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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 |
(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) |
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TheSky6
connection to telescope stopped following 'Timed out waiting for received data '
error. After slewing to the second target in the night (Hickson 97) an
ASCOM Utilities dialog box appeared in TheSky6 saying 'Timed out waiting for
received data' and it was noted that the position of the telescope in
TheSky6's virtual sky was siting some two 2 degrees from the target, whilst real
the telescope was correctly pointing at the target (based on images being
received from camera and the telescope position being reported in the POTH
window). Concerned about the implications for the next slew the Scope was
manually disconnected and then reconnected in the TheSky6 after which the
telescope began appearing at the correct position on the virtual sky.
Later during the session a 'Timed out waiting for received data' error
again occurred whilst taking images of NGC 5322, and whilst automated
Operations were running unmonitored. (See Fig 1
& Fig 2) The following target (GCVS Z And) and
indeed all the remaining targets in the session failed as the telescope didn't
slew from its position still on NGC 5322. The slew failures were picked up by
the Job Queue executor as a discrepancy between the amount of slewed requested
and the amount of slew measured, and execution passed to the next target in turn
without imaging. This seems to be the first time that this problem
has been encountered, and at least the first time to see it in definite
isolation of other problems (i.e. not mixed in with multiple errors when the
Observatory System including TheSky6, POTH & LX200 have become totally unstable). Potential workaround: In the event of a detecting a slewing discrepancy it
might be worth commanding TheSky6 to disconnect / reconnect to the telescope and
then issue a further 'slew to target' command. It's unsure if the Error
Dialog box has to be acknowledged first, if so, it might prevent this workaround
from being successful.
Resolved in due course (TheSky6, UPB Powerbox)
Fig 1. 'Timed
out waiting for received data' error (whilst imaging Hickson 97)
Fig 2.
'Timed out waiting for received data' error
(whilst imaging NGC 5322 & prior to slew to GCVS Z
And )
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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) |
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. |
Focus vs. Temperature Correlation (2018-09-01) |
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This Web Page: | Notes - Session 624 (2018-09-01) |
Last Updated : | 2023-11-26 |
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