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Sorry this might be very dumb on my side. I briefly remembers the eispac code uses Warren et al. 2014 to calibrate the files? Is there a place this is...

In [this notebook](https://github.com/sunpy/previous-workshop-notebooks/blob/master/2021_HinodeIRIS/tutorial.ipynb), there is an example of how to correct the EIS pointing by cross-correlating the 195.119 Fe XII intensity map with an AIA 193 Å image. There should...

Often when fitting a raster, there are parts of the raster, typically whole columns, where the line may not be able to be fit, either because of missing data or...

Dear all, I tried to apply a spatial binning over the vertical axis before fitting the data. I tried the "rebin" method from the NDcube class, but it replaces the...

There should be a note in the readme or somewhere in the docs saying to cite the JOSS paper as well as the Zenodo DOI for the specific version (if...

Hello, I was wondering what is the difference between the Doppler velocity maps and the non-thermal velocity maps? and how can I extract the non-velocity maps using the eispac? Here's...

Hello, I am studying a set of EIS observations but I noticed that there are not fit templates for all the lines in my dataset. Even for lines that spectral...

There are several places throughout the package where using units would be extremely helpful to both the user and in reducing the number of validation checks needed, e.g. `ccd_offset`, `rot_xy`....

Hi, I am trying to work with some sit and stare data. However, the keywords and plots refer to the time axis as a spatial one. It would great if...

When I load some data, astropy prints a message that says ``` INFO: uncertainty should have attribute uncertainty_type. [astropy.nddata.nddata] ``` I'm guessing this is because when uncertainties are loaded the...