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Hello,
is there a way, by using the NED query, to directly obtain the spectral energy distribution (SED) of a source?
I am referring to the table provided in the "Photometry and SED" section of an…
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**Description**
- when making the IRFs (Aeff and sensitivity), the thrown energy histogram that is stored in the SimTel and DL1 files should be used for weighting, rather than the analytic model of…
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## Description of the issue
We want to introduce a number of new terms regarding solar meteorology into the OEO. The first question we should discuss is, how to structure them into the ontology. Th…
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### HW 10 Objectives
Due EOD: Friday April 5th
(I'm using the midterm hiatus to reset the numbering scheme to make the homeworks go with the week they are due)
1. Build a simple slab model fo…
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**Please describe the use case that requires this feature.**
When training any of the sklearn models currently implemented I want to (re-)weight events to e.g a different energy spectrum to use the s…
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this one:
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Somebody knows WITH CERTAINTY if (and where) the energy bias is corrected by Gammapy in check_flux_from_dl3.ipynb?
We (me and some other LST member, they can reveal themselves if they want to) modifi…
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Currently calls to RRTMG have no memory, meaning the seed is initialized within each call (If I understand it properly). That means that the cloud configuration is not really randomized, and I suspect…
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### Problem Description
For a Drude-Lorentz bath, the `HEOMSolver` can take `DrudeLorentzBath` (Matsubara decomposition) or `DrudeLorentzPadeBath` (Padé decomposition). A shifted Drude-Lorentz bath […
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Hi @andreatramacere,
Very glad to see the JetSet evolving so fast and now also having preliminary implementation for Galactic objects! 👏🏻
Isn't that the very first line on the documentation pag…