  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Resolving the mystery of large VLBI-Gaia offsets
 Exp. Code:  ek046g  


Schedule Version:       1.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Yuri Kovalev

Address:  Lebedev Physical Institute
          Profsoyuznaya 84/32
          Moscow 117997
          Russia

Phone:    +7 (495) 3332167
EMAIL:    yyk@asc.rssi.ru
Fax:      +7 (495) 3332378
Phone during observation: +7 (915) 1546281

Observing mode: continuum

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               Resolving the mystery of large VLBI-Gaia offsets
  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   3 Mar 2020   Day  63 ---

 Next scan frequencies:  22139.49  22139.49  22139.49  22139.49  22203.49  22203.49  22203.49  22203.49
                         22267.49  22267.49  22267.49  22267.49  22331.49  22331.49  22331.49  22331.49
 Next BBC frequencies:     139.49    139.49    139.49    139.49    203.49    203.49    203.49    203.49
                           267.49    267.49    267.49    267.49    331.49    331.49    331.49    331.49
 Next scan bandwidths:      32.00     32.00     32.00     32.00     32.00     32.00     32.00     32.00
                            32.00     32.00     32.00     32.00     32.00     32.00     32.00     32.00

06 06 10  J1759+2343   18 42 51  39.3 347.2  0.7       0.0     0        0   06 05 40
06 09 40  =1756+237    18 46 21  39.1 346.2  0.8       0.0   210       62   06 05 41

06 48 41  J1759+2343   19 25 28  36.2 335.5  1.4       0.0  2318       62   06 48 41
06 52 11  =1756+237    19 28 59  35.9 334.6  1.5       0.0   210      116   06 48 42

06 56 28  J2253+1608   19 33 17  25.4  55.0 -3.4       0.0    84      116   06 56 28
06 59 58  =2251+158    19 36 48  26.0  54.4 -3.3       0.0   210      170   06 56 29

07 01 28  J2216+3518   19 38 17  18.1  33.2 -2.6       0.0    24      170   07 01 28
07 04 58  =2214+350    19 41 48  18.6  32.6 -2.6       0.0   210      224   07 01 29

07 05 51  J2244+4057   19 42 41  10.8  33.3 -3.0       0.0    12      224   07 05 51
07 09 21  =2241+406    19 46 12  11.3  32.8 -3.0       0.0   210      278   07 05 52

07 45 06  J2129-1538   20 22 02  71.0  60.4 -1.1       0.0  2004      278   07 45 06
07 48 36  =2126-158    20 25 33  71.7  58.8 -1.1       0.0   210      332   07 45 07

07 52 27  J2131-1207   20 29 25  69.7  50.0 -1.1       0.0   197      332   07 52 27
07 55 57  =2128-123    20 32 55  70.3  48.2 -1.0       0.0   210      386   07 52 28

08 15 22  J1759+2343   20 52 24  25.2 316.2  2.9       0.0  1031      386   08 15 22
08 18 52  =1756+237    20 55 54  24.6 315.6  2.9       0.0   210      441   08 15 23

08 48 21  J2129-1538   21 25 28  79.6   6.4 -0.1       0.0  1638      441   08 48 21
08 51 51  =2126-158    21 28 59  79.7   1.7 -0.0       0.0   210      495   08 48 22

08 52 25  J2131-1207   21 29 33  76.1   3.2 -0.1       0.0     0      495   08 52 25
08 55 55  =2128-123    21 33 04  76.1 359.6  0.0       0.0   210      549   08 52 26

08 58 01  J2253+1608   21 35 10  43.6  26.9 -1.3       0.0    42      549   08 58 01
09 01 31  =2251+158    21 38 41  44.0  25.8 -1.3       0.0   210      603   08 58 02

09 03 04  J2216+3518   21 40 14  28.1   8.5 -0.6       0.0    27      603   09 03 04
09 06 34  =2214+350    21 43 44  28.2   7.7 -0.6       0.0   210      657   09 03 05

09 07 41  J2244+4057   21 44 51  21.6  12.2 -1.0       0.0    26      657   09 07 41
09 11 11  =2241+406    21 48 21  21.8  11.5 -0.9       0.0   210      711   09 07 42
Schedule for HART      (Code Hh )                                   Page   3
               Resolving the mystery of large VLBI-Gaia offsets
  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   3 Mar 2020   Day  63 ---

09 24 33  J1759+2343   22 01 46  13.3 305.0  4.0       0.0   632      711   09 24 33
09 28 03  =1756+237    22 05 17  12.7 304.6  4.1       0.0   210      765   09 24 34

09 31 46  J2129-1538   22 09 00  76.3 316.9  0.6       0.0    91      765   09 31 46
09 35 16  =2126-158    22 12 31  75.7 314.3  0.7       0.0   210      819   09 31 47

09 35 50  J2131-1207   22 13 05  73.2 323.6  0.7       0.0     0      819   09 35 50
09 39 20  =2128-123    22 16 36  72.7 321.2  0.7       0.0   210      873   09 35 51

10 03 30  J0005+3820   22 40 49  22.6  18.1 -1.4       0.0  1322      873   10 03 30
10 07 00  =0003+380    22 44 20  22.8  17.4 -1.4       0.0   210      927   10 03 31

10 07 53  J0048+3157   22 45 13  24.9  28.9 -2.1       0.0     5      927   10 07 53
10 11 23  =0046+316    22 48 44  25.3  28.2 -2.0       0.0   210      982   10 07 54

10 12 33  J0052+4402   22 49 54  14.5  22.4 -2.1       0.0    18      982   10 12 33
10 16 03  =0049+437    22 53 24  14.7  21.8 -2.0       0.0   210     1036   10 12 34

10 17 14  J0152+3350   22 54 36  16.6  37.6 -3.0       0.0    14     1036   10 17 14
10 20 44  =0149+335    22 58 06  17.1  37.0 -2.9       0.0   210     1090   10 17 15

10 22 17  J0231+1322   22 59 39  24.9  59.3 -3.6       0.0    25     1090   10 22 17
10 25 47  =0229+131    23 03 10  25.6  58.7 -3.5       0.0   210     1144   10 22 18

10 36 57  J2131-1207   23 14 21  62.3 295.3  1.7       0.0   491     1144   10 36 57
10 40 27  =2128-123    23 17 52  61.6 294.3  1.8       0.0   210     1198   10 36 58

10 41 01  J2129-1538   23 18 26  62.8 286.9  1.8       0.0     0     1198   10 41 01
10 44 31  =2126-158    23 21 57  62.0 286.1  1.9       0.0   210     1252   10 41 02

11 35 09  J2129-1538   00 12 43  50.8 277.1  2.7       0.0  3015     1252   11 35 09
11 38 39  =2126-158    00 16 14  50.0 276.6  2.8       0.0   210     1306   11 35 10

11 39 13  J2131-1207   00 16 48  49.0 281.8  2.7       0.0     0     1306   11 39 13
11 42 43  =2128-123    00 20 18  48.2 281.3  2.8       0.0   210     1360   11 39 14

11 44 59  J2253+1608   00 22 35  42.8 330.8  1.5       0.0    53     1360   11 44 59
11 48 29  =2251+158    00 26 06  42.4 329.8  1.5       0.0   210     1414   11 45 00

11 49 50  J2216+3518   00 27 27  21.4 331.9  2.2       0.0    16     1414   11 49 50
11 53 20  =2214+350    00 30 58  21.0 331.2  2.2       0.0   210     1469   11 49 51

11 54 44  J2244+4057   00 32 22  18.6 339.0  1.8       0.0    43     1469   11 54 44
11 58 14  =2241+406    00 35 52  18.3 338.3  1.8       0.0   210     1523   11 54 45
Schedule for HART      (Code Hh )                                   Page   4
               Resolving the mystery of large VLBI-Gaia offsets
  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   3 Mar 2020   Day  63 ---

 ---------- >>> Pointing gap 3: all telescopes which need it <<< ----------

12 10 04  J0005+3820   00 47 44  25.0 351.2  0.7       0.0   642     1523   12 10 04
12 13 34  =0003+380    00 51 15  24.8 350.5  0.7       0.0   210     1577   12 10 05

12 14 40  J0048+3157   00 52 21  32.0 359.4  0.0       0.0    18     1577   12 14 40
12 18 10  =0046+316    00 55 52  32.0 358.5  0.1       0.0   210     1631   12 14 41

12 19 36  J0052+4402   00 57 18  19.9 359.3  0.1       0.0    34     1631   12 19 36
12 23 06  =0049+437    01 00 48  19.9 358.6  0.1       0.0   210     1685   12 19 37

12 24 15  J0152+3350   01 01 57  28.9  12.3 -0.9       0.0    12     1685   12 24 15
12 27 45  =0149+335    01 05 28  29.1  11.4 -0.8       0.0   210     1739   12 24 16

12 29 21  J0231+1322   01 07 05  45.5  30.4 -1.4       0.0    29     1739   12 29 21
12 32 51  =0229+131    01 10 35  45.8  29.4 -1.4       0.0   210     1793   12 29 22

12 34 52  J0251+4315   01 12 36  17.0  18.8 -1.7       0.0    34     1793   12 34 52
12 38 22  =0248+430    01 16 07  17.3  18.2 -1.6       0.0   210     1847   12 34 53

13 08 19  J2253+1608   01 46 08  30.8 310.6  2.9       0.0  1649     1847   13 08 19
13 11 59  =2251+158    01 49 49  30.1 309.9  2.9       0.0   220     1904   13 08 20

13 13 58  J2216+3518   01 51 49  10.5 318.1  3.6       0.0    54     1904   13 13 58
13 17 38  =2214+350    01 55 29   9.9 317.6  3.6  H    0.0     0     1961   13 13 59

13 18 21  J2244+4057   01 56 12   9.7 325.5  3.2       0.0     2     1961   13 18 21
13 22 01  =2241+406    01 59 53   9.3 325.0  3.2       0.0   220     2017   13 18 22

13 46 43  J0005+3820   02 24 39  18.0 332.2  2.3       0.0  1414     2017   13 46 43
13 50 23  =0003+380    02 28 19  17.7 331.6  2.4       0.0   220     2074   13 46 44

13 52 09  J0048+3157   02 30 06  27.3 336.2  1.7       0.0    58     2074   13 52 09
13 55 49  =0046+316    02 33 47  27.0 335.4  1.7       0.0   220     2131   13 52 10

 ---------- >>> Pointing gap 4: all telescopes which need it <<< ----------

14 05 24  J0052+4402   02 43 23  15.6 339.9  1.8       0.0   524     2131   14 05 24
14 09 04  =0049+437    02 47 04  15.3 339.3  1.9       0.0   220     2187   14 05 25

14 12 09  J0152+3350   02 50 10  28.7 346.7  0.9       0.0   128     2187   14 12 09
14 15 49  =0149+335    02 53 50  28.5 345.8  1.0       0.0   220     2244   14 12 10

14 17 19  J0231+1322   02 55 20  50.3 351.4  0.4       0.0    21     2244   14 17 19
14 20 59  =0229+131    02 59 00  50.1 350.0  0.4       0.0   220     2301   14 17 20
Schedule for HART      (Code Hh )                                   Page   5
               Resolving the mystery of large VLBI-Gaia offsets
  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   3 Mar 2020   Day  63 ---

14 23 19  J0251+4315   03 01 21  20.7 358.4  0.1       0.0    53     2301   14 23 19
14 26 59  =0248+430    03 05 01  20.7 357.6  0.2       0.0   220     2357   14 23 20

15 01 44  J2253+1608   03 39 52   9.0 293.0  4.7       0.0  1938     2357   15 01 44
15 05 24  =2251+158    03 43 33   8.2 292.6  4.8       0.0   220     2414   15 01 45

15 17 04  J0052+4402   03 55 15   8.6 328.9  3.0  H    0.0   615     2414   15 17 04
15 20 44  =0049+437    03 58 56   8.1 328.4  3.1  H    0.0     0     2471   15 17 05

15 23 22  J0152+3350   04 01 34  22.9 331.5  2.1       0.0   101     2471   15 23 22
15 27 02  =0149+335    04 05 14  22.5 330.8  2.2       0.0   220     2527   15 23 23

15 28 21  J0231+1322   04 06 34  44.5 327.2  1.6       0.0    11     2527   15 28 21
15 32 01  =0229+131    04 10 14  44.1 326.1  1.6       0.0   220     2584   15 28 22

15 34 05  J0251+4315   04 12 19  18.4 344.9  1.3       0.0    37     2584   15 34 05
15 37 45  =0248+430    04 15 59  18.2 344.2  1.4       0.0   220     2641   15 34 06

16 39 38  J0152+3350   05 18 02  13.0 318.5  3.4       0.0  3655     2641   16 39 38
16 43 18  =0149+335    05 21 43  12.5 318.0  3.5       0.0   220     2697   16 39 39

16 44 34  J0251+4315   05 23 00  12.7 333.0  2.5       0.0    20     2697   16 44 34
16 48 14  =0248+430    05 26 40  12.3 332.4  2.6       0.0   220     2754   16 44 35

17 56 16  J0231+1322   06 34 53  19.2 296.3  4.0       0.0  3995     2754   17 56 16
17 59 56  =0229+131    06 38 34  18.5 295.8  4.1       0.0   220     2811   17 56 17


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


 ======== Setup file: sess120.K2048
 --- WARNING ---  This group does not match an entry in the frequency catalog.
                  This might be ok because the catalog is not complete.
                  But be very careful to be sure that the setup is correct.

   Setup group:    7         Station: HART              Total bit rate:  2048
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
            22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
   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:  16  Setup file default.  Used with PCAL = 1MHz
   LO sum=   22139.49  22139.49  22139.49  22139.49  22203.49  22203.49  22203.49  22203.49
             22267.49  22267.49  22267.49  22267.49  22331.49  22331.49  22331.49  22331.49
   BBC fr=     139.49    139.49    139.49    139.49    203.49    203.49    203.49    203.49
               267.49    267.49    267.49    267.49    331.49    331.49    331.49    331.49
   Bandwd=      32.00     32.00     32.00     32.00     32.00     32.00     32.00     32.00
                32.00     32.00     32.00     32.00     32.00     32.00     32.00     32.00
    Matching frequency sets:  16

   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)

   0003+380          00 03 22.335504   * 00 05 57.175393     00 06 57.269173       0.13
 * J0005+3820        38 03 33.40997    * 38 20 15.14904      38 26 50.71943        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  1840 observations

   0008+704          00 08 49.693643   * 00 11 31.902797     00 12 33.380088       0.56
 * J0011+7045        70 28 50.79210    * 70 45 31.62634      70 52 12.97815        0.22
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  176 observations

   0046+316          00 46 04.857322   * 00 48 47.141480     00 49 50.417782       0.12
 * J0048+3157        31 41 04.49533    * 31 57 25.08484      32 03 52.15807        0.11
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  1080 observations

   0049+437          00 49 39.848494   * 00 52 27.825867     00 53 33.243813       0.18
 * J0052+4402        43 46 37.37207    * 44 02 54.51597      44 09 23.02751        0.15
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  255 observations

   0149+335          01 49 40.036701   * 01 52 34.576408     01 53 42.997123       0.18
 * J0152+3350        33 35 46.68972    * 33 50 33.15880      33 56 24.53342        0.18
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  151 observations

   0153+744          01 53 04.337075   * 01 57 34.964939     01 59 20.938938       0.44
 * J0157+7442        74 28 05.62189    * 74 42 43.22953      74 48 40.61066        0.11
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  1126 observations

   0229+131          02 29 02.524214   * 02 31 45.894061     02 32 50.099348       0.10
 * J0231+1322        13 09 40.78819    * 13 22 54.71634      13 28 03.65864        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  109449 observations

   0248+430          02 48 18.485707   * 02 51 34.536750     02 52 51.795578       0.14
 * J0251+4315        43 02 56.98557    * 43 15 15.82919      43 20 12.08478        0.11
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  1308 observations

   0538+498          05 38 43.517524   * 05 42 36.137901     05 44 09.012102       0.16
 * J0542+4951        49 49 42.83716    * 49 51 07.23379      49 51 44.80619        0.11
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  2002 observations

   1637+826          16 37 56.926910   * 16 32 31.969878     16 30 26.512818       0.78
 * J1632+8232        82 38 18.49826    * 82 32 16.39990      82 29 26.94415        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  10135 observations

   1738+451          17 38 39.409580   * 17 40 06.372611     17 40 40.416419       0.21
 * J1740+4506        45 08 20.31720    * 45 06 50.37091      45 05 58.05150        0.20
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  123 observations

   1756+237          17 56 55.937405   * 17 59 00.358089     17 59 49.254234       0.19
 * J1759+2343        23 43 55.77917    * 23 43 46.95383      23 43 31.81358        0.21
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  181 observations

   1807+698          18 07 18.543587   * 18 06 50.680645     18 06 38.255076       0.29
 * J1806+6949        69 48 57.10467    * 69 49 28.10852      69 49 20.65164        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  146554 observations

   1823+568          18 23 14.951492   * 18 24 07.068370     18 24 26.712726       0.18
 * J1824+5651        56 49 18.07202    * 56 51 01.49083      56 51 25.10036        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  11370 observations

   1849+670          18 49 16.505869   * 18 49 16.072281     18 49 14.045875       0.26
 * J1849+6705        67 02 07.88053    * 67 05 41.68027      67 06 48.72797        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  47097 observations

   2010+723          20 10 16.209308   * 20 09 52.303853     20 09 38.985242       0.41
 * J2009+7229        72 20 20.74085    * 72 29 19.35053      72 32 39.26266        0.12
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  438 observations

   2126-158          21 26 26.777532   * 21 29 12.175899     21 30 16.430362       0.10
 * J2129-1538       -15 51 50.34808    *-15 38 41.04191     -15 33 31.61052        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  14782 observations

   2128-123          21 28 52.676060   * 21 31 35.261752     21 32 38.429543       0.10
 * J2131-1207       -12 20 20.53571    *-12 07 04.79610     -12 01 53.38188        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  16909 observations

   2214+350          22 14 07.014327   * 22 16 20.009902     22 17 11.287124       0.12
 * J2216+3518        35 03 15.09223    * 35 18 14.17996      35 24 04.64471        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  30582 observations

   2241+406          22 41 57.956930   * 22 44 12.731148     22 45 04.621486       0.23
 * J2244+4057        40 41 27.56069    * 40 57 13.62048      41 03 24.24748        0.22
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  85 observations

   2251+158          22 51 29.519743   * 22 53 57.747942     22 54 55.259581       0.10
 * J2253+1608        15 52 54.34805    * 16 08 53.56088      16 15 07.88648        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  41804 observations

   2353+816          23 53 58.676764   * 23 56 22.793915     23 57 12.708414       0.72
 * J2356+8152        81 36 10.67120    * 81 52 52.25510      81 59 34.76279        0.10
                     /home/guest/rmc/SCHED/sched11.5/catalogs/rfc_2018a_cat.key
                     rfc_2018a Petrov and Kovalev, in preparation  3111 observations



SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE

     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.
  Source       Setup file             Frequency sets                  Observing hours
                                   (duplicates not shown)              Scan  Baseline
  J0005+3820 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.297    23.698
  J0011+7045 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.300    30.111
  J0048+3157 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.297    25.294
  J0052+4402 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.297    26.558
  J0152+3350 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.300    23.693
  J0157+7442 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.300    31.277
  J0231+1322 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.300    23.824
  J0251+4315 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.300    26.625
  J0542+4951 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.303    28.885
  J1632+8232 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.300    29.847
  J1740+4506 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.292    15.690
  J1759+2343 sess120.K2048         1 2 3 5 6 7 8 11 12 16            0.292    12.919
  J1806+6949 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.297    30.122
  J1824+5651 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.294    20.932
  J1849+6705 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.297    29.420
  J2009+7229 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.300    30.322
  J2129-1538 sess120.K2048         1 2 3 5 6 7 8 11 12 16            0.292    12.677
  J2131-1207 sess120.K2048         1 2 3 5 6 7 8 11 12 16            0.292    13.751
  J2216+3518 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.297    20.806
  J2244+4057 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.297    22.835
  J2253+1608 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13 16       0.297    20.363
  J2356+8152 sess120.K2048         1 2 3 4 5 6 7 8 11 12 13          0.300    29.434


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) 
   J0005+3820          47.7
   J0011+7045          78.4
   J0048+3157          46.8
   J0052+4402          56.9
   J0152+3350          57.9
   J0157+7442          85.8
   J0231+1322          56.8
   J0251+4315          72.6
   J0542+4951         102.3
   J1632+8232          97.4
   J1740+4506          87.3
   J1759+2343          78.8
   J1806+6949          90.4
   J1824+5651          84.1
   J1849+6705          85.7
   J2009+7229          83.6
   J2129-1538          23.5
   J2131-1207          21.9
   J2216+3518          43.1
   J2244+4057          47.7
   J2253+1608          22.8
   J2356+8152          88.8

  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 

