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In 4.0b, it is possible to overlay spectra from matched cubes:
in 4.0, it doesn't work:
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It appears to be common to discuss low-level pixel data from infrared imaging sensors as having "engineering units" of "electrons per second". (Higher-level data products are often ultimately flux-ca…
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Hi all,
A feature that would be really useful would be the ability to show a colorbar and scale (even if min/max values) like e.g.
https://matplotlib.org/stable/api/_as_gen/matplotlib.pyplot.colorba…
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Try with:
* astropy 5.2 or later
* jdaviz 3.1.2 or later
```python
from astropy import units as u
from astropy.io import fits
from astropy.nddata import StdDevUncertainty
from astropy.wcs i…
pllim updated
4 months ago
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Works:
```
cube.moment0(axis=0).write('test.fits')
cube.moment0(axis=1)
```
Fails:
```
In [13]: s.moment0(axis=1).write('test.fits')
ERROR: InconsistentAxisTypesError: ERROR 4 in wcs_types() at lin…
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Withb `net9.0` `ComponentBase` has a new [`Assets`](https://source.dot.net/#Microsoft.AspNetCore.Components/ComponentBase.cs,53) property to load static mapped asset files (mainly CSS and javascript f…
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The luminosity calculation should take into account that flux units might be per pixel or per unit area, and I don't think we should default to a given pixel scale since there is no sensible default -…
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The following test failed in one of my PRs. Looked unrelated to my change, but its also only occured once so creating this issue to track.
https://github.com/dotnet/aspire/blob/cc9c8f3e657fb19b02cb…
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When reducing the SOFI imaging data, I have encountered 3 issues with the header keywords in the merged final images.
1) Compared to the old pipeline version 2.2.2 the new version 2.2.6 (and 2.2.4 a…
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The following countermeasures need to be complete in the Deployment section of the SDElements survey. A link to the SD elements dashboard can be found here (access through VA Network): https://sde.lig…