  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Maser imaging
 Exp. Code:  GA037B  


Schedule Version:       1.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       Alexei Alakoz

Address:  ASC Lebedev
          Profsoyuznaya 84/32
          117997 Moscow, Russia
 

Phone:    +7-495-3332167
EMAIL:    alexey.alakoz@gmail.com
Fax:      +7-495-3332378
Phone during observation: +7-916-5452842

Observing mode: K-band, dual-pol

Notes:    K-band, Radioastron-compatible frequency setup
          P-CAL is OFF, Tsys is ON
          auto-level (AGC) is ON
          Please, send Mk5 disk packs to JIVE


COVER LETTER:

Project: Tracing micro-structures of H2O masers with ultimate angular resolution

RadioAstron-EVN out of session observations of W51 M/S

K-band, dual-polarization

Observational code: rags15b (RadioAstron), GA037B (ground)
Proposals: RA-AO3-02; GA037;
Task:  Maser imaging
Start(UT): 08.10.2015 15:00:00
Stop(UT) : 09.10.2015 00:00:00
Band: KK
Pcal: OFF, noise diode: ON
Source: W51_E8_H2O, 1923+210, 1928+154
GRT: Jb2(K), Ef(K), Nt(K), Sh(K), Ur(K), Tr(K), Ys(K), Ro(K:23:30-02:25), Hh(K)
SRT:  15:00-15:10; 15:20-15:50; 19:00-19:40; 19:50-20:00; 22:35-23:25
Comments: 1.7xED  PA=29.4
Comments: 22236 MHz

Comments:

Space Radio Telescope (SRT):
Records dual-polarization LSB and USB 16 MHz wide IFs of
the central frequency 22236.00 MHz, two IFs per polarization.
Bitrate: 128 Mbps (1-bit sampling)
Green Bank tracking station is used.

Ground:
Records dual-polarization LSB and USB 16 MHz wide IFs of
the central frequency 22236.00 MHz, two IFs per polarization.
Bitrate: 256 Mbps (2-bit sampling)

*** Please make sure that PCAL is OFF. Thanks! ***

Correlation:
This experiment will be correlated by the JIVE-SFXC correlator & ASC correlator.
Please, send all the data as disks or e-transfer to JIVE, then data will be forwarded to ASC (Moscow).

Alexei
Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Maser imaging
  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   8 Oct 2015   Day 281 ---

 ---------- Space-ground K-band fringe finder scan ----------

 Next scan frequencies:  22236.00  22236.00  22236.00  22236.00
 Next BBC frequencies:     636.00    636.00    636.00    636.00
 Next scan bandwidths:      16.00     16.00     16.00     16.00

15 00 00  1923+210     00 12 30  26.1 280.0  4.8      64.7     0        0   15 00 00
15 10 00  ---          00 22 32  24.0 281.1  4.9      64.3   600       19   15 00 01

 ---------- Ground-only K-band VLBI scans ----------

15 11 00  W51_E8_H2O   00 23 32  20.3 275.1  5.0      61.8    50       19   15 11 00
15 12 00  ---          00 24 32  20.1 275.2  5.0      61.8    60       21   15 11 01

15 12 00  1922+155     00 24 32  20.9 276.2  5.0      62.2    -5       21   No stop 
15 13 00  ---          00 25 33  20.7 276.4  5.0      62.1    55       23   15 12 01

15 13 00  W51_E8_H2O   00 25 33  19.9 275.4  5.0      61.7    -5       23   No stop 
15 14 00  ---          00 26 33  19.7 275.5  5.0      61.7    55       25   15 13 01

15 14 00  1922+155     00 26 33  20.4 276.5  5.0      62.1    -5       25   No stop 
15 15 00  ---          00 27 33  20.2 276.6  5.0      62.1    55       27   15 14 01

15 15 00  W51_E8_H2O   00 27 33  19.5 275.6  5.1      61.7    -5       27   No stop 
15 16 00  ---          00 28 33  19.3 275.7  5.1      61.7    55       29   15 15 01

15 16 00  1922+155     00 28 33  20.0 276.7  5.1      62.1    -5       29   No stop 
15 17 00  ---          00 29 33  19.8 276.8  5.1      62.0    55       31   15 16 01

15 17 00  W51_E8_H2O   00 29 33  19.0 275.9  5.1      61.6    -5       31   No stop 
15 18 00  ---          00 30 33  18.8 276.0  5.1      61.6    55       33   15 17 01

15 18 00  1922+155     00 30 33  19.6 277.0  5.1      62.0    -5       33   No stop 
15 19 00  ---          00 31 34  19.4 277.1  5.1      62.0    55       35   15 18 01

 ---------- Space-ground water maser scans (K-band) ----------

15 20 00  W51_E8_H2O   00 32 34  18.4 276.2  5.1      61.6    55       35   15 20 00
15 30 00  ---          00 42 35  16.3 277.4  5.3      61.3   600       54   15 20 01

15 31 00  W51_E8_H2O   00 43 35  16.1 277.6  5.3      61.3    58       54   15 31 00
15 40 00  ---          00 52 37  14.2 278.6  5.5      61.0   540       71   15 31 01

15 41 00  W51_E8_H2O   00 53 37  13.9 278.8  5.5      61.0    58       71   15 41 00
15 50 00  ---          01 02 39  12.0 279.9  5.6      60.6   540       88   15 41 01
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Maser imaging
  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   8 Oct 2015   Day 281 ---

 ---------- Ground-only K-band VLBI scans ----------

15 52 00  W51_E8_H2O   01 04 39  11.6 280.1  5.7      60.6   118       88   15 52 00
15 53 00  ---          01 05 39  11.4 280.2  5.7      60.5    60       90   15 52 01

15 53 00  1922+155     01 05 39  12.2 281.2  5.7      60.8    -5       90   No stop 
15 54 00  ---          01 06 39  12.0 281.3  5.7      60.7    55       92   15 53 01

15 54 45  W51_E8_H2O   01 07 24  11.0 280.4  5.7      60.5    40       92   15 54 45
15 55 45  ---          01 08 25  10.8 280.6  5.7      60.4    60       94   15 54 46

15 55 45  1922+155     01 08 25  11.6 281.5  5.7      60.7    -5       94   No stop 
15 56 45  ---          01 09 25  11.4 281.6  5.7      60.6    55       96   15 55 46

15 56 45  W51_E8_H2O   01 09 25  10.6 280.7  5.7      60.4    -5       96   No stop 
15 57 45  ---          01 10 25  10.4 280.8  5.8      60.3    55       98   15 56 46

15 57 45  1922+155     01 10 25  11.2 281.7  5.8      60.6    -5       98   No stop 
15 58 45  ---          01 11 25  11.0 281.9  5.8      60.5    55      100   15 57 46

15 58 45  W51_E8_H2O   01 11 25  10.2 280.9  5.8      60.3    -5      100   No stop 
15 59 45  ---          01 12 25  10.0 281.1  5.8      60.3    55      102   15 58 46

15 59 45  1922+155     01 12 25  10.7 282.0  5.8      60.5    -5      102   No stop 
16 00 45  ---          01 13 25  10.5 282.1  5.8      60.4    55      104   15 59 46

16 00 45  W51_E8_H2O   01 13 25   9.8 281.2  5.8      60.2    -5      104   No stop 
16 01 45  ---          01 14 26   9.6 281.3  5.8      60.2    55      106   16 00 46

16 01 45  1922+155     01 14 26  10.3 282.2  5.8      60.4    -5      106   No stop 
16 02 45  ---          01 15 26  10.1 282.3  5.8      60.3    55      108   16 01 46

16 02 45  W51_E8_H2O   01 15 26   9.3 281.4  5.8      60.1    -5      108   No stop 
16 03 45  ---          01 16 26   9.1 281.5  5.9      60.1    55      110   16 02 46

16 03 45  1922+155     01 16 26   9.9 282.5  5.9      60.3    -5      110   No stop 
16 04 45  ---          01 17 26   9.7 282.6  5.9      60.2    55      112   16 03 46

16 05 30  W51_E8_H2O   01 18 11   8.8 281.8  5.9      60.0    40      112   16 05 30
16 06 30  ---          01 19 11   8.6 281.9  5.9      60.0    60      113   16 05 31

16 06 30  1922+155     01 19 11   9.3 282.8  5.9      60.2    -5      113   No stop 
16 07 30  ---          01 20 11   9.1 282.9  5.9      60.1    55      115   16 06 31
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Maser imaging
  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   8 Oct 2015   Day 281 ---

16 07 30  W51_E8_H2O   01 20 11   8.3 282.0  5.9      59.9    -5      115   No stop 
16 08 30  ---          01 21 12   8.1 282.1  5.9      59.9    55      117   16 07 31

16 08 30  1922+155     01 21 12   8.9 283.0  5.9      60.1    -5      117   No stop 
16 09 30  ---          01 22 12   8.7 283.2  5.9      60.0    55      119   16 08 31

16 09 30  W51_E8_H2O   01 22 12   7.9 282.2  6.0      59.8    -5      119   No stop 
16 10 30  ---          01 23 12   7.7 282.4  6.0      59.8    55      121   16 09 31

16 10 30  1922+155     01 23 12   8.5 283.3  6.0      60.0    -5      121   No stop 
16 11 30  ---          01 24 12   8.3 283.4  6.0      59.9    55      123   16 10 31

16 11 30  W51_E8_H2O   01 24 12   7.5 282.5  6.0      59.7    -5      123   No stop 
16 12 30  ---          01 25 12   7.3 282.6  6.0      59.7    55      125   16 11 31

16 12 30  1922+155     01 25 12   8.1 283.5  6.0      59.9    -5      125   No stop 
16 13 30  ---          01 26 12   7.9 283.6  6.0      59.8    55      127   16 12 31

16 13 30  W51_E8_H2O   01 26 12   7.1 282.7  6.0      59.6    -5      127   No stop 
16 14 30  ---          01 27 13   6.9 282.9  6.0      59.6    55      129   16 13 31

16 14 30  1922+155     01 27 13   7.7 283.8  6.0      59.8    -5      129   No stop 
16 15 30  ---          01 28 13   7.5 283.9  6.0      59.7    55      131   16 14 31

16 16 15  W51_E8_H2O   01 28 58   6.5 283.1  6.1      59.5    40      131   16 16 15
16 17 15  ---          01 29 58   6.3 283.2  6.1      59.5    60      133   16 16 16

16 17 15  1922+155     01 29 58   7.1 284.1  6.1      59.6    -5      133   No stop 
16 18 15  ---          01 30 58   6.9 284.2  6.1      59.6    55      135   16 17 16

16 18 15  W51_E8_H2O   01 30 58   6.1 283.3  6.1      59.4    -5      135   No stop 
16 19 15  ---          01 31 58   5.9 283.5  6.1      59.4    55      137   16 18 16

16 19 15  1922+155     01 31 58   6.7 284.4  6.1      59.5    -5      137   No stop 
16 20 15  ---          01 32 59   6.5 284.5  6.1      59.5    55      138   16 19 16

16 20 15  W51_E8_H2O   01 32 59   5.7 283.6  6.1      59.3    -5      138   No stop 
16 21 15  ---          01 33 59   5.5 283.7  6.2      59.3    55      140   16 20 16

16 21 15  1922+155     01 33 59   6.3 284.6  6.1      59.4    -5      140   No stop 
16 22 15  ---          01 34 59   6.0 284.7  6.2      59.4    55      142   16 21 16

16 22 15  W51_E8_H2O   01 34 59   5.3 283.8  6.2      59.2    -5      142   No stop 
16 23 15  ---          01 35 59   5.1 284.0  6.2      59.2    55      144   16 22 16
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Maser imaging
  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   8 Oct 2015   Day 281 ---

16 23 15  1922+155     01 35 59   5.8 284.8  6.2      59.3    -5      144   No stop 
16 24 15  ---          01 36 59   5.6 285.0  6.2      59.2    55      146   16 23 16

16 25 15  1922+155     01 37 59   5.4 285.1  6.2      59.2    58      146   16 25 15
16 26 15  ---          01 39 00   5.2 285.2  6.2      59.1    60      148   16 25 16

16 29 45  2200+420     01 42 30  45.5 300.6  3.7      86.0   138      148   16 29 45
16 39 45  ---          01 52 32  43.6 300.8  3.8      84.5   600      167   16 29 46


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


 ======== Setup file: ra1cm2.set
   Matching groups in ./ga037b_freq.dat:
     sh1cm           From Porcas, from Huang Xinyong 231198

   Setup group:    1         Station: SHANGHAI          Total bit rate:   256
   Format: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels:  4    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=  21600.00  21600.00  21600.00  21600.00
   Net SB=         L         L         U         U
   IF SB =         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP 
   BBC   =         1         2         1         2
   BBC SB=         L         L         U         U
   IF    =        C         A         C         A 

  The following frequency sets based on these setups were used.

   Frequency Set:   4  Setup file default.  Used with PCAL = off
   LO sum=   22236.00  22236.00  22236.00  22236.00
   BBC fr=     636.00    636.00    636.00    636.00
   Bandwd=      16.00     16.00     16.00     16.00
    Matching frequency sets:   4

   Track assignments are: 
    track1=   6,  8,  2,  4
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * FAKERA            11 57 21.769299   * 12 00 00.000000     12 00 27.840860       0.00
                     85 16 41.77889    * 85 00 00.00000      84 54 39.41181        0.00
                     From catalog imbedded in main SCHED input file.
                     fake circumpolar target for a TS to look at

 * W51_E8_H2O        19 21 26.266096   * 19 23 43.934270     19 24 27.430383       0.00
                     14 24 34.98638    * 14 30 28.34980      14 32 42.15158        0.00
                     ./ga037b_sources.radioastron
                     H2O maser; position of the reference maser feature from 2010ApJ720...1055Sato, R

 * 1928+154          19 28 36.092068   * 19 30 52.766993     19 31 36.000232       0.00
   J1930+1532        15 26 11.96581    * 15 32 34.42720      15 34 57.53879        0.00
                     ./ga037b_sources.radioastron
                     clock offset calibrator for W51_E8, rfc_2013d Petrov, 2013, unpublished 139 obse

 * 1922+155          19 22 23.129975   * 19 24 39.455869     19 25 22.540606       0.00
   J1924+1540        15 34 46.75053    * 15 40 43.94156      15 42 59.24528        0.00
                     ./ga037b_sources.radioastron
                     phase reference source for W51, rfc_2015c Petrov

 * 1923+210          19 23 49.792392   * 19 25 59.605355     19 26 40.674741       0.00
   J1925+2106        21 00 23.30483    * 21 06 26.16191      21 08 44.60060        0.00
                     ./ga037b_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 35453 observations, RA-AO3-04

 * 0316+413          03 16 29.567283   * 03 19 48.160114     03 20 52.657952       0.00
   J0319+4130        41 19 51.91847    * 41 30 42.10559      41 33 57.01230        0.00
   3C84              ./ga037b_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 15448 observations, RA-AO3-04, RA-AO2-1

 * 2200+420          22 00 39.362504   * 22 02 43.291371     22 03 24.019410       0.00
   J2202+4216        42 02 08.59073    * 42 16 39.97987      42 21 34.82854        0.00
   BLLAC             ./ga037b_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 59417 observations, RA-AO3-04, RA-AO2-1



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
  FAKERA     ra1cm2.set            10                                2.183     0.000
  W51_E8_H2O ra1cm2.set            1 2 3 4 5 6 7 8 9                 3.983    78.251
  1928+154   ra1cm2.set            1 2 3 5 6 8 9                     0.167     3.500
  1922+155   ra1cm2.set            1 2 3 4 5 6 7 8 9                 2.033    32.324
  1923+210   ra1cm2.set            1 2 3 4 5 6 7 8 9                 0.167     6.000
  0316+413   ra1cm2.set            1 2 3 5 6 8 9                     0.391     4.967
  2200+420   ra1cm2.set            1 2 3 4 5 6 7 8 9                 0.750    18.461


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) 
   FAKERA              91.0
   W51_E8_H2O          98.4
   1928+154           100.2
   1922+155            98.7
   1923+210            99.3
   0316+413           132.0
   2200+420           127.3

  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 

