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I just thought that many part of the notebook will use galaxy/PSF models to present example of a specific phenomena.
What do you think about having one function to draw them that every section can use to have all the galaxies looking the same? Of course this can be adjust for specific cases (when you need 2 galaxies for example)
I am proposing that after the discussion about blending bias where we have some example of the effect of blending and we will link that to an example of deblending. This would make more sense if they are the same images. I think other section would benefit from this.
We can discuss this point during one of the book telecon.
The text was updated successfully, but these errors were encountered:
I just thought that many part of the notebook will use galaxy/PSF models to present example of a specific phenomena.
What do you think about having one function to draw them that every section can use to have all the galaxies looking the same? Of course this can be adjust for specific cases (when you need 2 galaxies for example)
I am proposing that after the discussion about blending bias where we have some example of the effect of blending and we will link that to an example of deblending. This would make more sense if they are the same images. I think other section would benefit from this.
We can discuss this point during one of the book telecon.
The text was updated successfully, but these errors were encountered: