Dries Van De Putte
Dries Van De Putte
See for example these 1d pdfs of the phat small example, for the symlog of the F814W flux. Almost everything falls in the leftmost bins (lowest symlog). I think the...
Here next step for #280. Aside from the change in the features table introduced by #283, the user-facing `Model` things are basically unchanged (unless users were "digging for the astropy...
In our current design, the model details, fit settings and fit results are put together in the Model class. This brings some complexity with it: - We always have to...
[github.com/drvdputt/pahfit/tree/experimental ](https://github.com/drvdputt/pahfit/tree/experimental) has diverged quite far from master. But it is in working order, and I am actively using it for my science goals. There are many aspects which we...
Currently, the rows corresponding to unused features are masked out, so that they are displayed as a row of "--" when model.features is shown in a notebook. (reminder: unused means...
Just a little thing I noticed. https://github.blog/2022-08-15-the-next-step-for-lgtm-com-github-code-scanning/ Or we could just remove the LGTM checks for now.
PAHFIT can currently not work without specifying an instrument pack. This is a problem for cases where there is no reasonable instrument. Example use case: seeing how a PAHFIT decomposition...
There were a series of strange issues with the Features class in certain edge cases - There are only dust features (#274) - There are only lines (#266) - Exceptions...
We build an index for a Features table, so that rows can be accessed by the feature name. In certain contexts, this index is no longer available, so `.loc` will...
We should revise the MIRI MRS instrument packs. E.g. the maximum wavelength of ch4 long should be updated to 28.7 (there was a change in the pipeline that extended the...