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The following code triggers the `RangesUpdate` event when using all the pan/zoom/reset tools, except for the `xwheel_pan` and `ywheel_pan` ones. I suspect this is not the intended behavior.
```
fr…
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### Instrument
Light curve fitting (Stages 4-6)
### What happened?
I'm using the WASP-39b ERS NIRSpec dataset, and I'm trying to fit a polynomial and step to it. I put values into the S5 fit_…
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Hi,
I am simulating a betatron radiation from LWFA electron beam. The radiation param I used is as attached. I run a test for 2000 steps (from 38000 to 40000) and plot the spectrum. The result I ob…
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Recently I've been thinking a bit about the future of big data in Electron Microscopy.
For the uninitiated: Due to increases in detector resolution and the increase of use of time-resolved EM, 4D …
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A "previous stages required" message should be displayed, but instead the screen takes forever to load nothing.
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Right now, we do not have special datastructures for IRFs, we use astropy quantities, numpy arrays.
This makes functions simpler and more flexible but an advantage of a specific datastructure would…
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Hi everybody!
After a welcoming meeting I had with this year GSoC mentors, @kandersolar and @AdamRJensen, and the other two participants, @RDaxini and @IoannisSifnaios, we were recommended to have …
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Arithmetic operations succeed so long as the flux arrays are of compatible shape, but do not check for equivalent spectral axis values. For example,
```
from specutils import Spectrum1D
import n…
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A number of people have asked following the rstudio::conf talk about how raster might be implemented in Arrow. Arrow serves a different purpose for raster (whose data buffers typically do not require …