Session Notes for AUST22 session
Prepared by Jing Sun, Vienna University of Technology
Prepared with VIE_SCHED
This session is for astrometry.

The current selection of sources is: (provided by Oleg Titov)
1. All sources for ASTROMETRIC sessions are selected in such way 
to be observed many times at higher elevation angles. Observing close to the horizont are not mandatory.
2. It is not necessary to cover the whole celestial sphere 
because this session is designed for ASTROMETRY but geodesy and EOP. 
Therefore, the northern hemisphere sources could be ignored without lost of precision.
3. A substantional number of ICRF2 defining sources having a good 
observational history is highly desirable to tie the newly observed targets 
with the well-established ones. Some of the potential ICRF2 defining 
candidated are observed occasionally, and their fluxes are not reliable. 
Therefore, I decided to rely on some strong ICRF2 defining sources for insurance. 
That's not a suprise that some of them have many observations collected by now.

===========================================================
----- Parameter listing --------------------------------------
 Experiment: AUST22                      Description AUST22/2014
 Scheduler:  VIEN                        Correlator: CRTN      
 Start:      2014-092-07:00:00           End:        2014-093-07:00:00
 Current yyyyddd:    2014092 (2014.25)  ( 56749 MJD, Wed 02Apr.)
 Greenwich sidereal time: 19:42:12  (07:00:00 UT)
 Sun's RA and DEC:   00h45.9m   4d55.5
===========================================================
First observations
Observation listing from file ./aust22.skd  for experiment AUST22   
Source      Start      DURATIONS                                           
name     yyddd-hhmmss   Hh  Hb  Ke  Ww  Yg
0122-003 14092-070000   93 303 284     303|    
0700-197 14092-070555      169 163 169 169|                                                                                                                                                                                                                                                                                                                                                                                    
......
End of listing.
===========================================================
Last observations
Observation listing from file ./aust22.skd  for experiment AUST22
Source      Start      DURATIONS                                           
name     yyddd-hhmmss   Hh  Hb  Ke  Ww  Yg
......                    
2030-689 14093-065101  147 482     482 482|
0758-737 14093-065958      482 434 482 482|
End of listing.
===========================================================

   SKED Summary from file ./aust22.skd  for experiment AUST22    

      (all scans with at least one subnet station)

 Average number of obs. per baseline per source(normalized by up-time) =     6.0
 Min =      1  Max =     15 (Baseline Hb-Ww on 1030-590 )  RMS =   6.8

 Total time:    1440.0 minutes (  24.0 hours)

 Key:     Hh=HARTRAO    Hb=HOBART12   Ke=KATH12M    Ww=WARK12M    Yg=YARRA12M   
                   Hh   Hb   Ke   Ww   Yg   Avg
 % obs. time:      13   81   56   69   77   59
 % cal. time:       3    4    3    3    4    3
 % slew time:      29    7    5    7    8   11
 % idle time:      55    9   36   21   11   26
 total # scans:   135  204  162  174  237  182
 # scans/hour :     6    9    7    8   10    8
 Avg scan (sec):   86  343  298  345  280  270
 Total GBytes:   1447 8759 6032 7501 8308 6409

      # OF OBSERVATIONS BY BASELINE
  |  Hh   Hb   Ke   Ww   Yg   StnTotal
--------------------------------------
Hh|       70   63   46  131     599
Hb|           136  168  172    1086
Ke|                121  153     967
Ww|                     137     953
Yg|                            1147

 Number of  2-station scans: 83
 Number of  3-station scans: 50
 Number of  4-station scans: 114
 Number of  5-station scans: 28

 Total # of scans, observations:   275     1197
===========================================================

If you have any questions, 
please contact Jing Sun (jing.sun@tuwien.ac.at) or 
Johannes Boehm (Johannes.Boehm@geo.tuwien.ac.at).