 -1.4       0.0   480      221   07 31 57

07 45 17  J1821-0502   20 41 56  50.6 296.0  2.3       0.0   182      221   07 45 17
07 48 17  =1818-050    20 44 57  50.0 295.3  2.4       0.0   180      224   07 45 18

07 48 17  G25.65+1.05  20 44 57  53.2 297.1  2.2       0.0   -33      224   No stop 
07 50 17  ---          20 46 57  52.8 296.6  2.2       0.0    87      226   07 48 18

07 50 17  J1821-0502   20 46 57  49.6 294.8  2.4       0.0   -34      226   No stop 
07 53 17  =1818-050    20 49 58  49.0 294.2  2.5       0.0   146      229   07 50 18

07 53 17  G25.65+1.05  20 49 58  52.2 295.9  2.2       0.0   -33      229   No stop 
07 55 17  ---          20 51 58  51.8 295.5  2.3       0.0    87      231   07 53 18

07 55 17  J1821-0502   20 51 58  48.6 293.8  2.5       0.0   -34      231   No stop 
07 58 17  =1818-050    20 54 59  48.0 293.1  2.5       0.0   146      234   07 55 18

07 58 17  G25.65+1.05  20 54 59  51.2 294.8  2.3       0.0   -33      234   No stop 
08 00 17  ---          20 56 59  50.8 294.3  2.4       0.0    87      236   07 58 18

08 01 02  J1821-0502   20 57 44  47.4 292.6  2.6       0.0    11      236   08 01 02
08 03 52  =1818-050    21 00 34  46.8 292.0  2.6       0.0   170      239   08 01 03

08 03 52  G25.65+1.05  21 00 34  50.1 293.5  2.4       0.0   -33      239   No stop 
08 05 52  ---          21 02 35  49.6 293.1  2.5       0.0    87      241   08 03 53
Schedule for HART      (Code Hh )                                   Page   8
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

08 05 52  J1821-0502   21 02 35  46.4 291.6  2.7       0.0   -34      241   No stop 
08 08 52  =1818-050    21 05 35  45.8 291.0  2.7       0.0   146      243   08 05 53

08 08 52  G25.65+1.05  21 05 35  49.0 292.5  2.5       0.0   -33      243   No stop 
08 10 52  ---          21 07 36  48.6 292.0  2.5       0.0    87      245   08 08 53

08 10 52  J1821-0502   21 07 36  45.3 290.6  2.8       0.0   -34      245   No stop 
08 13 52  =1818-050    21 10 36  44.7 290.1  2.8       0.0   146      248   08 10 53

08 13 52  G25.65+1.05  21 10 36  48.0 291.4  2.6       0.0   -33      248   No stop 
08 15 52  ---          21 12 36  47.6 291.0  2.6       0.0    87      250   08 13 53

08 16 37  J1821-0502   21 13 22  44.1 289.6  2.9       0.0    11      250   08 16 37
08 19 27  =1818-050    21 16 12  43.5 289.0  2.9       0.0   170      253   08 16 38

08 19 27  G25.65+1.05  21 16 12  46.8 290.3  2.7       0.0   -33      253   No stop 
08 21 27  ---          21 18 12  46.4 290.0  2.7       0.0    87      255   08 19 28

08 21 27  J1821-0502   21 18 12  43.1 288.7  2.9       0.0   -34      255   No stop 
08 24 27  =1818-050    21 21 13  42.4 288.2  3.0       0.0   146      258   08 21 28

08 29 52  J2202+4216   21 26 39  21.2   7.3 -0.6       0.0   188      258   08 29 52
08 37 52  =VR422201    21 34 40  21.4   5.7 -0.5       0.0   480      266   08 29 53

08 43 27  J1821-0502   21 40 16  38.3 285.0  3.3       0.0   196      266   08 43 27
08 46 27  =1818-050    21 43 16  37.7 284.6  3.4       0.0   180      268   08 43 28

08 46 27  G25.65+1.05  21 43 16  41.0 285.6  3.1       0.0   -33      268   No stop 
08 48 27  ---          21 45 17  40.6 285.3  3.2       0.0    87      270   08 46 28

08 48 27  J1821-0502   21 45 17  37.2 284.3  3.4       0.0   -34      270   No stop 
08 51 27  =1818-050    21 48 17  36.6 283.8  3.4       0.0   146      273   08 48 28

08 51 27  G25.65+1.05  21 48 17  39.9 284.8  3.2       0.0   -33      273   No stop 
08 53 27  ---          21 50 18  39.5 284.5  3.2       0.0    87      275   08 51 28

08 53 27  J1821-0502   21 50 18  36.1 283.5  3.5       0.0   -34      275   No stop 
08 56 27  =1818-050    21 53 18  35.5 283.1  3.5       0.0   146      278   08 53 28

08 56 27  G25.65+1.05  21 53 18  38.8 284.0  3.3       0.0   -33      278   No stop 
08 58 27  ---          21 55 18  38.4 283.7  3.3       0.0    87      280   08 56 28

08 59 12  J1821-0502   21 56 04  34.9 282.7  3.6       0.0    11      280   08 59 12
09 02 02  =1818-050    21 58 54  34.3 282.3  3.6       0.0   170      283   08 59 13
Schedule for HART      (Code Hh )                                   Page   9
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

09 02 02  G25.65+1.05  21 58 54  37.6 283.2  3.4       0.0   -33      283   No stop 
09 04 02  ---          22 00 54  37.2 282.9  3.4       0.0    87      285   09 02 03

09 04 02  J1821-0502   22 00 54  33.8 282.0  3.6       0.0   -34      285   No stop 
09 07 02  =1818-050    22 03 55  33.2 281.6  3.7       0.0   146      288   09 04 03

09 07 02  G25.65+1.05  22 03 55  36.5 282.4  3.5       0.0   -33      288   No stop 
09 09 02  ---          22 05 55  36.1 282.1  3.5       0.0    87      290   09 07 03

09 09 02  J1821-0502   22 05 55  32.7 281.3  3.7       0.0   -34      290   No stop 
09 12 02  =1818-050    22 08 56  32.1 280.9  3.8       0.0   146      292   09 09 03

09 12 02  G25.65+1.05  22 08 56  35.4 281.7  3.6       0.0   -33      292   No stop 
09 14 02  ---          22 10 56  35.0 281.4  3.6       0.0    87      294   09 12 03

09 14 47  J1821-0502   22 11 41  31.4 280.5  3.8       0.0    11      294   09 14 47
09 17 37  =1818-050    22 14 32  30.8 280.1  3.9       0.0   170      297   09 14 48

09 17 37  G25.65+1.05  22 14 32  34.2 280.9  3.7       0.0   -33      297   No stop 
09 19 37  ---          22 16 32  33.7 280.6  3.7       0.0    87      299   09 17 38

09 19 37  J1821-0502   22 16 32  30.4 279.9  3.9       0.0   -34      299   No stop 
09 22 37  =1818-050    22 19 32  29.7 279.5  4.0       0.0   146      302   09 19 38

09 27 58  J2202+4216   22 24 54  21.6 355.8  0.4       0.0   184      302   09 27 58
09 35 58  =VR422201    22 32 56  21.4 354.2  0.5       0.0   480      310   09 27 59

09 41 28  J1821-0502   22 38 26  25.5 277.1  4.3       0.0   191      310   09 41 28
09 44 28  =1818-050    22 41 27  24.8 276.7  4.3       0.0   180      313   09 41 29

09 44 28  G25.65+1.05  22 41 27  28.2 277.4  4.1       0.0   -33      313   No stop 
09 46 28  ---          22 43 27  27.7 277.1  4.1       0.0    87      314   09 44 29

09 46 28  J1821-0502   22 43 27  24.4 276.5  4.4       0.0   -34      314   No stop 
09 49 28  =1818-050    22 46 28  23.7 276.1  4.4       0.0   146      317   09 46 29

09 49 28  G25.65+1.05  22 46 28  27.1 276.8  4.2       0.0   -33      317   No stop 
09 51 28  ---          22 48 28  26.6 276.5  4.2       0.0    87      319   09 49 29

09 51 28  J1821-0502   22 48 28  23.3 275.9  4.4       0.0   -34      319   No stop 
09 54 28  =1818-050    22 51 29  22.6 275.5  4.5       0.0   146      322   09 51 29

09 54 28  G25.65+1.05  22 51 29  25.9 276.2  4.3       0.0   -33      322   No stop 
09 56 28  ---          22 53 29  25.5 275.9  4.3       0.0    87      324   09 54 29
Schedule for HART      (Code Hh )                                   Page  10
               A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
  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   8 Mar 2020   Day  68 ---

09 57 13  J1821-0502   22 54 14  22.0 275.2  4.5       0.0    11      324   09 57 13
10 00 03  =1818-050    22 57 05  21.3 274.9  4.6       0.0   170      327   09 57 14

10 00 03  G25.65+1.05  22 57 05  24.7 275.5  4.4       0.0   -33      327   No stop 
10 02 03  ---          22 59 05  24.2 275.3  4.4       0.0    87      329   10 00 04

10 02 03  J1821-0502   22 59 05  20.9 274.6  4.6       0.0   -34      329   No stop 
10 05 03  =1818-050    23 02 05  20.2 274.3  4.7       0.0   146      332   10 02 04

10 05 03  G25.65+1.05  23 02 05  23.6 274.9  4.4       0.0   -33      332   No stop 
10 07 03  ---          23 04 06  23.1 274.7  4.5       0.0    87      334   10 05 04

10 07 03  J1821-0502   23 04 06  19.8 274.1  4.7       0.0   -34      334   No stop 
10 10 03  =1818-050    23 07 06  19.1 273.7  4.7       0.0   146      337   10 07 04

10 10 03  G25.65+1.05  23 07 06  22.4 274.3  4.5       0.0   -33      337   No stop 
10 12 03  ---          23 09 06  22.0 274.1  4.6       0.0    87      338   10 10 04

10 12 48  J1821-0502   23 09 52  18.5 273.4  4.8       0.0    11      338   10 12 48
10 15 38  =1818-050    23 12 42  17.8 273.1  4.8       0.0   170      341   10 12 49

10 15 38  G25.65+1.05  23 12 42  21.2 273.7  4.6       0.0   -33      341   No stop 
10 17 38  ---          23 14 42  20.7 273.4  4.7       0.0    87      343   10 15 39

10 17 38  J1821-0502   23 14 42  17.4 272.8  4.9       0.0   -34      343   No stop 
10 20 38  =1818-050    23 17 43  16.7 272.5  4.9       0.0   146      346   10 17 39

10 25 23  J2202+4216   23 22 29  19.3 344.7  1.3       0.0   148      346   10 25 23
10 32 23  =VR422201    23 29 30  18.9 343.4  1.4       0.0   420      353   10 25 24

10 37 18  J1821-0502   23 34 26  12.9 270.7  5.2       0.0   156      353   10 37 18
10 40 18  =1818-050    23 37 26  12.3 270.3  5.3       0.0   180      356   10 37 19

10 40 18  G25.65+1.05  23 37 26  15.6 270.9  5.0       0.0   -33      356   No stop 
10 42 18  ---          23 39 26  15.2 270.7  5.1       0.0    87      358   10 40 19

10 42 43  J1821-0502   23 39 52  11.7 270.1  5.3       0.0    -9      358   10 42 43
10 47 43  =1818-050    23 44 52  10.6 269.5  5.4       0.0   291      362   10 42 44

10 52 39  J2202+4216   23 49 49  17.5 339.7  1.8       0.0   159      362   10 52 39
10 59 59  =VR422201    23 57 10  16.9 338.4  1.9       0.0   440      370   10 52 40


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


 ======== Setup file: sess120.M128
   Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq_RDBE.dat:
     hh5cm           Values confirmed by E-mail Jonathan Quick 20170808 (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:   9  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=   6661.54  6661.54  6661.54  6661.54  6665.54  6665.54  6665.54  6665.54
             6669.54  6669.54  6669.54  6669.54  6673.54  6673.54  6673.54  6673.54
   BBC fr=    151.54   151.54   151.54   151.54   155.54   155.54   155.54   155.54
              159.54   159.54   159.54   159.54   163.54   163.54   163.54   163.54
   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:   9

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8,  9, 10, 11, 12, 13, 14, 15, 16
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

   Source                         Source position (RA/Dec)                        Error
                        (B1950)             (J2000)             (Date)            (mas)

 * G25.65+1.05       18 31 40.145161   * 18 34 20.900000     18 35 24.212719       0.00
                    -06 02 05.96283    *-05 59 42.10000     -05 58 47.77192        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 49.657769   * 13 31 08.288061     13 32 04.445364       0.17
 * J1331+3030        30 45 58.64066    * 30 30 32.95930      30 24 13.70356        0.16
   1328+307          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J1331+30          GSFC 2016a X/S astro solution,    269 observations.
                     Doppler based on other sources.

 * 3C345             16 41 17.606229   * 16 42 58.809967     16 43 39.138831       0.79
   J1642+3948        39 54 10.81492    * 39 48 36.99399      39 46 08.15073        0.59
   1641+399          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J1642+39          GSFC 2016a X/S astro solution,  53724 observations.
                     Doppler based on other sources.

   1818-050          18 18 32.138842   * 18 21 11.809566     18 22 14.767578       0.13
 * J1821-0502       -05 03 46.86951    *-05 02 20.08544     -05 01 48.68974        0.24
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    107 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362504   * 22 02 43.291371     22 03 30.904400       0.01
 * J2202+4216        42 02 08.59075    * 42 16 39.97988      42 22 18.13421        0.00
   BLLAC             /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   2200+420          GSFC 2016a X/S astro solution,  52189 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+1.05sess120.M128          1 2 3 4 5 6 7 8 9                 1.900    50.691
  J1331+3030 sess120.M128          1 2 3 4 5 6 7 8 9                 0.250     9.000
  3C345      sess120.M128          1 2 3 4 5 6 7 8 9                 0.133     4.800
  J1821-0502 sess120.M128          1 2 3 4 5 6 7 8 9                 3.319   105.877
  J2202+4216 sess120.M128          1 2 3 4 5 6 7 8 9                 1.439    40.465


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         69.9
   J1331+3030         139.0
   3C345               99.3
   J1821-0502          73.2
   J2202+4216          49.9

  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 

