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HD 143006 Imaging Tutorial Part 1 #61
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Is the main focus to compare DSHARP with the dirty image (i.e. that's what we should focus on explaining)? I know a lot of the code is very similar to some of the smaller tutorials and I want to make sure the scope of this tutorial is wide enough to get the point across but without running into any problems of duplicating too much of the smaller tutorials. |
I think the main goal of this part I tutorial is to familiarize the reader with the DSHARP dataset. The code for gridding, producing the dirty image, and displaying it will indeed be familiar with the other tutorials. The comparison with the DSHARP FITS image is basically to show that our MPoL-produced dirty image looks similar to the actual FITS CLEAN image provided by the survey. (Of course, the MPoL dirty image still has sidelobe responses because it hasn't been "cleaned"). |
Okay thank you! |
Added file HD143006_Tut_P1 to docs/tutorials folder Modified Makefile and index.rst for the addition of the new tutorial Collaboration on tutorial with: @trq5014, @hgrzy, @RCF42 Tutorial to close Issue MPoL-dev#61
Closed by #74 |
An overview of the HD 143006 imaging series is provided in #25
Part I should cover
So the main contents of this tutorial will be
.npz
file available for download here, which can follow theastropy
loading in other tutorials.The text was updated successfully, but these errors were encountered: