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Issue: the current default reference frequency for power law spectral models in BLIP is 25 Hz, which is a relic from ground-based interferometers. The more common choice for LISA is 1 mHz.
Steps:
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HelloI
I tried to rerun the program under MacOS (Sequoia 15.0).
Environment:
java 21.0.4 2024-07-16 LTS
nextflow 24.10.0
Docker version 27.3.1, build ce12230
On the test data, it stops pr…
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Hi @jjery2243542
Thank you for your paper and code.
I see spectral normalization in your code, not in your paper.
Does SN work? How is the effect?
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Hello,
Will the use of Conditional Batch Normalization in the generator cancel Spectral Normalization?
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I'm curious if you've tried the Spectral Normalization technic for your approach? At least at resolution 128^2 it didn't work for me
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I noticed earlier today that Haiku has SpectralNormalization -- very cool!
I'm interested in implementing an improved version, which does a much better job estimating the norm for convolutional lay…
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While I was debugging using the Wannier90 parser, I got some errors to be fixed (see [nomad-parser-wannier90#3](https://github.com/FAIRmat-NFDI/nomad-parser-wannier90/pull/3)):
- [ ] Change order o…
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Your spectral normalization normalizes the spectral norm of the weight matrix W so that it satisfies the Lipschitz constraint = 1. So we consider whether to combine the wasserstein gan with spectral n…
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## 一言でいうと
GANの要件であるDiscriminatorのLipschitzs制約を重要視し、Discriminatorの各層にSpectral Normalizationを適用することでGeneratorが精度の高い出力を得られるようになる。
### 論文リンク
* https://drive.google.com/file/d/0B8HZ50DPgR3eSVV6YlF…