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using lcviz for non Kepler or Tess data #66
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lcviz depends strongly on using a lightkurve object under-the-hood, but if there isn't an automatic parser for your data, you should be able to parse it externally manually and then pass arrays directly to lightkurve before loading into lcviz. If that gives you any problems with your data, please do let us know and we can try to fix it. We are hoping to do an official first release soon, but just note that there may be some API breaking changes between now and then. If you have any suggestions for improvements, let us know! |
Dear Kyle, |
Fantastic - glad to hear that you got it working and you're finding lcviz useful! If you think your changes are general and useful to be added to lightkurve, please consider opening a PR there. Otherwise, if you want to post a snippet here, someone might find that helpful if they want to try something similar on their end in the future. Access to subsets from the public API doesn't exist quite yet, but you can call internal methods (this is read-only, so safe to do so... the output just isn't convenient and the API is subject to change without deprecation, etc): Hope this helps! |
Thank you for the response, I have tried you suggestion and it works! Will there be a public API in the near future to access the subsets, as we would like to make this a permanent part of the jupyter notebook threads used for xmm-sas analysis? |
Probably not in the immediate future, but its definitely in our plans (for jdaviz, which will then be adopted here as well). I'll close this issue since it seems the lightkurve workaround is doing the trick for you, and open a new one to track that (feel free to subscribe to it). I also opened the discussion tab on the repo in case you have any suggestions or questions that don't fall under "issues". |
Hello,
I have been very interested in exploring the interactive plotting opportunity lcviz offers for displaying light curves, however no matter how much I looked and tried it myself I could not use it for my own fits file which is XMM-Newton data and not Kepler nor Tess. I saw that at the page it is mentioned that lcviz is not limited to the use of Kepler and Tess, however I could not find any guidelines nor figure it out myself. At the current stage of it, is it possible to open our custom files without using lightkurve, or is this something under development?
Many thanks :)
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