-
Since the spectral weight of each oscillator is an intrinsic property which is calculated from the parameters, it should be an always available attribute of any oscillator instance. Moreover, if the p…
-
I've spend sometime thinking about PR #83. It is really the AKARI+Spitzer scipack. This PR is fine as it is and should be merged once discussion is resolved.
For the future, would it be better to…
-
I am currently working on a project involving the fitting of a CO data cube using the LTE_Molecule model in PySpecKit (version 1.0.1 on a 64-bit Windows system).Despite varying the initial guess param…
-
@keflavich When trying to fit some old VLA data I get the error message below. Here I'm trying to fit the NH3(1,1) line, and in the header it is stored as velocity. Is there something obvious I should…
-
It would be useful to have code that would use the saved sparse lnp files to generate a model spectrum+range or model spectra for the BEAST fits. This would allow comparisons from the BEAST fits to e…
-
I'm currently trying to use my own logging and wrap around some of the JWST pipeline. This works OK, but the logs seem to produce multiple outputs once I've used anything that wraps around stpipe. I i…
-
Currently montblanc uses a spectral index model for the frequency axis
I(v) = I(v0)(v/v0)^alpha
In some cases it is preferable to fit a more flexible model. In particular it is not possible to fit i…
-
I tried to compare the results between CPU UMAP and GPU UMAP with fashion mnist dataset, it seems the CPU implementation is more accuracy from a visualization point. The comparison is made between br…
-
-
Some tools for characterizing the noise in the RM cubes (those produced by RM-synthesis and/or RM-clean) would be useful for a number of purposes, e.g. source-finding, combating Ricean bias.