David's Astronomy Pages
Notes - Session 624  (2018-09-01)

   
Bullet Session Aims & Highlights
 - Observing Result
 - Night Summary Plot
 
Bullet Operational Issues
  - Critical Issues (0),  Major Issues (1),  Minor Issues (2),  Small Defects (0),  Continuous Improvement (0)
 
Bullet Fully Automated Operation 
 
Bullet Autofocussing
 
Bullet Images from 2018-09-01  >>
 
 

2018-09-01 (Automated Operation Testing)


Session Aims & Highlights (2018-09-01)

Main aims

Main of this nighttime session were

  1. Targets. Acquire images for a selection of variable stars, nearby stars, star clusters
    (since moon illumination had dropped below 70% it was anticipated that Schedule Builder would include more Deep Sky Targets, e.g. galaxies, than in the last few sessions)  .
  2. Software. Test fixes & modifications made to the Observatory Control Program (CCDApp2) since the last session
  3. Stability. Continue checking stability of the Observatory system components (POTH.Hub , Telescope + Dome, Observatory Control Software, Computers)

Equipment & Software

Highlights

Summary Plots & Logs

Observing Result (2018-09-01, S624)
Observatory Unlocked at 01:11, Operations started at 01:15,
Fully-Automated Mode from 01:16, Job Queue started at 01:26, 
Scope Connection Problems (slew failures) from 03:06
Job Queue ended at 04:25. Session finished at 04:28
Image
(Observation Status :  Green=Completed, Yellow= Partially Completed, Red= Failed)
 
Night Sky Summary Plot - 2018-09-01
Top axis: Sky Brightness at Zenith (in ADU/s)
Lefthand axis: Local Time (hh LT). Righthand axis: Sun Altitude (degs)
Note: Wind Speed values are invalid on this night
 (Sensor had disconnected and VWS putting out constant value of 13.2 mph)
Image

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Operational Issues (2018-09-01, S624)

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Critical Issues

Major Issues

Minor Issues

Small Defects

Continuous Improvement

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Fig 1 'Timed out waiting for received data' error (whilst imaging Hickson 97)
Image

Fig 2.  'Timed out waiting for received data' error  (whilst imaging NGC 5322 & prior to slew to GCVS Z And )
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Autofocussing

An autofocussing run was inserted with Job Queue as part of executing the WDS GRB 34 target, which modified the focus position by 189 steps. The new data point (temperature 14.0°C) was later used to update the current Focus vs. Temperature graph and provide a new temperature corrected focus equation whose coefficients will be used for setting focus positions at the next session
    Focus Position = -127.8 * T + 4805, where T is temperature in °C

(It remains to be whether this equation is a good predictor of focus for temperatures at 3°C and below. The slope of line has been  has been getting less steep as more data in collected in the 9 to 14°C range but is this a consequence of  having more data to define for defining a best fit line or a measure of the uncertainty produced by the spread in measured focus at the same temperature )

Focus Profile (2018-09-01)
Image 
  
Close Up of Focus Profile
F0 is the position where the focuser was originally positioned
(in this case it was the position calculated from the best temperature based focus
coefficients determined from recent sessions). It’s not too bad, but it is clearly on the
low side of best focus on this night (or at least at this time).

F1a is the best focus position determined from the data and my automated curve fitting method.
(I use this to provide a corrective focus offset or empirical fix to the temperature
modelled focus position. I use this for the rest of the session or until superseded by a new offset) .


F1b is the focus position that I assume other methods might choose as the best focus which is
essentially where FWHM measurements were the lowest .
(This point is slightly offset on the higher side from F1a. Seeing and/or cloud condition was probably
just a bit better when the two points either side of F1b were taken
but probably doesn’t give an absolute picture of the best focus position.
Image 
 
Focus vs. Temperature Correlation  (2018-09-01) 
 Image

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