Kyle Westfall
Kyle Westfall
The passband integration errors, used for both the emission-line moments and the spectral indices, are likely very poor. We've known this for a while given MC experiments from Portsmouth and...
The setup of the parameters for the main wrapper classes should be streamlined by adding a method that does the setup from a config (*.ini) file. This improves the clarity...
Users want to "stop" the code before it completes all the analysis steps and have it still write the MAPS and LOGCUBE files. This was an intended functionality but fails.
Within the current infrastructure, would it be possible to select which properties are used to construct the box and whisker plots? Could we add properties from the DAPall file as...
### Description Addresses #16648 . This is a basic port of a nearly identical class from the MaNGA data-analysis pipeline. This is a basic utility class that allows for the...
Addresses #1149 . This requires the new `Covariance` subclass of `astropy.nddata.NDUncertainty`; see https://github.com/astropy/astropy/pull/16690. When on the `covariance` branch in astropy, this is functional code, but I have punted on some...
As titled. Addresses #849 . ------ - [x] For new contributors: Did you add yourself to the "Authors.rst" file? For documentation changes: - [ ] For documentation changes: Does your...
astropy==6.1.4 ccdproc==2.4.2 numpy==2.1.2 The current implementation of `Combine.sigma_clipping` overwrites any existing mask. Is that intended? I.e., instead of: ``` self.data_arr.mask = sigma_clip(self.data_arr.data, sigma_lower=low_thresh, sigma_upper=high_thresh, axis=kwd.get('axis', 0), copy=kwd.get('copy', False), maxiters=kwd.get('maxiters', 1),...