-
There has been some discussion in https://github.com/official-stockfish/Stockfish/pull/2260 about the test bounds, how to optimize for resource usage and how to verify scaling and whatnot. So I opened…
-
Recently I got a problem in the Cholesky decomposition when I run `star_BD.py --samples=5`
```
Traceback (most recent call last):
File "/usr/local/AstroPhysics/Python_Anaconda/anaconda2/envs/py…
-
@mostafa-razavi
As applications provide consistent results (see remark 3.1) with earlier work it is likely that the liquid
densities have been either (i) taken from previous work cited in referen…
-
A first principles model of the MagnetoShield shall be developed. [This](http://ctms.engin.umich.edu/CTMS/index.php?example=Introduction§ion=ControlStateSpace) could be used as a starting point, b…
-
From slack:
We are currently considering a proposal where we would simulate a very small piece of the sky (around the size of a tract or a raft) to full 10 year depth for a validation test very soo…
-
CosmoDC2_5000 will be delivered in healpixel files covering 1 octant of the sky, over 3 redshift ranges (0-1, 1-2, 2-3)
Here is the slide from the DC2 telecon (https://docs.google.com/presentation/d/…
-
`using Measurements, Rotations`
I create a quaternion with uncertainty:
```
julia> q1 = Quat(1.0 ± 0.01,0.0 ± 0.01,0.0 ± 0.001,0.0 ± 0.002)
3×3 Quat{Measurement{Float64}}(1.0±0.0, 0.0±0.01, 0.0±…
-
_The problem:_ Many astrophysical spectra are composed of the superposition of two or more individual spectra, for example unresolved multiple systems or starspots.
_Suggested solution:_
The compos…
gully updated
5 years ago
-
Dear experts,
We are working on low pt L2Res measurement by using 2015D low PU data samples. We need to re-derive MCTruth corrections to improve and reduce uncertainties.
Our MC sample[1] is reconst…
-
I would be nice to have the uncertainties (e.g. error of the measurement) or weights used as part of the fitting.
Lmfit (https://lmfit.github.io/lmfit-py/model.html) uses it as weights. So when you…