  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Phase-referencing of NGC4418
 Exp. Code:  EV019B  


Schedule Version:       1.00
Processed by SCHED version:  11.00  Release of Feb. 15, 2013

PI:       Eskil Varenius

Address:  Chalmers University of Technology
          Onsala Space Observatory
          34992 Onsla
          Sweden

Phone:    +46 31 7725545
EMAIL:    varenius@chalmers.se
Fax:      N/A
Phone during observation: +46 70 6755341

Observing mode: Phase-referencing of NGC4418 at 6cm (1 Gb/s)

Notes:    Part of EV019; See also exp. EV019A at L-band.
 
 
 

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Phase-referencing of NGC4418
  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
----------------------------------------------------------------------------------------

 --- Thu   6 Mar 2014   Day  65 ---

 Next scan frequencies:  4942.49  4942.49  4942.49  4942.49  4974.49  4974.49  4974.49  4974.49
                         5006.49  5006.49  5006.49  5006.49  5038.49  5038.49  5038.49  5038.49
 Next BBC frequencies:    742.49   742.49   742.49   742.49   774.49   774.49   774.49   774.49
                          806.49   806.49   806.49   806.49   838.49   838.49   838.49   838.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00

19 30 00  J1232        14 32 36  46.0 225.9  2.0      38.0     0        0   19 30 00
19 31 00  ---          14 33 36  45.8 226.1  2.0      38.2    60        8   19 30 01

19 31 29  NGC4418      14 34 06  46.1 229.1  2.1      40.3    22        8   19 31 29
19 35 29  ---          14 38 06  45.4 230.2  2.2      41.1   240       38   19 31 30

19 35 59  J1232        14 38 36  45.0 227.5  2.1      39.2    23       38   19 35 59
19 36 59  ---          14 39 36  44.9 227.8  2.1      39.4    60       46   19 36 00

19 37 28  NGC4418      14 40 05  45.1 230.7  2.2      41.5    22       46   19 37 28
19 41 28  ---          14 44 06  44.4 231.8  2.3      42.3   240       77   19 37 29

19 41 57  J1232        14 44 35  44.1 229.1  2.2      40.4    23       77   19 41 57
19 42 57  ---          14 45 35  43.9 229.4  2.2      40.6    60       85   19 41 58

19 43 26  NGC4418      14 46 05  44.1 232.3  2.3      42.6    23       85   19 43 26
19 47 26  ---          14 50 05  43.4 233.3  2.4      43.3   240      115   19 43 27

19 47 56  J1232        14 50 35  43.1 230.7  2.3      41.5    23      115   19 47 56
19 48 56  ---          14 51 35  42.9 231.0  2.3      41.7    60      123   19 47 57

19 49 25  NGC4418      14 52 04  43.1 233.8  2.4      43.7    23      123   19 49 25
19 53 25  ---          14 56 05  42.4 234.8  2.5      44.4   240      154   19 49 26

19 53 54  J1232        14 56 34  42.1 232.2  2.4      42.6    23      154   19 53 54
19 54 54  ---          14 57 34  41.9 232.5  2.4      42.8    60      162   19 53 55

19 55 23  NGC4418      14 58 04  42.0 235.2  2.5      44.7    23      162   19 55 23
19 59 23  ---          15 02 04  41.3 236.2  2.6      45.4   240      192   19 55 24

19 59 53  J1232        15 02 34  41.1 233.7  2.5      43.7    23      192   19 59 53
20 00 53  ---          15 03 34  40.9 233.9  2.5      43.8    60      200   19 59 54

20 01 22  NGC4418      15 04 03  41.0 236.6  2.6      45.7    23      200   20 01 22
20 05 22  ---          15 08 04  40.3 237.6  2.7      46.3   240      231   20 01 23

20 05 51  J1232        15 08 33  40.0 235.1  2.6      44.7    23      231   20 05 51
20 06 51  ---          15 09 33  39.8 235.3  2.6      44.8    60      238   20 05 52
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Phase-referencing of NGC4418
  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
----------------------------------------------------------------------------------------

 --- Thu   6 Mar 2014   Day  65 ---

20 07 20  NGC4418      15 10 03  39.9 238.0  2.7      46.6    23      238   20 07 20
20 11 20  ---          15 14 03  39.2 238.9  2.8      47.2   240      269   20 07 21

20 11 50  J1232        15 14 33  39.0 236.5  2.7      45.6    23      269   20 11 50
20 12 50  ---          15 15 33  38.8 236.7  2.7      45.7    60      277   20 11 51

20 13 19  NGC4418      15 16 02  38.8 239.3  2.8      47.4    23      277   20 13 19
20 17 19  ---          15 20 03  38.1 240.2  2.9      48.0   240      308   20 13 20

20 17 48  J1232        15 20 32  37.9 237.8  2.8      46.5    23      308   20 17 48
20 18 48  ---          15 21 32  37.7 238.0  2.8      46.6    60      315   20 17 49

20 19 17  NGC4418      15 22 02  37.7 240.6  2.9      48.3    23      315   20 19 17
20 23 17  ---          15 26 02  36.9 241.4  3.0      48.8   240      346   20 19 18

20 23 47  J1232        15 26 32  36.8 239.1  2.9      47.3    23      346   20 23 47
20 24 47  ---          15 27 32  36.6 239.3  2.9      47.5    60      354   20 23 48

20 25 16  NGC4418      15 28 01  36.6 241.8  3.0      49.0    23      354   20 25 16
20 29 16  ---          15 32 02  35.8 242.7  3.1      49.5   240      385   20 25 17

20 30 00  J1256        15 32 46  37.6 232.1  2.6      42.8    29      385   20 30 00
20 34 00  ---          15 36 46  36.9 233.0  2.7      43.4   240      415   20 30 01

20 34 39  J1232        15 37 26  34.8 241.3  3.1      48.7    27      415   20 34 39
20 35 39  ---          15 38 26  34.6 241.5  3.1      48.9    60      423   20 34 40

20 36 08  NGC4418      15 38 55  34.5 244.0  3.2      50.3    23      423   20 36 08
20 40 08  ---          15 42 56  33.7 244.8  3.3      50.8   240      454   20 36 09

20 40 38  J1232        15 43 25  33.6 242.5  3.2      49.5    23      454   20 40 38
20 41 38  ---          15 44 26  33.4 242.7  3.2      49.6    60      462   20 40 39

20 42 07  NGC4418      15 44 55  33.3 245.2  3.3      51.0    23      462   20 42 07
20 46 07  ---          15 48 56  32.6 245.9  3.4      51.4   240      492   20 42 08

20 46 36  J1232        15 49 25  32.5 243.6  3.3      50.2    23      492   20 46 36
20 47 36  ---          15 50 25  32.3 243.8  3.3      50.3    60      500   20 46 37

20 48 05  NGC4418      15 50 54  32.2 246.3  3.4      51.6    23      500   20 48 05
20 52 05  ---          15 54 55  31.4 247.0  3.5      52.0   240      531   20 48 06

20 52 35  J1232        15 55 24  31.3 244.8  3.4      50.8    23      531   20 52 35
20 53 35  ---          15 56 25  31.1 244.9  3.4      50.9    60      538   20 52 36
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Phase-referencing of NGC4418
  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
----------------------------------------------------------------------------------------

 --- Thu   6 Mar 2014   Day  65 ---

20 54 04  NGC4418      15 56 54  31.0 247.4  3.5      52.2    23      538   20 54 04
20 58 04  ---          16 00 55  30.2 248.1  3.6      52.6   240      569   20 54 05

20 58 33  J1232        16 01 24  30.2 245.9  3.5      51.5    23      569   20 58 33
20 59 33  ---          16 02 24  30.0 246.0  3.5      51.6    60      577   20 58 34

21 00 03  NGC4418      16 02 53  29.8 248.4  3.6      52.8    23      577   21 00 03
21 04 03  ---          16 06 54  29.0 249.1  3.7      53.1   240      608   21 00 04

21 04 32  J1232        16 07 23  29.0 246.9  3.6      52.0    23      608   21 04 32
21 05 32  ---          16 08 24  28.8 247.1  3.6      52.1    60      615   21 04 33

21 06 01  NGC4418      16 08 53  28.6 249.4  3.7      53.3    23      615   21 06 01
21 10 01  ---          16 12 54  27.8 250.1  3.8      53.6   240      646   21 06 02

21 10 30  J1232        16 13 23  27.8 248.0  3.7      52.6    23      646   21 10 30
21 11 30  ---          16 14 23  27.6 248.1  3.7      52.7    60      654   21 10 31

21 12 00  NGC4418      16 14 52  27.4 250.4  3.8      53.8    23      654   21 12 00
21 16 00  ---          16 18 53  26.6 251.1  3.9      54.1   240      685   21 12 01

21 16 29  J1232        16 19 22  26.6 249.0  3.8      53.1    23      685   21 16 29
21 17 29  ---          16 20 23  26.4 249.1  3.8      53.2    60      692   21 16 30

21 17 58  NGC4418      16 20 52  26.2 251.4  3.9      54.3    23      692   21 17 58
21 21 58  ---          16 24 53  25.4 252.1  4.0      54.6   240      723   21 17 59

21 22 27  J1232        16 25 22  25.4 250.0  3.9      53.6    23      723   21 22 27
21 23 27  ---          16 26 22  25.2 250.1  3.9      53.7    60      731   21 22 28

21 23 57  NGC4418      16 26 51  25.0 252.4  4.0      54.7    23      731   21 23 57
21 27 57  ---          16 30 52  24.1 253.0  4.1      55.0   240      762   21 23 58

21 28 26  J1232        16 31 21  24.2 250.9  4.0      54.1    23      762   21 28 26
21 29 26  ---          16 32 22  24.0 251.1  4.0      54.2    60      769   21 28 27

21 29 55  NGC4418      16 32 51  23.7 253.3  4.1      55.1    23      769   21 29 55
21 33 55  ---          16 36 52  22.9 254.0  4.2      55.4   240      800   21 29 56

21 34 49  J1256        16 37 45  25.7 245.0  3.7      51.3    41      800   21 34 49
21 38 49  ---          16 41 46  24.9 245.7  3.7      51.7   240      831   21 34 50

21 39 48  J1232        16 42 45  21.9 252.7  4.2      54.9    48      831   21 39 48
21 40 48  ---          16 43 45  21.7 252.9  4.2      55.0    60      838   21 39 49
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Phase-referencing of NGC4418
  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
----------------------------------------------------------------------------------------

 --- Thu   6 Mar 2014   Day  65 ---

21 41 17  NGC4418      16 44 14  21.4 255.1  4.3      55.8    23      838   21 41 17
21 45 17  ---          16 48 15  20.6 255.7  4.3      56.1   240      869   21 41 18

21 45 46  J1232        16 48 44  20.7 253.7  4.3      55.3    23      869   21 45 46
21 46 46  ---          16 49 45  20.4 253.8  4.3      55.4    60      877   21 45 47

21 47 15  NGC4418      16 50 14  20.1 256.0  4.4      56.2    23      877   21 47 15
21 51 15  ---          16 54 15  19.3 256.6  4.4      56.4   240      908   21 47 16

21 51 45  J1232        16 54 44  19.4 254.6  4.4      55.7    23      908   21 51 45
21 52 45  ---          16 55 44  19.2 254.7  4.4      55.8    60      915   21 51 46

21 53 14  NGC4418      16 56 13  18.9 256.9  4.5      56.5    23      915   21 53 14
21 57 14  ---          17 00 14  18.1 257.4  4.5      56.7   240      946   21 53 15

21 57 43  J1232        17 00 43  18.2 255.4  4.5      56.1    23      946   21 57 43
21 58 43  ---          17 01 44  18.0 255.6  4.5      56.1    60      954   21 57 44

21 59 12  NGC4418      17 02 13  17.7 257.7  4.6      56.8    23      954   21 59 12
22 03 12  ---          17 06 14  16.8 258.3  4.6      57.0   240      985   21 59 13

22 03 42  J1232        17 06 43  16.9 256.3  4.6      56.4    23      985   22 03 42
22 04 42  ---          17 07 43  16.7 256.5  4.6      56.4    60      992   22 03 43

22 05 11  NGC4418      17 08 12  16.4 258.6  4.7      57.1    23      992   22 05 11
22 09 11  ---          17 12 13  15.6 259.2  4.7      57.3   240     1023   22 05 12

22 09 40  J1232        17 12 42  15.7 257.2  4.7      56.7    23     1023   22 09 40
22 10 40  ---          17 13 43  15.5 257.3  4.7      56.7    60     1031   22 09 41

22 11 09  NGC4418      17 14 12  15.1 259.4  4.8      57.3    23     1031   22 11 09
22 15 09  ---          17 18 13  14.3 260.0  4.8      57.5   240     1062   22 11 10

22 16 02  J1256        17 19 05  17.5 251.6  4.4      54.8    40     1062   22 16 02
22 20 02  ---          17 23 06  16.6 252.2  4.4      55.1   240     1092   22 16 03

22 20 59  J1232        17 24 04  13.3 258.8  4.9      57.2    47     1092   22 20 59
22 21 59  ---          17 25 04  13.1 258.9  4.9      57.3    60     1100   22 21 00

22 22 29  NGC4418      17 25 33  12.7 261.0  5.0      57.8    23     1100   22 22 29
22 26 29  ---          17 29 34  11.9 261.5  5.0      57.9   240     1131   22 22 30

22 26 58  J1232        17 30 03  12.1 259.6  5.0      57.5    23     1131   22 26 58
22 27 58  ---          17 31 03  11.8 259.7  5.0      57.5    60     1138   22 26 59
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               Phase-referencing of NGC4418
  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
----------------------------------------------------------------------------------------

 --- Thu   6 Mar 2014   Day  65 ---

22 28 27  NGC4418      17 31 33  11.5 261.8  5.1      58.0    23     1138   22 28 27
22 32 27  ---          17 35 33  10.6 262.4  5.1      58.1   240     1169   22 28 28

22 32 56  J1232        17 36 03  10.8 260.4  5.1      57.7    23     1169   22 32 56
22 33 56  ---          17 37 03  10.6 260.6  5.1      57.7    60     1177   22 32 57

22 34 26  NGC4418      17 37 32  10.2 262.6  5.2      58.1    23     1177   22 34 26
22 38 26  ---          17 41 33   9.4 263.2  5.2      58.2   240     1208   22 34 27

22 38 55  J1232        17 42 02   9.5 261.2  5.2      57.9    23     1208   22 38 55
22 39 55  ---          17 43 02   9.3 261.4  5.2      57.9    60     1215   22 38 56

22 40 24  NGC4418      17 43 32   8.9 263.4  5.3      58.3    23     1215   22 40 24
22 44 24  ---          17 47 32   8.1 264.0  5.3      58.4   240     1246   22 40 25

22 44 54  J1232        17 48 02   8.3 262.0  5.3      58.1    23     1246   22 44 54
22 45 54  ---          17 49 02   8.0 262.2  5.3      58.1    60     1254   22 44 55

22 46 23  NGC4418      17 49 31   7.7 264.2  5.4      58.4    23     1254   22 46 23
22 50 23  ---          17 53 32   6.8 264.7  5.4      58.5   240     1285   22 46 24

22 50 52  J1232        17 54 01   7.0 262.8  5.4      58.3    23     1285   22 50 52
22 51 52  ---          17 55 01   6.8 263.0  5.4      58.3    60     1292   22 50 53

22 52 21  NGC4418      17 55 31   6.4 265.0  5.5      58.6    23     1292   22 52 21
22 56 21  ---          17 59 31   5.5 265.5  5.5      58.6   240     1323   22 52 22

22 56 51  J1232        18 00 01   5.7 263.6  5.5      58.4    23     1323   22 56 51
22 57 51  ---          18 01 01   5.5 263.8  5.5      58.4    60     1331   22 56 52

22 58 20  NGC4418      18 01 30   5.1 265.8  5.6      58.7    23     1331   22 58 20
23 02 20  ---          18 05 31   4.2 266.3  5.6  D   58.7     0     1362   22 58 21

23 09 09  J1256        18 12 21   6.4 259.2  5.3      57.7   397     1362   23 09 09
23 13 09  ---          18 16 22   5.6 259.7  5.3      57.9   240     1392   23 09 10


SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


 ======== Setup file: sess114.C1024
   Matching groups in /opt/sched/sched_11.0/catalogs/freq.dat:
     sh6cm           Update freq. range AnTao 22Mar08

   Setup group:    8         Station: SHANGHAI          Total bit rate:  1024
   Format: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00
             4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00
   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         2         1         2         3         4         3         4
                   5         6         5         6         7         8         7         8
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        C         A         C         A         C         A         C         A 
                  C         A         C         A         C         A         C         A 

  The following frequency sets based on these setups were used.

   Frequency Set:  10  Setup file default.  Used pcal sets:   1
   LO sum=   4942.49  4942.49  4942.49  4942.49  4974.49  4974.49  4974.49  4974.49
             5006.49  5006.49  5006.49  5006.49  5038.49  5038.49  5038.49  5038.49
   BBC fr=    742.49   742.49   742.49   742.49   774.49   774.49   774.49   774.49
              806.49   806.49   806.49   806.49   838.49   838.49   838.49   838.49
   Bandwd=     16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
               16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
    Matching frequency sets:  10

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 1MHZ
    PCALXB1=   S1    S3    S5    S7    S9    S11   S13   S15
    PCALXB2=   S2    S4    S6    S8    S10   S12   S14   S16
    PCALFR1=   490   510   490   510   490   510   490   510
    PCALFR2=   490   510   490   510   490   510   490   510

   Track assignments are: 
    track1=   2,  4,  6,  8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

   Source                         Source position (RA/Dec)                        Error
                        (B1950)             (J2000)             (Date)            (mas)

 * NGC4418           12 24 20.753136   * 12 26 54.612600     12 27 40.017185       0.00
                    -00 36 03.52524    *-00 52 39.37200     -00 57 32.25383        0.00
                     From catalog imbedded in main SCHED input file.

 * J1232             12 29 25.899380   * 12 32 00.015985     12 32 45.502055       0.00
                    -02 07 31.66618    *-02 24 04.79425     -02 28 56.46174        0.00
                     From catalog imbedded in main SCHED input file.

 * J1256             12 53 35.831298   * 12 56 11.166566     12 56 56.987968       0.00
                    -05 31 07.99587    *-05 47 21.52473     -05 52 05.88561        0.00
                     From catalog imbedded in main SCHED input file.



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
  NGC4418    sess114.C1024         1 2 3 4 5 6 9 10 11 12 13 1 +     6.200   363.199
  J1232      sess114.C1024         1 2 3 4 5 6 9 10 11 12 13 1 +     1.567    90.600
  J1256      sess114.C1024         1 2 3 4 5 6 9 10 11 12 13 1 +     0.533    35.333


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) 
   NGC4418            159.5
   J1232              157.8
   J1256              151.0

  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 

