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I use `simCluster` to create synthetic clusters with the $Gaia$ magnitudes using the following lines in the `.yaml` file but I only get the $u, g, r, i, z, J, H,$ and $K$ data.
```
main_sequ…
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- [x] KRC find spectral models, send to JRAD
(The R~10,000 model grid at http://phoenix.astro.physik.uni-goettingen.de/?page_id=16 would be my recommended starting point)
## Pre NYC HW
- [ ] KRC fi…
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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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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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#### 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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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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1.) The wavelength of the photometric data points seems to be too narrow. This is clearest when plotting data for wide filters, e.g. WISE W3:
[WISE-Filter.pdf](https://github.com/user-attachments/fil…
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Part of #452
There is a bunch YJHKLM MKO photometry in columns BV:CN.
Question for @kilohoku - When we ingest photometry, we try to include both telescope and instrument, not just filter. Ide…
kelle updated
2 months ago
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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…