Peter Melchior

Sure! I think what you're asking is how to compute the log probabilities of some spectra with the pretrained flow, right? If so, this should work ```python desi, model =...

I should let you know that as of version 0.2.6, we recommend a standard `pip install spender` and then this pattern: ```python flow = spender.hub.load('desi_edr_galaxy_flow', map_location=accelerator.device) desi, model = spender.hub.load('desi_edr_galaxy',...

The file organization is part of our SDSS data model. You can use the function `SDSS.save_in_batches` to created the necessary file structures. In short, we bundle N=1024 spectra into one...

We're working on a simpler data loading approach, but in the meantime, this should work: ```python from spender.data.sdss import SDSS dir = "your_storage_directory" # get all IDs from master catalog,...

+1 for this request. I have tried to install the package in python 3.9 and recent versions of cython, but failed.

Thanks for reporting. I think `nside` is treated correctly, but we don't get the see the expected result. Here's why I think this happens: 1. `map.density` only plots the non-empty...

Yeah, but you see the effect of item 2: the map is pixelized. So, what you see are not the healpix cells but the resolution limit of your backend _before...

OK, that needs to get fixed! Let me see what's going on.

Have you done any runtime tests on interpolated images? I have done some testing on scarlet2, where we implement the same Bernstein&Gruen method, and see massive costs even if the...

Thanks! Benjamin did check the code here. My question is: do you have runtime numbers for an Fourier resampling method?