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Hey, I wanted to ask if you planned on implementing the BCMultiTemplateFitter from the C++ version. Or if there is anything similar in the Julia version. This would be very useful when fitting multipl…
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### What is the problem this feature will solve?
A common problem is wanting to fit along the spectral axis of a higher dimensional data cube, for example having a 3D space - space - wavelength cub…
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Some repos
- [BVEP](https://github.com/ins-amu/bvep)
- [tvb-inversion](https://github.com/the-virtual-brain/tvb-inversion)
- [whobpyt](https://github.com/JohnGriffiths/whobpyt)
have some sta…
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### Description
Seeing `test_fitting_with_initial_values[DogBoxLSQFitter]` fail with numpy 1.26.0 installed from MambaForge/Miniforge3 on an M1 Mac.
### Expected behavior
Fit should converge …
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We need PSD-based methods for fitting models with frequency-specific weighting. See branch:model_fitting for progress. I've been working for a few months on this, but not quite done. To complete, we n…
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**A description of identification and classification of HCO+ baseline fitting issues in the TP data (SPW 21)**
**Identification:** Baseline issues can be identified in plots from the HSD_Baseline t…
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The normalization of the global covariance is described by a free parameter `logAmp` (the actual normalization is `(10**logAmp)**2`). But if such normalization is much higher than the median value of …
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What is the correspondence between parameters of simple analytical model and the parameters used by spinW to evaluate such models? Difference should be either eliminated or clearly explained in user m…
abuts updated
3 weeks ago
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Hello,
Hello, I am relatively new to Orange(and data mining) and wanted to ask for advice. I am fitting a bunch of spectral data to Fano (see picture). The fits are pretty sharp, partly due to the …
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This is driven by astropy/specutils#303. When fitting spectral lines, we want to know which parameter of a model is the "center". In `specutils` the planned solution for now is to just guess based o…