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- run ATpneumatics_checkout
- open dome: auxtel/atdome/open_dome.py
- open mirror covers (component: ATPneumatics, cmd: openM1Cover)
- enable corrections:
- With run command, disable dome following.
- run correct pointing (put range for target there)
- try to run latiss_wep_align to focus telescope - may not work, may have to do manual focus sweep
- NOTE: FIND CORRECT AZ POINTING FOR THE DOME
- Find targets of mag 12 +/- 1 at a large range of airmasses/elevations and take images of those without moving dome
- take_image_latiss as engtest → with g band in filter wheel, reason is on-sky, probably
- stop tracking
- point to MOSS and take a series of images there
- take_image_latiss
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Talked with Elana last week about usability of the images with different pulse durations. Had a lot of images that look quite bad, and Elana agrees that even a different centroiding algorithm might not be the most effective way to go.
Now want to:
- plot a window of anemometer data against the movement in x and y that was worrying with the temperature data previously
- figure out how the total standard deviation column is calculated such that it is less than the y in some cases
- compare in temperature for multiple sets of beam pairs
- change axis labels to aximuth and elevation after angle changes
- more clearly split out in the code where these angle changes are
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for the oscillatory motion over time, figure out if we fourier transform, is there a power spectrum
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Presentation from 11.11 Notes:
- We have hardware that seems to work with the slight issue that dome jitter contributes problems
- Broadly speaking, rms increases with image motion between pairs
- The sonic anemometer data seems to bear no significant relation to moss data
- Chris trusts MOSS more as it is still a more direct measurement of what we actually care about
- Episodic jumps between pairs with opening and closing between pairs
- We are not seeing systematic focal length shifts with temperature which is great!
- Image motion in x in y correlation - work in progress