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I've tried running SPECIES on several different spectra, including the example solar spectrum. After calculating the line widths, the code always throws an error with the following output in the log:
…
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Hi Meredith,
This looks good!
Next step -- Can you calculate the dispersion of the points around the lines please?
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We just started an official conversation how to include **non-interacting physical binary** in the BEAST fitting (see also issue #19). Our motivation for this development is that (1) binary stars exis…
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![phoenix_peterplot_full](https://user-images.githubusercontent.com/65725585/97597665-00c17c80-19fe-11eb-9b38-7bd3fd42af96.png)
![phoenix_peterplot_ha](https://user-images.githubusercontent.com/6…
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Hi Tim,
Over the past few days I've been wondering how hard could it be to tune `VESPA` so that one can readily apply it to TESS photometry.
A few things came up:
— A magnitude for the band in …
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Hello All,
I've noticed that some of the template subclasses are missing, namely O: 1-4 ; B:7 ; A: 4,5,8 ; K: 6,7,5 ; L: 4,5,7,8,9. I did some investigation and noticed that templates only exist for…
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### Bug report
**Bug summary**
Spurious results for RAMSES particle projection plots at CPU boundaries. The dataset for the simulation is quite large, so I didn't find anywhere to upload it (2.4…
cphyc updated
5 years ago
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**Which documentation page is causing an issue?**
Please include the URL of the page
https://cogsworth.readthedocs.io/en/latest/pages/install.html
**What is the problem?**
Please quote the sec…
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An effective and efficient forward model is required for population-level stellar population inference. Let's start with a toy model.
The simplest case is only varying stellar mass and current SFR…
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A significant fraction of what we know about nature and the Universe has been discovered or informed by transients. This question addresses the large amount of work done, and that will be done in the …