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Dear authors,
I am training the model on SVHN with coeff=0.3, after 200 epochs, many singular values are still larger than 1.
Are there any other parameters to be adjusted?
Best,
Liang
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Hi, inspired from your model, I have written a similar ESRGAN model with spectral_normalization and a few other tweaks. Although mostly, the underlying model architecture is same. I am also using VGG1…
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- [x] adapt Utsav's code from https://github.com/utsav-akhaury/ADMM/tree/main/ADMM_PnP_Radio
- [x] use the Tikhonov filtered image as initialization for the solution (first guess)
- [x] add shape…
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In the current cosmoDC2 model, for galaxies of the same stellar mass the distributions of restframe _(g-r)_ and _(r-i)_ colors of the two populations are identical:
- red sequence cluster galaxies …
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- DADVI ([paper](https://www.jmlr.org/papers/volume25/23-1015/23-1015.pdf)) pre-samples the Gaussian noise in the `init` and then is fully deterministic in `update` which makes for more stable trainin…
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i find citation 13,16,30 and do not know exact principle of hinge loss.
i feel confus…
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Our [advanced examples](https://librosa.org/doc/latest/advanced.html) gallery could be expanded in a few ways, especially toward covering different application areas like speech or bioacoustics. I'm …
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Interested in looking at the FFTs of the current profiles and the voltage profiles.
Could there be EMP contamination with the magnetic signals? I do not believe it would. So how would I check?
Th…
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## Data Analysis Question
GRID global minimization perhaps serves my purpose better since my model is not complex (_a log-parabola + Gaussian line(s)_). Let's call this **Model1**. From the [ThreeM…
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I'd like to have a function `spectral_distribution` which takes a kernel defined over R^d and returns in spectral distribution. For example
```julia
function spectral_distribution(k::SqExponential…