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#### Summary:
Reorganize the stan example repository and include predictive metrics for the purpose of a collective model set which will be used as the Bayesian computation benchmark.
#### Descri…
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RuntimeError: The size of tensor a (4) must match the size of tensor b (2) at non-singleton dimension 0
IterativeLatentUpscale[1/4]: 1452.0x1089.0 (scale:1.11)
!!! Exception during processing!!! …
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Hi,
Im using the `downscaleCV` function to test some GLM models with folds that within them, the years are not consecutive, for example:
fold1: 1979 1985 1991 1997 2003 2009
fold2: 1980 1986 1992…
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The title says it all. Encoding type it read from the second byte of sampling period, and compression byte is read from the encoding byte. Here is the patch:
```
--- convert/parsescp.c.orig 2018-1…
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Not much of a bug, but possibly a potenial improvement. `Picking.js`' [getRayIntersection](https://github.com/CesiumGS/cesium/blob/44ac2ff1293fc89cccfb58fc70f372123215261b/Source/Scene/Picking.js#L72…
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> thanks for you job,my question is :
raise KeyError("Non-existent config key: {}".format(full_key))
KeyError: 'Non-existent config key: MODEL.HEAD.DENSE_DEPTH
here is config:
MODEL:
INPLACE…
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work out how to put temporal effects in
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The stellar grid is currently based on isochrones. This the grid has uniform spacing in age, but non-uniform in mass. Isochrones are best for dealing with ensembles of stars, but not necessarily for…
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Hi there, thanks for making and maintaining this excellent project!
I was wondering why the covariance output of the predict function is a Matrix in the shape of the kernel function. As far as I ca…
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This might be a misunderstanding on my part, but currently we expect that the SelectOracle and PrepareOracle selection registers should match up (in terms of bitsizes) (this is assumed in #508), AND t…