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If simultaneously fitting the stellar and extinction, it would be good to do this with a composite model.
For example, assume a blackbody for the stellar and one of the dust_extinction models. Need …
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Part of #452
@kilohoku - I see some JHK measurements in the "2MASS" columns which don't appear to be 2MASS sources. Are the majority of these from a particular instrument/telescope that is not 2M…
kelle updated
3 months ago
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Hello,
Would it be possible to add the DECam u-band and VR-filters to gaiaxpy. They are available at https://noirlab.edu/science/programs/ctio/filters/Dark-Energy-Camera
Thank you!
-Katie FAsbend…
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#### TLDR
After creating an isochrone object, changing the filters, while keep all else constant, does not cause SPISEA to not recalculate that isochrone.
#### Suspected cause
This appears to be…
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I'm encountering an issue with PHOEBE broadcasting the following variable during import when I run it within MPI, but I want to not use MPI and parallelization within PHOEBE. This is lines 164–168 in …
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Thanks a lot for providing this helpful tool for working with the XP spectra!
I noticed that the uncertainties that are returned by `calibrate` depend on the number of basis components that I use f…
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I'd like to raise a rather broad issue for discussion about making specutils compatible with spectroscopic data sets from fields such as laboratory plasma physics and heliophysics.
I'm coming fro…
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I've just started having a play with the tomo_challenge data, and I'm curious about some of the quirks of the dataset. To this end, I've included here a bunch of observations & questions. I understand…
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Three somewhat linked problems:
- [x] When setting `'ism_red'` to less than 1.0 in a model parameter dictionary for a `model_box`, the wavelength of the model gets very restricted (up to ca. 0.8 µm…
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I believe the planck function bb_func in planck.py appears to be missing a factor of wavelength. At line 99, x = factor \* x \* x \* x and then there is one more wavelength factor divided out at the e…