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VLTI aperture #145
VLTI aperture #145
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One might want to get a vlt aperture without spiders but still having the segments. Therefore we have to define the spider_start/end anyway.
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Codecov Report
@@ Coverage Diff @@
## master #145 +/- ##
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- Coverage 80.93% 80.70% -0.23%
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Files 95 95
Lines 6923 7044 +121
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+ Hits 5603 5685 +82
- Misses 1320 1359 +39
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- Baselines vary as function of pointing on the sky. Currently, this function only returns the aperture for zenith pointing.
- Put pngs of the reference/baseline apertures as a comment.
I meant |
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Add changelog for v0.5.0.
I think the aperture will also change with azimuth. Think about two telescopes, what happens when you observe at the horizon and parallel to the telescopes, you will only see a single aperture. Should I also add the dOPD to the apertures ? Because the dOPD is Baseline * direction vector. |
Which is why I said "pointing on the sky" rather than "altitude". 😛
Maybe have a separate function for that rather than integrate it into FYI, I would be fine with just having a few sentences in the docstring without any extra implementation for non-Zenith pointing, ie. leave it as it is now. Whichever you feel like doing. The failed tests need to be fixed though. |
Ok. I can implement both next week. I have already done the coding for the different on-sky pointings. I was thinking you were only talking about altitude because you mentioned zenith. My brain just completely ignored azimuth at that point. |
Faster modulated pyramid wavefront sensor
All changes have been implemented, tests have been added. All checks have been passed. I think this is ready to be merged. |
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LGTM.
An implementation of the VLTI aperture. Based on the ESO P105 VLTI manual.