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I really like your software, it makes it easier to judge the hype of powerlaws in datasets.
However, right now it focuses on fitting full datasets, creating their PDF and CDF on the fly. I'd like to …
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During the last coding sprint, @cgalelli and I tried to implement a generalised 1D model to
1. Avoid code duplication between temporal and spectral models
2. Enable an easy API for fitting other …
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To support tools for performing instrument-specific spectral analysis on SPICE data, the following generalized infrastructure must be developed/improved with the following priority:
| Functionality…
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**Reporter: Kyle Conroy**
To reproduce:
```
import numpy as np
from jdaviz import Specviz
import tempfile
from astroquery.mast import Observations
data_dir = tempfile.gettempdir()
fn =…
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This has come up several times now, and would be very useful for dealing with strongly shaped axes, racetrack/figure8 type shapes etc.
The main things to do:
- [x] Add a toroidal stream function…
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Hi, I am running Modelplot command as shown in the snippet. But everytime I am not getting the legends of the detectors in the plot. Is it a bug or do I need to make any change for that? Since there w…
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There are concerns that the current Stokes I fitting code may not be the best currently available (since it's based on the FORTRAN MINPACK-1 package from 1980). Some experimenting is needed to determi…
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### Provide a general description of the issue or problem.
The fitting infrastructure provided by @KriSun95 is a valuable addition to the package. To help modularity, flexibility and ease of maint…
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Right now the `QuantityModel` (as output by the fitting machinery) only accepts inputs with the *same* units as the spectrum.spectral_axis that was used to create it. It would be nice if it also reco…
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Gaussian Fitting is commonly used for fitting data like spectral line. (#22 is related issue)
This issue is to focus on the details and implementations of algorithms(a few kind of algorithms are in…