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reported by: @CloudyLex
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Title:
Stark broadening of lines from transition between states n = 3 to n = 2 in neutral helium. An experimental and computer-simulation study
Authors:
Gigosos, M. A.…
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* Novelty of the project
* The project proposal is well-prepared and detailed; thus, its novelty is highlighted by the idea of visualizing digital modulation schemes. To enhance the novelty, it is…
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**Submitting author:** @prashjha (Prashant K Jha)
**Repository:** https://github.com/prashjha/PeriDEM
**Branch with paper.md** (empty if default branch): joss
**Version:** v0.2.1
**Editor:** @matthewf…
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z>2 Lyman-break galaxies are likely to be QSO contaminants so we should develop and include appropriate templates for this class of objects. My instinct is that the ELG templates may be sufficient bu…
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Possible integration of the karabo with SPH-EXA Simulation.
1. Extra-Galactic Foreground
2. Studying Confusion limit in HI observations
3. For z=0 simulation mock data
4. Simulating observation of…
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- [x] Data axis selection should not update any of the 3D visualization plots
~~- [ ] Contour 3D seems to fail for many volumes, and it is slow computations, it could be replaced by dash_slicer http…
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### label
ICON-CLM-202407-1-1
### label_extended
ICON model in Climate Limited-area Mode (ICON-CLM), Version 202407-1-1
### source_id
ICON-CLM-202407-1-1
### source_type
ARCM
### release_year
…
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- Allow the SRW Spectral Flux report to run on NERSC.
- For idealized undulator, add the "Accurate" magnetic field treatment option (use the Approximate method by default for idealized simulations)…
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Two suggestions for possible improvement of the user-friendliness of the MICADO setup:
1) As indicated in #110, the current setup with three independent `FilterWheels` (`filter_wheel_1`, `filter_wh…
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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…