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Now that astropy/astropy#4855 is merged, we can refactor the code to use that feature. But that feature is only for Astropy v2 or greater.
Related:
* astropy/astropy#6183
* https://gist.github.co…
pllim updated
2 weeks ago
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Couple of stuff to look at:
- [x] `07.Unsupervised_Learning-Transformations_and_Dimensionality_Reduction` fix `digits_plot` no output in jupyter-lab
- [x] `14.Model_Complexity_and_GridSearchCV` Av…
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Updated version of Kurucz models - including good wavelength coverage in the JWST range.
Ideally would replace CK04. Need to pick a reasonable resolution. And decide on what to do with the extra gr…
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# Deep visualizations
Deep visualizations is a technique to use neural networks as generative models for pictures/video. It would be cool to generate audio from a GAN but many tools already exist to …
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When I import astromodels.xspec, I get the following error:
ImportError: cannot import name '_xspec' from partially initialized module 'astromodels.xspec' (most likely due to a circular import) (/…
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Would the spectral norm get canceled out because it appears on both the nominator and denominator of the batch normalization equation?
I mean:
`bn(x*w/sn(w)) = gamma * (x*w/sn(w) - mean(x*w/sn(w))…
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Your work has been of great help for my research, so thank you very much first of all.
I was trying to implement your work on rotated mnist and CIFAR-10.
Here are my questions..
1)When tryin…
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(nllp) MacBook-Air-3:lnlp user$ python main.py tests/test_data/data.csv
Welcome to the NLLP CLI!
Loaded data from tests/test_data/data.csv
1. Run a Topic Model
2. Run an Optimization routine fo…
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Hi Julia,
I am currently trying to reconstruct your model and I have a few questions that I would like to clarify with you.
1. In your 2018 journal paper, you showed that architecture of your mo…
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Currently montblanc uses a spectral index model for the frequency axis
I(v) = I(v0)(v/v0)^alpha
In some cases it is preferable to fit a more flexible model. In particular it is not possible to fit i…