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I've spend sometime thinking about PR #83. It is really the AKARI+Spitzer scipack. This PR is fine as it is and should be merged once discussion is resolved.
For the future, would it be better to…
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As the attenuation law is not universal, one should use a model allowing different UV slope, 2175 bump strength whenever the spectral coverage allows it. For this purpose, one of the most used recipe …
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Since the spectral weight of each oscillator is an intrinsic property which is calculated from the parameters, it should be an always available attribute of any oscillator instance. Moreover, if the p…
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Hello,
First of all, thank you for the great book. It is a really useful read to understand spectral rendering in particular and the maths behind tracing. I have two questions that are hopefully ea…
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This will serve as a roadmap for the implementation of the "chunking" approach, which will eventually become a major mode of operation for Starfish. The rationale for doing this is that currently, fit…
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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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@keflavich When trying to fit some old VLA data I get the error message below. Here I'm trying to fit the NH3(1,1) line, and in the header it is stored as velocity. Is there something obvious I should…
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reported by: @CloudyLex
```
Title:
Stark broadening of lines from transition between states n = 3 to n = 2 in neutral helium. An experimental and computer-simulation study
Authors:
Gigosos, M. A.…
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It would be useful to have code that would use the saved sparse lnp files to generate a model spectrum+range or model spectra for the BEAST fits. This would allow comparisons from the BEAST fits to e…
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I tried to compare the results between CPU UMAP and GPU UMAP with fashion mnist dataset, it seems the CPU implementation is more accuracy from a visualization point. The comparison is made between br…