Kris Cooper
Kris Cooper
Separate more of the instrument specific code from the more general fitting code. Remove the ability to pass files and dictionaries directly to the fitter. instead, the files (or dictionaries)...
This tackles a subset of the points raised in #81 where we define the format of the instrument data to be fitted. The aim is to ensure that the loading...
### Describe the bug Issue when using `numpy.float64` numbers for the parameters in `sunxspex.emission.bremsstrahlung_thick_target` as it ends up returning all `nans` and `infs`. Weirdly, rounding to 15 decimal places with...
### Describe the feature Previously, only files and dictionaries containing data to be fitted could be passed to the fitting code. This was improved in #107 where a bug was...
Overall Issue: Fit NuSTAR spectra - spectra are dominated by bright 2-4MK source and want to test whether the additional low count-rate emission at higher energies is real (i.e. consistent...
This PR aims to start introducing code in the fitting refactor, first aiming to implement `astropy` models (discussion started in #81). A few scripts are included into the `fitting` module...
## PR Description As described in #147 , this draft shows how the gain can be applied in `sunkit-spex` as it is applied in XSPEC. More discussion is needed but...
### Provide a general description of the issue or problem. It turns out that the gain correction (if applied) being performed in `fitting_legacy` is not being done in the same...
### Provide a general description of the issue or problem. This issue is just to highlight a To-do item: **to scan through the package and remove placeholder code that might...