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## ❓ Questions
Hi. When I use
**demucs -n htdemucs "Path"** commmand I get _"FATAL: htdemucs_ft is neither a single pre-trained model or a bag of models."_ message. What am I doing wrong? Thank…
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I noticed a strange behavior where after a logzsol value of 0.2 all points in a standard BPT diagram ([NII]/Hα, [OIII]/Hβ) are stuck to a certain value. I am using default stellar libraries: "mist" a…
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Using fitting.fit_continuum to fit a simple linear continuum to two continuum windows gives significantly different slopes for two different realizations of the noise. The chi^2 (by-eye) value someti…
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Make an IPython notebook that shows how to get the following data for every TeV source
* Spectral points
* How to dump spectral point data to text files
* Spectral global model (power-law or exp …
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From the [JOSS paper](https://github.com/openjournals/joss-papers/blob/joss.06323/joss.06323/10.21105.joss.06323.pdf), I see that "operators used inside SpeedyWeather.jl are exposed to the user, facil…
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I'm trying to calculate the equivalent width of a few absorption lines in a high res stellar spectrum my mentor provided me (size: 2.9 mb). I have a pretty simple piece of code for calculating equival…
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While discussing where to store the Gaunt factor for `Bremsstrahlung` emission model in #352, @Mateasek proposed to create a subpackage `cherab.default_data` to store the default atomic data distribut…
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From the radiative and functional models, create a sherpa model automagically, e.g.:
``` python
>>> from naima.models import create_sherpa_model, Synchrotron, PowerLaw
>>> SynPL = create_sherpa_model…
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Currently the code can model single stars with starspots @gully (with a single temp. and fill factor). We (@tofflemire, @gully and @edgillen) want to extend that to do full modelling of intrinsic (e.g…
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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…