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What sorts of tools and collaborations can we leverage to minimize unnecessary reproduction of effort?
Here are some that were mentioned in PlasmaPy/PlasmaPy#162 :
* [MassiveOES](https://bitbucket…
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reported by: @CloudyLex
http://astroatom.wordpress.com/2011/07/01/new-effective-recombination-coefficients-for-nebular-n-i-lines/
New effective recombination coefficients for nebular N II lines
Po…
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Hi,
I'd like to suggest a small change in the `calc_adev_phase` function:
The line
`s = np.sum(v_arr * v_arr)`
should be replaced by
`s = np.sum(abs(v_arr)**2)`
This will make the adev and…
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I did a test between PM Optical coupling gel and Petroleum Jelly. I could see no difference in count rate. Is Optical coupling gel Petroleum Jelly or something else. We are considering what to inc…
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**Submitting author:** @DavidT3 (David J Turner)
**Repository:** https://github.com/DavidT3/DAXA
**Branch with paper.md** (empty if default branch): paper/writeJOSSPaper
**Version:** v0.2.0
**Editor:*…
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The concerned repo is for using Astropy and affiliated packages to make a publication-quality spectrum with labeled emission lines through a cube. I am proposing to turn the GitHub repo at [https://gi…
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It is probably not an issue to most of the users, but I find the current hyperspy metadata structure to be a bit clumsy. My main issue is with SEM and TEM leafs. These are like singletons. It makes th…
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From Researchgate:
> Hi Matthias,
Congrats on having made staRdom open! That people can PARAFAC on R is a great idea, and I'm also looking forward to trying it.
Although not the main point of you…
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The documentation on the HITRAN website explained that it is possible to calculate the Lorentzian HWHM with partial pressure. I see that the `absorptionCoefficient_Lorentz` and other `absorptionCoeffi…
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@RobeReyes should do a literature search on this object and select some recent papers that he thinks are interesting and relevant.