  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3D View of high-mass star formation: gas Kinematics and Magnetic Field
 Exp. Code:  EM117O  


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 = G012.68-0.18
 
 

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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

 Next scan frequencies:  6661.17  6661.17  6661.17  6661.17  6665.17  6665.17  6665.17  6665.17
                         6669.17  6669.17  6669.17  6669.17  6673.17  6673.17  6673.17  6673.17
 Next BBC frequencies:    151.17   151.17   151.17   151.17   155.17   155.17   155.17   155.17
                          159.17   159.17   159.17   159.17   163.17   163.17   163.17   163.17
 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 00 00  J1331+3030   14 51 46  30.6 340.0  1.3       0.0     0        0   02 00 00
02 10 00  =3C286       15 01 48  29.8 337.7  1.5       0.0   600       10   02 00 01

02 10 30  J1331+3030   15 02 18  29.7 337.6  1.5       0.0     9       10   02 10 30
02 20 30  =3C286       15 12 19  28.8 335.4  1.7       0.0   600       19   02 10 31

02 24 50  3C345        15 16 40  21.3  17.8 -1.4       0.0   138       19   02 24 50
02 34 50  ---          15 26 42  21.9  15.8 -1.3       0.0   600       29   02 24 51

02 35 20  3C345        15 27 12  22.0  15.7 -1.3       0.0     9       29   02 35 20
02 45 20  ---          15 37 14  22.5  13.8 -1.1       0.0   600       39   02 35 21

02 50 20  J1331+3030   15 42 14  25.7 329.0  2.2       0.0   176       39   02 50 20
03 00 20  =3C286       15 52 16  24.5 327.0  2.3       0.0   600       48   02 50 21

03 04 50  J1832-2039   15 56 47  53.8  90.0 -2.6       0.0    94       48   03 04 50
03 09 50  =1829-207    16 01 48  54.9  89.5 -2.5       0.0   300       53   03 04 51

03 09 50 G012.68-0.18  16 01 48  58.2  82.5 -2.2       0.0   -36       53   No stop 
03 11 50  ---          16 03 48  58.7  82.2 -2.2       0.0    84       55   03 09 51

03 12 35  J1832-2039   16 04 33  55.5  89.2 -2.5       0.0     9       55   03 12 35
03 15 30  =1829-207    16 07 29  56.2  88.8 -2.4       0.0   175       58   03 12 36

03 15 30 G012.68-0.18  16 07 29  59.5  81.6 -2.1       0.0   -36       58   No stop 
03 17 30  ---          16 09 29  59.9  81.3 -2.1       0.0    84       60   03 15 31

03 17 30  J1832-2039   16 09 29  56.6  88.6 -2.4       0.0   -36       60   No stop 
03 20 30  =1829-207    16 12 29  57.3  88.2 -2.3       0.0   144       63   03 17 31

03 20 30 G012.68-0.18  16 12 29  60.6  80.8 -2.0       0.0   -36       63   No stop 
03 22 30  ---          16 14 30  61.0  80.4 -2.0       0.0    84       65   03 20 31

03 23 15  J1832-2039   16 15 15  57.9  87.9 -2.3       0.0     9       65   03 23 15
03 26 10  =1829-207    16 18 10  58.6  87.5 -2.3       0.0   175       67   03 23 16

03 26 10 G012.68-0.18  16 18 10  61.8  79.7 -1.9       0.0   -36       67   No stop 
03 28 10  ---          16 20 11  62.3  79.4 -1.9       0.0    84       69   03 26 11
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

03 28 10  J1832-2039   16 20 11  59.1  87.3 -2.2       0.0   -36       69   No stop 
03 31 10  =1829-207    16 23 11  59.7  86.9 -2.2       0.0   144       72   03 28 11

03 31 10 G012.68-0.18  16 23 11  63.0  78.8 -1.9       0.0   -36       72   No stop 
03 33 10  ---          16 25 11  63.4  78.4 -1.8       0.0    84       74   03 31 11

03 33 10  J1832-2039   16 25 11  60.2  86.6 -2.1       0.0   -36       74   No stop 
03 36 10  =1829-207    16 28 12  60.9  86.2 -2.1       0.0   144       77   03 33 11

03 36 10 G012.68-0.18  16 28 12  64.1  77.8 -1.8       0.0   -36       77   No stop 
03 38 10  ---          16 30 12  64.5  77.4 -1.7       0.0    84       79   03 36 11

03 38 55  J1832-2039   16 30 57  61.5  85.9 -2.0       0.0     9       79   03 38 55
03 41 50  =1829-207    16 33 53  62.1  85.5 -2.0       0.0   175       82   03 38 56

03 41 50 G012.68-0.18  16 33 53  65.3  76.6 -1.7       0.0   -36       82   No stop 
03 43 50  ---          16 35 53  65.7  76.1 -1.7       0.0    84       84   03 41 51

03 43 50  J1832-2039   16 35 53  62.6  85.2 -2.0       0.0   -36       84   No stop 
03 46 50  =1829-207    16 38 54  63.3  84.7 -1.9       0.0   144       87   03 43 51

03 51 20  J1331+3030   16 43 24  17.5 317.9  3.2       0.0    91       87   03 51 20
04 01 20  =3C286       16 53 26  15.9 316.3  3.4       0.0   600       96   03 51 21

04 29 30  J1832-2039   17 21 41  72.7  76.0 -1.2       0.0  1514       96   04 29 30
04 32 30  =1829-207    17 24 41  73.4  75.2 -1.1       0.0   180       99   04 29 31

04 32 30 G012.68-0.18  17 24 41  75.9  58.5 -0.8       0.0   -36       99   No stop 
04 34 30  ---          17 26 41  76.3  57.4 -0.8       0.0    84      101   04 32 31

04 34 30  J1832-2039   17 26 41  73.8  74.5 -1.1       0.0   -36      101   No stop 
04 37 30  =1829-207    17 29 42  74.5  73.6 -1.1       0.0   144      104   04 34 31

04 37 30 G012.68-0.18  17 29 42  76.9  55.5 -0.8       0.0   -36      104   No stop 
04 39 30  ---          17 31 42  77.2  54.1 -0.7       0.0    84      106   04 37 31

04 39 30  J1832-2039   17 31 42  74.9  72.9 -1.0       0.0   -36      106   No stop 
04 42 30  =1829-207    17 34 43  75.6  71.8 -1.0       0.0   144      109   04 39 31

04 42 30 G012.68-0.18  17 34 43  77.8  51.9 -0.7       0.0   -36      109   No stop 
04 44 30  ---          17 36 43  78.1  50.4 -0.6       0.0    84      111   04 42 31

04 45 15  J1832-2039   17 37 28  76.1  70.7 -0.9       0.0     9      111   04 45 15
04 48 10  =1829-207    17 40 24  76.8  69.4 -0.9       0.0   175      114   04 45 16
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

04 48 10 G012.68-0.18  17 40 24  78.8  47.3 -0.6       0.0   -36      114   No stop 
04 50 10  ---          17 42 24  79.1  45.5 -0.5       0.0    84      116   04 48 11

04 50 10  J1832-2039   17 42 24  77.2  68.5 -0.8       0.0   -36      116   No stop 
04 53 10  =1829-207    17 45 25  77.8  67.0 -0.8       0.0   144      119   04 50 11

05 11 55  J1832-2039   18 04 13  81.5  53.4 -0.5       0.0  1103      119   05 11 55
05 14 55  =1829-207    18 07 13  82.0  50.2 -0.4       0.0   180      121   05 11 56

05 14 55 G012.68-0.18  18 07 13  81.9  13.4 -0.1       0.0   -36      121   No stop 
05 16 55  ---          18 09 13  82.0  10.1 -0.1       0.0    84      123   05 14 56

05 16 55  J1832-2039   18 09 13  82.4  47.8 -0.4       0.0   -36      123   No stop 
05 19 55  =1829-207    18 12 14  82.9  43.9 -0.4       0.0   144      126   05 16 56

05 19 55 G012.68-0.18  18 12 14  82.1   4.9 -0.0       0.0   -36      126   No stop 
05 21 55  ---          18 14 14  82.1   1.4 -0.0       0.0    84      128   05 19 56

05 21 55  J1832-2039   18 14 14  83.2  40.9 -0.3       0.0   -36      128   No stop 
05 24 55  =1829-207    18 17 15  83.6  36.0 -0.3       0.0   144      131   05 21 56

05 24 55 G012.68-0.18  18 17 15  82.1 356.2  0.0       0.0   -36      131   No stop 
05 26 55  ---          18 19 15  82.1 352.8  0.1       0.0    84      133   05 24 56

05 27 40  J1832-2039   18 20 00  83.9  31.0 -0.2       0.0     9      133   05 27 40
05 30 35  =1829-207    18 22 56  84.2  25.1 -0.2       0.0   175      136   05 27 41

05 30 35 G012.68-0.18  18 22 56  81.9 346.6  0.1       0.0   -36      136   No stop 
05 32 35  ---          18 24 56  81.8 343.3  0.2       0.0    84      138   05 30 36

05 32 35  J1832-2039   18 24 56  84.4  20.7 -0.1       0.0   -36      138   No stop 
05 35 35  =1829-207    18 27 57  84.6  13.6 -0.1       0.0   144      141   05 32 36

05 35 35 G012.68-0.18  18 27 57  81.6 338.6  0.2       0.0   -36      141   No stop 
05 37 35  ---          18 29 57  81.4 335.6  0.2       0.0    84      143   05 35 36

05 37 35  J1832-2039   18 29 57  84.7   8.7 -0.1       0.0   -36      143   No stop 
05 40 35  =1829-207    18 32 57  84.8   1.0 -0.0       0.0   144      145   05 37 36

05 40 35 G012.68-0.18  18 32 57  81.1 331.3  0.3       0.0   -36      145   No stop 
05 42 35  ---          18 34 58  80.9 328.6  0.3       0.0    84      147   05 40 36

05 43 20  J1832-2039   18 35 43  84.7 354.0  0.0       0.0     9      147   05 43 20
05 46 15  =1829-207    18 38 38  84.6 346.7  0.1       0.0   175      150   05 43 21
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

05 46 15 G012.68-0.18  18 38 38  80.4 324.1  0.4       0.0   -36      150   No stop 
05 48 15  ---          18 40 39  80.2 321.7  0.4       0.0    84      152   05 46 16

05 48 15  J1832-2039   18 40 39  84.5 341.9  0.1       0.0   -36      152   No stop 
05 51 15  =1829-207    18 43 39  84.3 335.2  0.2       0.0   144      155   05 48 16

05 51 15 G012.68-0.18  18 43 39  79.7 318.5  0.5       0.0   -36      155   No stop 
05 53 15  ---          18 45 39  79.4 316.5  0.5       0.0    84      157   05 51 16

05 53 15  J1832-2039   18 45 39  84.0 331.1  0.2       0.0   -36      157   No stop 
05 56 15  =1829-207    18 48 40  83.7 325.4  0.3       0.0   144      160   05 53 16

05 56 15 G012.68-0.18  18 48 40  78.9 313.6  0.6       0.0   -36      160   No stop 
05 58 15  ---          18 50 40  78.6 311.9  0.6       0.0    84      162   05 56 16

05 59 00  J1832-2039   18 51 25  83.3 320.7  0.3       0.0     9      162   05 59 00
06 01 55  =1829-207    18 54 21  82.9 316.3  0.3       0.0   175      165   05 59 01

06 20 55  J1832-2039   19 13 24  79.4 297.6  0.7       0.0  1118      165   06 20 55
06 23 55  =1829-207    19 16 24  78.8 295.7  0.7       0.0   180      168   06 20 56

06 23 55 G012.68-0.18  19 16 24  73.8 295.9  1.0       0.0   -36      168   No stop 
06 25 55  ---          19 18 25  73.4 295.0  1.1       0.0    84      169   06 23 56

06 25 55  J1832-2039   19 18 25  78.4 294.5  0.8       0.0   -36      169   No stop 
06 28 55  =1829-207    19 21 25  77.8 292.9  0.8       0.0   144      172   06 25 56

06 28 55 G012.68-0.18  19 21 25  72.7 293.8  1.1       0.0   -36      172   No stop 
06 30 55  ---          19 23 26  72.3 293.0  1.1       0.0    84      174   06 28 56

06 30 55  J1832-2039   19 23 26  77.4 291.9  0.8       0.0   -36      174   No stop 
06 33 55  =1829-207    19 26 26  76.7 290.5  0.9       0.0   144      177   06 30 56

06 33 55 G012.68-0.18  19 26 26  71.7 291.9  1.2       0.0   -36      177   No stop 
06 35 55  ---          19 28 26  71.3 291.1  1.2       0.0    84      179   06 33 56

06 36 40  J1832-2039   19 29 12  76.2 289.4  0.9       0.0     9      179   06 36 40
06 39 35  =1829-207    19 32 07  75.5 288.2  1.0       0.0   175      182   06 36 41

06 39 35 G012.68-0.18  19 32 07  70.5 289.9  1.3       0.0   -36      182   No stop 
06 41 35  ---          19 34 07  70.1 289.3  1.3       0.0    84      184   06 39 36

06 41 35  J1832-2039   19 34 07  75.1 287.5  1.0       0.0   -36      184   No stop 
06 44 35  =1829-207    19 37 08  74.5 286.4  1.1       0.0   144      187   06 41 36
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

06 44 35 G012.68-0.18  19 37 08  69.4 288.3  1.4       0.0   -36      187   No stop 
06 46 35  ---          19 39 08  69.0 287.8  1.4       0.0    84      189   06 44 36

06 46 35  J1832-2039   19 39 08  74.0 285.7  1.1       0.0   -36      189   No stop 
06 49 35  =1829-207    19 42 09  73.4 284.8  1.1       0.0   144      192   06 46 36

06 49 35 G012.68-0.18  19 42 09  68.4 286.9  1.5       0.0   -36      192   No stop 
06 51 35  ---          19 44 09  67.9 286.4  1.5       0.0    84      194   06 49 36

06 52 20  J1832-2039   19 44 54  72.8 284.0  1.2       0.0     9      194   06 52 20
06 55 15  =1829-207    19 47 50  72.1 283.2  1.2       0.0   175      196   06 52 21

06 55 15 G012.68-0.18  19 47 50  67.1 285.4  1.5       0.0   -36      196   No stop 
06 57 15  ---          19 49 50  66.7 284.9  1.6       0.0    84      198   06 55 16

06 57 15  J1832-2039   19 49 50  71.7 282.7  1.3       0.0   -36      198   No stop 
07 00 15  =1829-207    19 52 50  71.0 281.9  1.3       0.0   144      201   06 57 16

07 00 15 G012.68-0.18  19 52 50  66.1 284.2  1.6       0.0   -36      201   No stop 
07 02 15  ---          19 54 51  65.6 283.7  1.7       0.0    84      203   07 00 16

07 02 15  J1832-2039   19 54 51  70.6 281.4  1.4       0.0   -36      203   No stop 
07 05 15  =1829-207    19 57 51  69.9 280.7  1.4       0.0   144      206   07 02 16

07 24 05  J1832-2039   20 16 44  65.7 277.1  1.7       0.0  1108      206   07 24 05
07 27 05  =1829-207    20 19 45  65.1 276.6  1.8       0.0   180      209   07 24 06

07 27 05 G012.68-0.18  20 19 45  60.1 278.9  2.1       0.0   -36      209   No stop 
07 29 05  ---          20 21 45  59.7 278.5  2.1       0.0    84      211   07 27 06

07 29 05  J1832-2039   20 21 45  64.6 276.2  1.8       0.0   -36      211   No stop 
07 32 05  =1829-207    20 24 46  63.9 275.8  1.9       0.0   144      214   07 29 06

07 32 05 G012.68-0.18  20 24 46  59.0 278.1  2.2       0.0   -36      214   No stop 
07 34 05  ---          20 26 46  58.6 277.7  2.2       0.0    84      216   07 32 06

07 34 05  J1832-2039   20 26 46  63.5 275.4  1.9       0.0   -36      216   No stop 
07 37 05  =1829-207    20 29 46  62.8 275.0  1.9       0.0   144      219   07 34 06

07 37 05 G012.68-0.18  20 29 46  57.9 277.3  2.2       0.0   -36      219   No stop 
07 39 05  ---          20 31 47  57.4 277.0  2.3       0.0    84      221   07 37 06

07 39 50  J1832-2039   20 32 32  62.2 274.6  2.0       0.0     9      221   07 39 50
07 42 45  =1829-207    20 35 27  61.5 274.2  2.0       0.0   175      223   07 39 51
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

07 42 45 G012.68-0.18  20 35 27  56.6 276.4  2.3       0.0   -36      223   No stop 
07 44 45  ---          20 37 28  56.2 276.1  2.4       0.0    84      225   07 42 46

07 44 45  J1832-2039   20 37 28  61.1 273.9  2.1       0.0   -36      225   No stop 
07 47 45  =1829-207    20 40 28  60.4 273.5  2.1       0.0   144      228   07 44 46

07 47 45 G012.68-0.18  20 40 28  55.5 275.7  2.4       0.0   -36      228   No stop 
07 49 45  ---          20 42 29  55.0 275.4  2.5       0.0    84      230   07 47 46

07 49 45  J1832-2039   20 42 29  60.0 273.2  2.2       0.0   -36      230   No stop 
07 52 45  =1829-207    20 45 29  59.3 272.8  2.2       0.0   144      233   07 49 46

07 52 45 G012.68-0.18  20 45 29  54.4 275.0  2.5       0.0   -36      233   No stop 
07 54 45  ---          20 47 29  53.9 274.7  2.5       0.0    84      235   07 52 46

07 55 30  J1832-2039   20 48 14  58.7 272.5  2.2       0.0     9      235   07 55 30
07 58 25  =1829-207    20 51 10  58.0 272.1  2.3       0.0   175      238   07 55 31

07 58 25 G012.68-0.18  20 51 10  53.1 274.2  2.6       0.0   -36      238   No stop 
08 00 25  ---          20 53 10  52.7 274.0  2.6       0.0    84      240   07 58 26

08 00 25  J1832-2039   20 53 10  57.6 271.9  2.3       0.0   -36      240   No stop 
08 03 25  =1829-207    20 56 11  56.9 271.5  2.4       0.0   144      243   08 00 26

08 03 25 G012.68-0.18  20 56 11  52.0 273.6  2.7       0.0   -36      243   No stop 
08 05 25  ---          20 58 11  51.5 273.3  2.7       0.0    84      245   08 03 26

08 06 10  J1832-2039   20 58 56  56.3 271.2  2.4       0.0     9      245   08 06 10
08 09 05  =1829-207    21 01 52  55.6 270.9  2.5       0.0   175      247   08 06 11

08 27 35  J1832-2039   21 20 25  51.4 268.9  2.8       0.0  1088      247   08 27 35
08 30 35  =1829-207    21 23 25  50.8 268.5  2.8       0.0   180      250   08 27 36

08 30 35 G012.68-0.18  21 23 25  45.9 270.4  3.1       0.0   -36      250   No stop 
08 32 35  ---          21 25 26  45.4 270.1  3.2       0.0    84      252   08 30 36

08 32 35  J1832-2039   21 25 26  50.3 268.3  2.9       0.0   -36      252   No stop 
08 35 35  =1829-207    21 28 26  49.6 268.0  2.9       0.0   144      255   08 32 36

08 35 35 G012.68-0.18  21 28 26  44.7 269.8  3.2       0.0   -36      255   No stop 
08 37 35  ---          21 30 26  44.3 269.6  3.3       0.0    84      257   08 35 36

08 37 35  J1832-2039   21 30 26  49.2 267.8  3.0       0.0   -36      257   No stop 
08 40 35  =1829-207    21 33 27  48.5 267.5  3.0       0.0   144      260   08 37 36
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

08 40 35 G012.68-0.18  21 33 27  43.6 269.3  3.3       0.0   -36      260   No stop 
08 42 35  ---          21 35 27  43.1 269.1  3.3       0.0    84      262   08 40 36

08 43 21  J1832-2039   21 36 13  47.9 267.3  3.0       0.0    10      262   08 43 21
08 46 16  =1829-207    21 39 09  47.2 267.0  3.1       0.0   175      265   08 43 22

08 46 16 G012.68-0.18  21 39 09  42.3 268.7  3.4       0.0   -36      265   No stop 
08 48 16  ---          21 41 09  41.9 268.5  3.4       0.0    84      267   08 46 17

08 48 16  J1832-2039   21 41 09  46.8 266.8  3.1       0.0   -36      267   No stop 
08 51 16  =1829-207    21 44 10  46.1 266.5  3.2       0.0   144      269   08 48 17

08 51 16 G012.68-0.18  21 44 10  41.2 268.2  3.5       0.0   -36      269   No stop 
08 53 16  ---          21 46 10  40.7 267.9  3.5       0.0    84      271   08 51 17

08 53 16  J1832-2039   21 46 10  45.6 266.3  3.2       0.0   -36      271   No stop 
08 56 16  =1829-207    21 49 10  45.0 266.0  3.3       0.0   144      274   08 53 17

08 56 16 G012.68-0.18  21 49 10  40.1 267.6  3.6       0.0   -36      274   No stop 
08 58 16  ---          21 51 11  39.6 267.4  3.6       0.0    84      276   08 56 17

08 59 02  J1832-2039   21 51 57  44.4 265.8  3.3       0.0    10      276   08 59 02
09 01 57  =1829-207    21 54 52  43.7 265.5  3.4       0.0   175      279   08 59 03

09 01 57 G012.68-0.18  21 54 52  38.8 267.1  3.7       0.0   -36      279   No stop 
09 03 57  ---          21 56 53  38.3 266.9  3.7       0.0    84      281   09 01 58

09 03 57  J1832-2039   21 56 53  43.2 265.3  3.4       0.0   -36      281   No stop 
09 06 57  =1829-207    21 59 53  42.6 265.0  3.4       0.0   144      284   09 03 58

09 06 57 G012.68-0.18  21 59 53  37.7 266.6  3.7       0.0   -36      284   No stop 
09 08 57  ---          22 01 54  37.2 266.4  3.8       0.0    84      286   09 06 58

09 09 43  J1832-2039   22 02 40  41.9 264.8  3.5       0.0    10      286   09 09 43
09 12 38  =1829-207    22 05 35  41.3 264.5  3.5       0.0   175      289   09 09 44

09 29 43  J1832-2039   22 22 43  37.5 263.0  3.8       0.0  1003      289   09 29 43
09 32 43  =1829-207    22 25 43  36.8 262.7  3.9       0.0   180      292   09 29 44

09 32 43 G012.68-0.18  22 25 43  31.9 264.1  4.2       0.0   -36      292   No stop 
09 34 43  ---          22 27 44  31.4 263.9  4.2       0.0    84      293   09 32 44

09 34 43  J1832-2039   22 27 44  36.3 262.6  3.9       0.0   -36      293   No stop 
09 37 43  =1829-207    22 30 44  35.7 262.3  4.0       0.0   144      296   09 34 44
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

09 37 43 G012.68-0.18  22 30 44  30.7 263.6  4.3       0.0   -36      296   No stop 
09 39 43  ---          22 32 45  30.3 263.4  4.3       0.0    84      298   09 37 44

09 39 43  J1832-2039   22 32 45  35.2 262.1  4.0       0.0   -36      298   No stop 
09 42 43  =1829-207    22 35 45  34.6 261.9  4.0       0.0   144      301   09 39 44

09 42 43 G012.68-0.18  22 35 45  29.6 263.1  4.3       0.0   -36      301   No stop 
09 44 43  ---          22 37 45  29.2 262.9  4.4       0.0    84      303   09 42 44

09 45 28  J1832-2039   22 38 31  33.9 261.6  4.1       0.0     9      303   09 45 28
09 48 23  =1829-207    22 41 26  33.3 261.4  4.1       0.0   175      306   09 45 29

09 48 23 G012.68-0.18  22 41 26  28.4 262.6  4.4       0.0   -36      306   No stop 
09 50 23  ---          22 43 26  27.9 262.4  4.5       0.0    84      308   09 48 24

09 50 23  J1832-2039   22 43 26  32.8 261.2  4.2       0.0   -36      308   No stop 
09 53 23  =1829-207    22 46 27  32.2 260.9  4.2       0.0   144      311   09 50 24

09 53 23 G012.68-0.18  22 46 27  27.2 262.1  4.5       0.0   -36      311   No stop 
09 55 23  ---          22 48 27  26.8 261.9  4.6       0.0    84      313   09 53 24

09 55 23  J1832-2039   22 48 27  31.7 260.8  4.3       0.0   -36      313   No stop 
09 58 23  =1829-207    22 51 28  31.1 260.5  4.3       0.0   144      316   09 55 24

09 58 23 G012.68-0.18  22 51 28  26.1 261.7  4.6       0.0   -36      316   No stop 
10 00 23  ---          22 53 28  25.7 261.5  4.6       0.0    84      318   09 58 24

10 01 08  J1832-2039   22 54 13  30.5 260.3  4.3       0.0     9      318   10 01 08
10 04 03  =1829-207    22 57 09  29.8 260.0  4.4       0.0   175      320   10 01 09

10 04 03 G012.68-0.18  22 57 09  24.9 261.1  4.7       0.0   -36      320   No stop 
10 06 03  ---          22 59 09  24.4 260.9  4.7       0.0    84      322   10 04 04

10 06 03  J1832-2039   22 59 09  29.4 259.8  4.4       0.0   -36      322   No stop 
10 09 03  =1829-207    23 02 09  28.7 259.6  4.5       0.0   144      325   10 06 04

10 09 03 G012.68-0.18  23 02 09  23.7 260.7  4.8       0.0   -36      325   No stop 
10 11 03  ---          23 04 10  23.3 260.5  4.8       0.0    84      327   10 09 04

10 11 48  J1832-2039   23 04 55  28.1 259.3  4.5       0.0     9      327   10 11 48
10 14 43  =1829-207    23 07 50  27.4 259.1  4.6       0.0   175      330   10 11 49

10 39 13  J1832-2039   23 32 24  22.0 256.9  5.0       0.0  1448      330   10 39 13
10 42 13  =1829-207    23 35 25  21.4 256.6  5.0       0.0   180      333   10 39 14
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
----------------------------------------------------------------------------------------

 --- Sat   7 Mar 2020   Day  67 ---

10 42 13 G012.68-0.18  23 35 25  16.4 257.5  5.3       0.0   -36      333   No stop 
10 44 13  ---          23 37 25  16.0 257.4  5.4       0.0    84      335   10 42 14

10 44 13  J1832-2039   23 37 25  20.9 256.5  5.1       0.0   -36      335   No stop 
10 47 13  =1829-207    23 40 26  20.3 256.2  5.1       0.0   144      338   10 44 14

10 47 13 G012.68-0.18  23 40 26  15.3 257.1  5.4       0.0   -36      338   No stop 
10 50 13  ---          23 43 26  14.6 256.8  5.5       0.0   144      341   10 47 14

10 50 13  J1832-2039   23 43 26  19.6 255.9  5.2       0.0   -36      341   No stop 
10 53 13  =1829-207    23 46 27  19.0 255.7  5.2       0.0   144      343   10 50 14

10 53 13 G012.68-0.18  23 46 27  14.0 256.5  5.5       0.0   -36      343   No stop 
10 56 13  ---          23 49 27  13.3 256.2  5.6       0.0   144      346   10 53 14

10 56 13  J1832-2039   23 49 27  18.3 255.4  5.3       0.0   -36      346   No stop 
10 59 58  =1829-207    23 53 13  17.5 255.1  5.3       0.0   189      350   10 56 14


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:   7  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=   6661.17  6661.17  6661.17  6661.17  6665.17  6665.17  6665.17  6665.17
             6669.17  6669.17  6669.17  6669.17  6673.17  6673.17  6673.17  6673.17
   BBC fr=    151.17   151.17   151.17   151.17   155.17   155.17   155.17   155.17
              159.17   159.17   159.17   159.17   163.17   163.17   163.17   163.17
   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:   7

   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)

 * G012.68-0.18      18 10 59.237691   * 18 13 54.750000     18 15 03.984627       0.00
                    -18 02 40.99379    *-18 01 46.57000     -18 01 23.22923        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         57.50    57.50    57.50    57.50    57.50    57.50    57.50    57.50
                         57.50    57.50    57.50    57.50    57.50    57.50

 * 3C84              03 16 29.567265   * 03 19 48.160096     03 21 06.550898       1.50
   J0319+4130        41 19 51.91692    * 41 30 42.10404      41 35 02.64175        2.86
   0316+413          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J0319+41          GSFC 2016a X/S astro solution,  10291 observations.
                     Doppler based on other sources.

   3C286             13 28 49.657769   * 13 31 08.288061     13 32 04.420515       0.17
 * J1331+3030        30 45 58.64066    * 30 30 32.95930      30 24 13.65488        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 39.102106       0.79
   J1642+3948        39 54 10.81492    * 39 48 36.99399      39 46 08.22670        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.

   1829-207          18 29 12.261807   * 18 32 11.046470     18 33 21.455518       0.20
 * J1832-2039       -20 42 02.03596    *-20 39 48.20359     -20 38 52.59257        0.32
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    128 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362504   * 22 02 43.291371     22 03 30.892318       0.01
 * J2202+4216        42 02 08.59075    * 42 16 39.97988      42 22 18.37519        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
  G012.68-0.1sess120.M128          1 2 3 4 5 6 7 8 9                 1.867    38.676
  3C84       sess120.M128          1 2 3 4 5 6 8 9                   0.133     3.733
  J1331+3030 sess120.M128          1 2 3 4 5 6 7 8 9                 1.317    39.159
  3C345      sess120.M128          1 2 3 4 5 6 7 8 9                 0.333    11.971
  J1832-2039 sess120.M128          1 2 3 4 5 6 7 8 9                 3.171    73.508
  J2202+4216 sess120.M128          2 3 4 5 6 8 9                     0.167     3.500


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) 
   G012.68-0.18        73.6
   3C84                73.1
   J1331+3030         138.6
   3C345               98.8
   J1832-2039          69.4
   J2202+4216          50.0

  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 

