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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…
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# New Operator
### Describe the operator
The STFT operator was added to ONNX v17, and it's a major addition for a lot of audio models, as a lot of them rely either on spectrogram processing, or …
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I am playing around with your model to think about timescales for fabric evolution.
I can reproduce your demo result in /demo/fabric-evolution/run-fabric-evolution.py
However, if I change the num…
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Sorry for bother you again!
After you give the initialization code, we try to train with our own data. When we run the demo.py with our own initialization model, we find this question:
_size …
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Dear Haijin Zeng,
I am thoroughly impressed by your work and the pre-trained models you have shared. However, I currently do not have permission to access the pre-trained condition function and spe…
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Is there a possibility to add spectra of the following form?
dN/dE = F x (E/E_0) ^ ( -alpha - beta x log(E/E_0) )
Usually called log-parabolic form.
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Today.
https://heasarc.gsfc.nasa.gov/xanadu/xspec/issues/issues.html
although not all the web pages have been updated at this time. I just happened to notice the issues page had changed.
no i…
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Hi there,
With any input, the standard `ErrorModel` schema is generated.
spec
```yaml
ErrorModel:
type: object
properties:
type:
type: string
…
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z>2 Lyman-break galaxies are likely to be QSO contaminants so we should develop and include appropriate templates for this class of objects. My instinct is that the ELG templates may be sufficient bu…
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Hi there @pkuxmq , thanks for your great impressive work!
On reading the Appendix F.1 part, I'm a little bit confused about the restriction on ||W||.
Since the proof has been given that ||W||