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Sgr_A_st_k_03_TP
[uid://A001/X15a0/Xe0](https://almascience.org/aq/?result_view=observation&mous=uid://A001/X15a0/Xe0)
* [x] Observations completed?
* [x] Delivered?
* [x] Downloaded? (specify where…
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Sgr_A_st_ab_03_TP
[uid://A001/X15a0/X146](https://almascience.org/aq/?result_view=observation&mous=uid://A001/X15a0/X146)
* [x] Observations completed?
* [x] Delivered?
* [x] Downloaded? (specify wh…
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I am adding a new module to support inferences of an emission component from circumstellar disks. My assumptions for the purpose of this implementation are:
1. The emission component is spectrally…
gully updated
6 years ago
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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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Sgr_A_st_i_03_TP
[uid://A001/X15a0/Xd4](https://almascience.org/aq/?result_view=observation&mous=uid://A001/X15a0/Xd4)
* [x] Observations completed?
* [x] Delivered?
* [x] Downloaded? (specify where…
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Using fitting.fit_continuum to fit a simple linear continuum to two continuum windows gives significantly different slopes for two different realizations of the noise. The chi^2 (by-eye) value someti…
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Sgr_A_st_a_03_TP
[uid://A001/X1590/X30ae](https://almascience.org/aq/?result_view=observation&mous=uid://A001/X1590/X30ae)
* [x] Observations completed?
* [x] Delivered?
* [x] Downloaded? (spec…
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Just some thoughts about a new spectrum class. Probably too fancy and too object orientated.
Note the inst files already have the `Spectrum` method for spectral data
https://github.com/mzechmeiste…
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Cool tutorials from @pmocz. Not sure how they fit into this project, but thought I'd bookmark them here.
> Hi everyone! 👋 I wanted to share some introductory ~100 line Python code tutorials with th…
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Sgr_A_st_t_03_TP
[uid://A001/X15a0/X116](https://almascience.org/aq/?result_view=observation&mous=uid://A001/X15a0/X116)
* [x] Observations completed?
* [x] Delivered?
* [x] Downloaded? (specify whe…