  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
 Exp. Code:  EM117D  


Schedule Version:       1.00
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 = G075.76+0.34
 
 

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

 --- Tue   1 Mar 2016   Day  61 ---

 Next scan frequencies:  6666.25  6666.25  6666.25  6666.25  6670.25  6670.25  6670.25  6670.25
                         6674.25  6674.25  6674.25  6674.25  6678.25  6678.25  6678.25  6678.25
 Next BBC frequencies:    156.25   156.25   156.25   156.25   160.25   160.25   160.25   160.25
                          164.25   164.25   164.25   164.25   168.25   168.25   168.25   168.25
 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

05 39 45  J2015+3710   18 08 20  20.1  26.6 -2.1       0.0     0        0   05 39 45
05 44 45  =2013+370    18 13 21  20.6  25.7 -2.0       0.0   300        5   05 39 46

05 44 45 G075.76+0.34  18 13 21  19.8  26.7 -2.1       0.0   -29        5   No stop 
05 46 45  ---          18 15 22  20.0  26.4 -2.1       0.0    91        7   05 44 46

05 47 15  J2015+3710   18 15 52  20.8  25.3 -2.0       0.0     1        7   05 47 15
05 50 15  =2013+370    18 18 52  21.1  24.7 -2.0       0.0   180       10   05 47 16

05 50 15 G075.76+0.34  18 18 52  20.3  25.7 -2.1       0.0   -29       10   No stop 
05 52 15  ---          18 20 53  20.5  25.3 -2.0       0.0    91       12   05 50 16

05 52 15  J2015+3710   18 20 53  21.3  24.3 -1.9       0.0   -29       12   No stop 
05 55 15  =2013+370    18 23 53  21.6  23.7 -1.9       0.0   151       14   05 52 16

05 55 15 G075.76+0.34  18 23 53  20.8  24.8 -2.0       0.0   -29       14   No stop 
05 57 15  ---          18 25 53  21.0  24.4 -1.9       0.0    91       16   05 55 16

05 57 45  J2015+3710   18 26 23  21.8  23.3 -1.8       0.0     1       16   05 57 45
06 00 45  =2013+370    18 29 24  22.1  22.7 -1.8       0.0   180       19   05 57 46

06 00 45 G075.76+0.34  18 29 24  21.3  23.8 -1.9       0.0   -29       19   No stop 
06 02 45  ---          18 31 24  21.5  23.4 -1.8       0.0    91       21   06 00 46

06 03 15  J2015+3710   18 31 54  22.3  22.2 -1.7       0.0     1       21   06 03 15
06 06 15  =2013+370    18 34 55  22.5  21.6 -1.7       0.0   180       24   06 03 16

06 06 15 G075.76+0.34  18 34 55  21.8  22.7 -1.8       0.0   -29       24   No stop 
06 08 15  ---          18 36 55  22.0  22.3 -1.8       0.0    91       26   06 06 16

06 08 15  J2015+3710   18 36 55  22.7  21.2 -1.7       0.0   -29       26   No stop 
06 11 15  =2013+370    18 39 56  23.0  20.6 -1.6       0.0   151       29   06 08 16

06 40 35  J2202+4216   19 09 20  10.8  31.2 -2.9       0.0  1680       29   06 40 35
06 48 35  =VR422201    19 17 22  11.8  30.0 -2.8       0.0   480       37   06 40 36

06 50 20  J2015+3710   19 19 07  25.5  12.5 -0.9       0.0    24       37   06 50 20
06 53 20  =2013+370    19 22 08  25.6  11.9 -0.9       0.0   180       39   06 50 21
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

06 53 20 G075.76+0.34  19 22 08  25.1  13.1 -1.0       0.0   -29       39   No stop 
06 55 20  ---          19 24 08  25.2  12.7 -1.0       0.0    91       41   06 53 21

06 55 20  J2015+3710   19 24 08  25.7  11.5 -0.9       0.0   -29       41   No stop 
06 58 20  =2013+370    19 27 08  25.8  10.8 -0.8       0.0   151       44   06 55 21

06 58 20 G075.76+0.34  19 27 08  25.3  12.1 -0.9       0.0   -29       44   No stop 
07 00 20  ---          19 29 09  25.4  11.6 -0.9       0.0    91       46   06 58 21

07 00 20  J2015+3710   19 29 09  25.9  10.4 -0.8       0.0   -29       46   No stop 
07 03 20  =2013+370    19 32 09  26.0   9.7 -0.7       0.0   151       49   07 00 21

07 03 20 G075.76+0.34  19 32 09  25.6  11.0 -0.8       0.0   -29       49   No stop 
07 05 20  ---          19 34 10  25.6  10.6 -0.8       0.0    91       51   07 03 21

07 05 53  J2015+3710   19 34 43  26.1   9.2 -0.7       0.0     4       51   07 05 53
07 08 53  =2013+370    19 37 43  26.2   8.5 -0.6       0.0   180       54   07 05 54

07 08 53 G075.76+0.34  19 37 43  25.8   9.8 -0.7       0.0   -29       54   No stop 
07 10 53  ---          19 39 43  25.9   9.4 -0.7       0.0    91       56   07 08 54

07 10 53  J2015+3710   19 39 43  26.3   8.1 -0.6       0.0   -29       56   No stop 
07 13 53  =2013+370    19 42 44  26.4   7.4 -0.6       0.0   151       59   07 10 54

07 13 53 G075.76+0.34  19 42 44  26.0   8.7 -0.7       0.0   -29       59   No stop 
07 15 53  ---          19 44 44  26.0   8.3 -0.6       0.0    91       61   07 13 54

07 15 53  J2015+3710   19 44 44  26.5   7.0 -0.5       0.0   -29       61   No stop 
07 18 53  =2013+370    19 47 45  26.5   6.3 -0.5       0.0   151       63   07 15 54

07 18 53 G075.76+0.34  19 47 45  26.1   7.6 -0.6       0.0   -29       63   No stop 
07 20 53  ---          19 49 45  26.2   7.2 -0.5       0.0    91       65   07 18 54

07 21 26  J2015+3710   19 50 18  26.6   5.7 -0.4       0.0     4       65   07 21 26
07 24 26  =2013+370    19 53 19  26.7   5.1 -0.4       0.0   180       68   07 21 27

07 24 26 G075.76+0.34  19 53 19  26.3   6.4 -0.5       0.0   -29       68   No stop 
07 26 26  ---          19 55 19  26.3   6.0 -0.4       0.0    91       70   07 24 27

07 26 26  J2015+3710   19 55 19  26.7   4.6 -0.3       0.0   -29       70   No stop 
07 29 26  =2013+370    19 58 19  26.7   4.0 -0.3       0.0   151       73   07 26 27

07 29 26 G075.76+0.34  19 58 19  26.4   5.3 -0.4       0.0   -29       73   No stop 
07 31 26  ---          20 00 20  26.4   4.9 -0.4       0.0    91       75   07 29 27
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

07 31 26  J2015+3710   20 00 20  26.8   3.5 -0.3       0.0   -29       75   No stop 
07 34 26  =2013+370    20 03 20  26.8   2.8 -0.2       0.0   151       78   07 31 27

07 36 21  J2202+4216   20 05 16  16.5  22.3 -2.0       0.0    35       78   07 36 21
07 44 21  =VR422201    20 13 17  17.2  20.9 -1.8       0.0   480       86   07 36 22

07 46 31  J2015+3710   20 15 27  26.9   0.1 -0.0       0.0    49       86   07 46 31
07 49 31  =2013+370    20 18 28  26.9 359.5  0.0       0.0   180       88   07 46 32

07 49 31 G075.76+0.34  20 18 28  26.6   0.8 -0.1       0.0   -29       88   No stop 
07 51 31  ---          20 20 28  26.6   0.4 -0.0       0.0    91       90   07 49 32

07 51 31  J2015+3710   20 20 28  26.9 359.0  0.1       0.0   -29       90   No stop 
07 54 31  =2013+370    20 23 29  26.9 358.3  0.1       0.0   151       93   07 51 32

07 54 31 G075.76+0.34  20 23 29  26.6 359.7  0.0       0.0   -29       93   No stop 
07 56 31  ---          20 25 29  26.6 359.3  0.1       0.0    91       95   07 54 32

07 56 31  J2015+3710   20 25 29  26.8 357.9  0.2       0.0   -29       95   No stop 
07 59 31  =2013+370    20 28 29  26.8 357.2  0.2       0.0   151       98   07 56 32

07 59 31 G075.76+0.34  20 28 29  26.6 358.6  0.1       0.0   -29       98   No stop 
08 01 31  ---          20 30 30  26.6 358.2  0.1       0.0    91      100   07 59 32

08 02 11  J2015+3710   20 31 10  26.8 356.6  0.3       0.0    11      100   08 02 11
08 05 11  =2013+370    20 34 10  26.7 356.0  0.3       0.0   180      103   08 02 12

08 05 11 G075.76+0.34  20 34 10  26.6 357.4  0.2       0.0   -29      103   No stop 
08 07 11  ---          20 36 11  26.6 356.9  0.2       0.0    91      105   08 05 12

08 07 11  J2015+3710   20 36 11  26.7 355.5  0.3       0.0   -29      105   No stop 
08 10 11  =2013+370    20 39 11  26.6 354.9  0.4       0.0   151      108   08 07 12

08 10 11 G075.76+0.34  20 39 11  26.5 356.2  0.3       0.0   -29      108   No stop 
08 12 11  ---          20 41 12  26.5 355.8  0.3       0.0    91      110   08 10 12

08 12 11  J2015+3710   20 41 12  26.6 354.4  0.4       0.0   -29      110   No stop 
08 15 11  =2013+370    20 44 12  26.5 353.7  0.5       0.0   151      112   08 12 12

08 15 11 G075.76+0.34  20 44 12  26.4 355.1  0.4       0.0   -29      112   No stop 
08 17 11  ---          20 46 12  26.4 354.7  0.4       0.0    91      114   08 15 12

08 17 51  J2015+3710   20 46 52  26.5 353.2  0.5       0.0    11      114   08 17 51
08 20 51  =2013+370    20 49 53  26.4 352.5  0.6       0.0   180      117   08 17 52
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

08 20 51 G075.76+0.34  20 49 53  26.3 353.9  0.5       0.0   -29      117   No stop 
08 22 51  ---          20 51 53  26.3 353.5  0.5       0.0    91      119   08 20 52

08 22 51  J2015+3710   20 51 53  26.3 352.1  0.6       0.0   -29      119   No stop 
08 25 51  =2013+370    20 54 54  26.2 351.4  0.6       0.0   151      122   08 22 52

08 25 51 G075.76+0.34  20 54 54  26.2 352.8  0.5       0.0   -29      122   No stop 
08 27 51  ---          20 56 54  26.1 352.4  0.6       0.0    91      124   08 25 52

08 27 51  J2015+3710   20 56 54  26.2 351.0  0.7       0.0   -29      124   No stop 
08 30 51  =2013+370    20 59 55  26.0 350.3  0.7       0.0   151      127   08 27 52

08 33 31  J2202+4216   21 02 35  20.3  11.9 -1.0       0.0    80      127   08 33 31
08 41 31  =VR422201    21 10 36  20.7  10.4 -0.9       0.0   480      135   08 33 32

08 44 31  J2015+3710   21 13 37  25.4 347.3  1.0       0.0    99      135   08 44 31
08 47 31  =2013+370    21 16 37  25.3 346.7  1.0       0.0   180      137   08 44 32

08 47 31 G075.76+0.34  21 16 37  25.4 348.1  0.9       0.0   -29      137   No stop 
08 49 31  ---          21 18 38  25.3 347.7  0.9       0.0    91      139   08 47 32

08 49 31  J2015+3710   21 18 38  25.2 346.3  1.0       0.0   -29      139   No stop 
08 52 31  =2013+370    21 21 38  25.0 345.6  1.1       0.0   151      142   08 49 32

08 52 31 G075.76+0.34  21 21 38  25.1 347.0  1.0       0.0   -29      142   No stop 
08 54 31  ---          21 23 38  25.0 346.6  1.0       0.0    91      144   08 52 32

08 54 31  J2015+3710   21 23 38  24.9 345.2  1.1       0.0   -29      144   No stop 
08 57 31  =2013+370    21 26 39  24.7 344.6  1.2       0.0   151      147   08 54 32

08 57 31 G075.76+0.34  21 26 39  24.9 346.0  1.1       0.0   -29      147   No stop 
08 59 31  ---          21 28 39  24.7 345.5  1.1       0.0    91      149   08 57 32

09 00 16  J2015+3710   21 29 24  24.6 344.0  1.2       0.0    16      149   09 00 16
09 03 16  =2013+370    21 32 25  24.4 343.4  1.3       0.0   180      152   09 00 17

09 03 16 G075.76+0.34  21 32 25  24.5 344.8  1.2       0.0   -29      152   No stop 
09 05 16  ---          21 34 25  24.4 344.3  1.2       0.0    91      154   09 03 17

09 05 16  J2015+3710   21 34 25  24.2 343.0  1.3       0.0   -29      154   No stop 
09 08 16  =2013+370    21 37 26  24.0 342.4  1.4       0.0   151      157   09 05 17

09 08 16 G075.76+0.34  21 37 26  24.2 343.7  1.3       0.0   -29      157   No stop 
09 10 16  ---          21 39 26  24.1 343.3  1.3       0.0    91      159   09 08 17
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

09 10 16  J2015+3710   21 39 26  23.9 341.9  1.4       0.0   -29      159   No stop 
09 13 16  =2013+370    21 42 27  23.7 341.3  1.4       0.0   151      162   09 10 17

09 13 16 G075.76+0.34  21 42 27  23.9 342.7  1.3       0.0   -29      162   No stop 
09 15 16  ---          21 44 27  23.8 342.3  1.4       0.0    91      163   09 13 17

09 16 01  J2015+3710   21 45 12  23.5 340.8  1.5       0.0    16      163   09 16 01
09 19 01  =2013+370    21 48 12  23.3 340.2  1.5       0.0   180      166   09 16 02

09 19 01 G075.76+0.34  21 48 12  23.5 341.5  1.4       0.0   -29      166   No stop 
09 21 01  ---          21 50 13  23.4 341.1  1.5       0.0    91      168   09 19 02

09 21 01  J2015+3710   21 50 13  23.1 339.8  1.6       0.0   -29      168   No stop 
09 24 01  =2013+370    21 53 13  22.9 339.2  1.6       0.0   151      171   09 21 02

09 24 01 G075.76+0.34  21 53 13  23.1 340.5  1.5       0.0   -29      171   No stop 
09 26 01  ---          21 55 14  23.0 340.1  1.5       0.0    91      173   09 24 02

09 26 01  J2015+3710   21 55 14  22.7 338.8  1.7       0.0   -29      173   No stop 
09 29 01  =2013+370    21 58 14  22.5 338.2  1.7       0.0   151      176   09 26 02

09 29 01 G075.76+0.34  21 58 14  22.7 339.5  1.6       0.0   -29      176   No stop 
09 31 01  ---          22 00 14  22.6 339.1  1.6       0.0    91      178   09 29 02

09 31 01  J2015+3710   22 00 14  22.3 337.8  1.7       0.0   -29      178   No stop 
09 34 01  =2013+370    22 03 15  22.0 337.2  1.8       0.0   151      181   09 31 02

09 38 01  J2202+4216   22 07 16  21.7 359.2  0.1       0.0   160      181   09 38 01
09 46 01  =VR422201    22 15 17  21.7 357.6  0.2       0.0   480      188   09 38 02

09 50 21  J2015+3710   22 19 38  20.5 334.1  2.1       0.0   179      188   09 50 21
09 53 21  =2013+370    22 22 38  20.2 333.6  2.1       0.0   180      191   09 50 22

09 53 21 G075.76+0.34  22 22 38  20.6 334.8  2.0       0.0   -29      191   No stop 
09 55 21  ---          22 24 38  20.4 334.5  2.0       0.0    91      193   09 53 22

09 55 21  J2015+3710   22 24 38  20.0 333.2  2.1       0.0   -29      193   No stop 
09 58 21  =2013+370    22 27 39  19.7 332.7  2.2       0.0   151      196   09 55 22

09 58 21 G075.76+0.34  22 27 39  20.1 333.9  2.1       0.0   -29      196   No stop 
10 00 21  ---          22 29 39  19.9 333.6  2.1       0.0    91      198   09 58 22

10 00 21  J2015+3710   22 29 39  19.5 332.3  2.2       0.0   -29      198   No stop 
10 03 21  =2013+370    22 32 40  19.2 331.8  2.3       0.0   151      201   10 00 22
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

10 03 21 G075.76+0.34  22 32 40  19.6 333.0  2.2       0.0   -29      201   No stop 
10 05 21  ---          22 34 40  19.4 332.6  2.2       0.0    91      203   10 03 22

10 06 01  J2015+3710   22 35 20  18.9 331.3  2.3       0.0    11      203   10 06 01
10 09 01  =2013+370    22 38 21  18.6 330.8  2.4       0.0   180      206   10 06 02

10 09 01 G075.76+0.34  22 38 21  19.0 332.0  2.3       0.0   -29      206   No stop 
10 11 01  ---          22 40 21  18.8 331.6  2.3       0.0    91      208   10 09 02

10 11 01  J2015+3710   22 40 21  18.3 330.4  2.4       0.0   -29      208   No stop 
10 14 01  =2013+370    22 43 22  18.0 329.9  2.5       0.0   151      211   10 11 02

10 14 01 G075.76+0.34  22 43 22  18.5 331.1  2.4       0.0   -29      211   No stop 
10 16 01  ---          22 45 22  18.3 330.8  2.4       0.0    91      212   10 14 02

10 16 01  J2015+3710   22 45 22  17.8 329.5  2.5       0.0   -29      212   No stop 
10 19 01  =2013+370    22 48 22  17.4 329.0  2.5       0.0   151      215   10 16 02

10 19 01 G075.76+0.34  22 48 22  17.9 330.2  2.4       0.0   -29      215   No stop 
10 21 01  ---          22 50 23  17.7 329.9  2.5       0.0    91      217   10 19 02

10 21 36  J2015+3710   22 50 58  17.1 328.6  2.6       0.0     6      217   10 21 36
10 24 36  =2013+370    22 53 58  16.8 328.1  2.6       0.0   180      220   10 21 37

10 24 36 G075.76+0.34  22 53 58  17.3 329.3  2.5       0.0   -29      220   No stop 
10 26 36  ---          22 55 59  17.1 328.9  2.6       0.0    91      222   10 24 37

10 26 36  J2015+3710   22 55 59  16.5 327.7  2.7       0.0   -29      222   No stop 
10 29 36  =2013+370    22 58 59  16.2 327.3  2.7       0.0   151      225   10 26 37

10 29 36 G075.76+0.34  22 58 59  16.7 328.4  2.6       0.0   -29      225   No stop 
10 31 36  ---          23 00 59  16.5 328.1  2.6       0.0    91      227   10 29 37

10 31 36  J2015+3710   23 00 59  15.9 326.9  2.7       0.0   -29      227   No stop 
10 34 36  =2013+370    23 04 00  15.6 326.4  2.8       0.0   151      230   10 31 37

10 38 56  J2202+4216   23 08 21  20.1 347.3  1.1       0.0   180      230   10 38 56
10 46 56  =VR422201    23 16 22  19.7 345.8  1.2       0.0   480      237   10 38 57

10 51 26  J2015+3710   23 20 53  13.4 323.8  3.1       0.0   189      237   10 51 26
10 54 26  =2013+370    23 23 53  13.0 323.3  3.1       0.0   180      240   10 51 27

10 54 26 G075.76+0.34  23 23 53  13.6 324.4  3.0       0.0   -29      240   No stop 
10 56 26  ---          23 25 53  13.4 324.1  3.1       0.0    91      242   10 54 27
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

10 56 26  J2015+3710   23 25 53  12.7 323.0  3.2       0.0   -29      242   No stop 
10 59 26  =2013+370    23 28 54  12.3 322.6  3.2       0.0   151      245   10 56 27

10 59 26 G075.76+0.34  23 28 54  13.0 323.7  3.1       0.0   -29      245   No stop 
11 01 26  ---          23 30 54  12.7 323.4  3.1       0.0    91      247   10 59 27

11 01 26  J2015+3710   23 30 54  12.0 322.3  3.2       0.0   -29      247   No stop 
11 04 26  =2013+370    23 33 55  11.6 321.8  3.3       0.0   151      250   11 01 27

11 04 26 G075.76+0.34  23 33 55  12.3 322.9  3.2       0.0   -29      250   No stop 
11 06 26  ---          23 35 55  12.0 322.6  3.2       0.0    91      252   11 04 27

11 06 56  J2015+3710   23 36 25  11.3 321.5  3.3       0.0     1      252   11 06 56
11 09 56  =2013+370    23 39 26  10.8 321.1  3.4       0.0   180      255   11 06 57

11 09 56 G075.76+0.34  23 39 26  11.5 322.1  3.3       0.0   -29      255   No stop 
11 11 56  ---          23 41 26  11.3 321.8  3.3       0.0    91      257   11 09 57

11 11 56  J2015+3710   23 41 26  10.6 320.8  3.4       0.0   -29      257   No stop 
11 14 56  =2013+370    23 44 27  10.1 320.3  3.5       0.0   151      260   11 11 57

11 14 56 G075.76+0.34  23 44 27  10.8 321.4  3.4       0.0   -29      260   No stop 
11 16 56  ---          23 46 27  10.6 321.1  3.4       0.0    91      262   11 14 57

11 16 56  J2015+3710   23 46 27   9.8 320.1  3.5       0.0   -29      262   No stop 
11 19 56  =2013+370    23 49 27   9.4 319.6  3.6       0.0   151      264   11 16 57

11 19 56 G075.76+0.34  23 49 27  10.1 320.7  3.5       0.0   -29      264   No stop 
11 21 56  ---          23 51 28   9.8 320.4  3.5       0.0    91      266   11 19 57

11 22 26  J2015+3710   23 51 58   9.0 319.3  3.6       0.0     1      266   11 22 26
11 25 26  =2013+370    23 54 58   8.6 318.9  3.6       0.0   180      269   11 22 27

11 25 26 G075.76+0.34  23 54 58   9.3 319.9  3.5       0.0   -29      269   No stop 
11 27 26  ---          23 56 59   9.0 319.6  3.6       0.0    91      271   11 25 27

11 27 26  J2015+3710   23 56 59   8.3 318.6  3.7       0.0   -29      271   No stop 
11 30 26  =2013+370    23 59 59   7.8 318.2  3.7  D    0.0     0      274   11 27 27

11 30 26 G075.76+0.34  23 59 59   8.6 319.2  3.6       0.0   -29      274   No stop 
11 32 26  ---          00 01 59   8.3 319.0  3.7       0.0    91      276   11 30 27

11 38 41  J2202+4216   00 08 15  15.9 336.5  2.1       0.0   298      276   11 38 41
11 46 41  =VR422201    00 16 17  15.2 335.2  2.2       0.0   480      284   11 38 42
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
----------------------------------------------------------------------------------------

 --- Tue   1 Mar 2016   Day  61 ---

12 35 36  J2202+4216   01 05 20   9.9 327.7  3.0       0.0  2912      284   12 35 36
12 43 36  =VR422201    01 13 21   8.9 326.5  3.2       0.0   480      291   12 35 37


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


 ======== Setup file: sess116.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: MARK5B            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=   6666.25  6666.25  6666.25  6666.25  6670.25  6670.25  6670.25  6670.25
             6674.25  6674.25  6674.25  6674.25  6678.25  6678.25  6678.25  6678.25
   BBC fr=    156.25   156.25   156.25   156.25   160.25   160.25   160.25   160.25
              164.25   164.25   164.25   164.25   168.25   168.25   168.25   168.25
   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=  18, 26,  2, 10, 20, 28,  4, 12, 22, 30,  6, 14, 24, 32,  8, 16
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * G075.76+0.34      20 19 48.964357   * 20 21 41.094000     20 22 16.167756       0.00
                     37 15 51.67525    * 37 25 29.10000      37 28 31.48301        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                        -10.00   -10.00   -10.00   -10.00   -10.00   -10.00   -10.00   -10.00
                        -10.00   -10.00   -10.00   -10.00   -10.00   -10.00

   3C286             13 28 49.657758   * 13 31 08.288051     13 31 53.704256       0.18
 * J1331+3030        30 45 58.64059    * 30 30 32.95924      30 25 25.06967        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.

   2013+370          20 13 37.014511   * 20 15 28.729797     20 16 03.684961       0.13
 * J2015+3710        37 01 44.45895    * 37 10 59.51482      37 13 54.59117        0.18
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished    131 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362505   * 22 02 43.291372     22 03 22.063487       0.00
 * J2202+4216        42 02 08.59077    * 42 16 39.97990      42 21 18.92116        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
  G075.76+0.3sess116.M128          1 2 3 4 5 6 7 8 10                2.300    74.971
  J1331+3030 sess116.M128          1 2 3 4 5 6 7 8                   0.217     7.798
  J2015+3710 sess116.M128          1 2 3 4 5 6 7 8 10                3.933   144.257
  J2202+4216 sess116.M128          1 2 3 4 5 6 7 8 10                1.341    53.901


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) 
   G075.76+0.34        56.7
   J1331+3030         135.8
   J2015+3710          57.4
   J2202+4216          50.9

  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 

