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I have finished a complete first draft of the code that rescales the stellar masses in protoDC2. I am raising this Issue so that people can understand the techniques I am using to solve the problem of…
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The AGPL license is strong copyleft license, designed so that **anything** copyrightable, and in particular an item used on a network such as Ruth, will always be available for free. For example, Rut…
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Based on discussions with @mducle and @Jon-Taylor during the developer meeting:
My understanding is that `Rebin` is handling uncertainties correctly, whereas `Rebin2D` is wrong. The argument can be…
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Is there a way to upload more geologic attribute values? We have a few groups, formations, and members that are not available through the data entry form. We are going to start bulkloading some of our…
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Hello,
I am calculating luminosity for a log parabola model using the following code. I want to compute the uncertainties in the output values. Since the code performs a numerical integration, is i…
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I have a suggestion for bootstrapping.
I am creating a function to do it, which I am going to call `geterrors` (for a project now, but to be incorporated in htmd in the future, and maybe called getst…
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refs #420: NXcanSAS was ratified at 2016NIAC
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Most "plots" that will be submitted are really just histograms (1D or 2D or 3D). So what you need is a way to specify the bin boundaries and the contents of each bin. I would suggest asking people to …
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When it comes to language about uncertainties, I think it would be helpful if we can settle on a common terminology and definitions. From NIST perspective, this may a necessity. The document will ha…
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few questions/comments:
- why is the thickness for the latest plies 0, e.g. for the 3 plies ?
- can we actually extract the average thickness from the contour plot by averaging automatically avail…