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Plotting the size of extended sources will make the life easier when studying crowded regions (e.g. Galactic plane).
For disk and Gaussian sources the r68 could be used (in this way they are easily c…
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The `base_mapper` plot function is bugged and sometimes will break the pipe.
Needs to investigate and fix, but low priority since I will no longer use it to generate input dataset for DL models.
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Hi,
I use the Skymap to identify the objects in sky. But to align the telescope in exactly position of the object is very hard. Is there a way to use the phone tied in the telescope and use the gyrosc…
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With the new environment variable `OPENBLAS_CORETYPE=Haswell` I am getting
```
tyuan@cobalt06:~$ singularity exec /cvmfs/icecube.opensciencegrid.org/containers/realtime/skymap_scanner\:3.14.9 python…
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Currently, the Skymap Scanner implements [frame object diff](https://docs.icecube.aq/icetray/main/projects/frame_object_diff/index.html) logic for GCD information.
Alerts coming from the pole carry…
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Also maybe the positions of the Sun and Moon would be helpful.
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Related to #126
LIGO/Virgo alerts are distributed through [GCN](https://gcn.gsfc.nasa.gov/) in VOEvent format, XML documents.
- [LIGO/Virgo Public Alerts User Guide](https://emfollow.docs.ligo.…
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Sometimes the final plot fails for cascades (today's example `run00136692.evt000006590287.HESE`).
```
arange: cannot compute length
```
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The distribution of the best seeing will affect our ability to deblend objects. To start to probe this, @pmelchior and I looked at the spatial distribution of the best seeing. For example, here's a …
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This is a general issue to discuss what changes we want to make to the follow-up strategy in advance of O4.
TODO: write a bit about the current system.