-
My progress so far for this project has been in completing spectral analysis on 5 young stars. Phase one, in which I complete by-eye fittings of models to data on the give spectra using the PHOENIX da…
-
There are concerns that the current Stokes I fitting code may not be the best currently available (since it's based on the FORTRAN MINPACK-1 package from 1980). Some experimenting is needed to determi…
-
Hey, I wanted to ask if you planned on implementing the BCMultiTemplateFitter from the C++ version. Or if there is anything similar in the Julia version. This would be very useful when fitting multipl…
-
At the end of the sky subtraction fit, we could consider fitting for a residual spectral background per CCD amplifier, either a constant term or a linear function of wavelength and a polynomial functi…
-
When converting simulated PHA data from a `gdt.core.simulate.pha.PhaSimulator` object to a `gdt.core.pha.PHA` object using `gdt.core.simulate.pha.PhaSimulator.to_pha`, setting the energy_range attribu…
-
Fabio Acero talk at the Chandra Workshop presented the results of 3D spectral-spatial analysis of Cas A. He combined Sherpa (models and I/O) and gamma-py (3D) to perform the fitting. Sherpa needs to b…
-
### What is the problem this feature will solve?
A common problem is wanting to fit along the spectral axis of a higher dimensional data cube, for example having a 3D space - space - wavelength cub…
-
Some repos
- [BVEP](https://github.com/ins-amu/bvep)
- [tvb-inversion](https://github.com/the-virtual-brain/tvb-inversion)
- [whobpyt](https://github.com/JohnGriffiths/whobpyt)
have some sta…
-
Hello,
Hello, I am relatively new to Orange(and data mining) and wanted to ask for advice. I am fitting a bunch of spectral data to Fano (see picture). The fits are pretty sharp, partly due to the …
-
Sgr_A_st_ah_03_TP
[uid://A001/X15a0/X16a](https://almascience.org/aq/?result_view=observation&mous=uid://A001/X15a0/X16a)
* [x] Observations completed?
* [x] Delivered?
* [x] Downloaded? (specify wh…