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As of CMD v3.4 the post-AGB and WD phases are *in preparation*. Tracks that use `COLIBRI` instead of `No`, add a star with label `9` beyond `log(age)~7.9`. This single star looks like this:
![Deepi…
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In this commit https://github.com/asteca/ASteCA/commit/7d2fda6fbf11a2849e5b1567331ec08630a46f84 we fixed issue #346.
I asked here https://stackoverflow.com/q/58596873/1391441 about how to do that a…
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tag: astrometry
Given many (at least three) star with known equatorial coordinates, they can be used to transform the whole set of stars in the frame to RA & DEC.
The function should take the fo…
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After #484, use the masses to derive the IMF and PMF of the cluster.
Keep in mind when moving stars over the isochrone to obtain their masses:
- Present results using: all stars in cluster region …
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Once the code is able to handle N-dimensional diagrams from mixed photometric systems, a separate image file should be generated showing CMDs and CCDs for every possible combinations of magnitudes and…
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Instead of dumping all output files for a cluster inside the `output` folder, generate a unique folder with the format `CLUSTER_1712231344` where `1712231344` is the date (`17/12/23`) and the time (`1…
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[ArviZ: Exploratory analysis of Bayesian models](https://arviz-devs.github.io/arviz/)
> ArviZ is a Python package for exploratory analysis of Bayesian models. Includes functions for posterior analy…
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Move all random number generation to a separate function, and provide the ability to seed this function via [numpy.random.seed](http://docs.scipy.org/doc/numpy/reference/generated/numpy.random.seed.ht…
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ASteCA currently uses emcee v3.0rc2 packaged along with the code. When the final v3 version is released, remove this from the code and install emcee with conda.
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See `bh87coord` with `semi` mode and:
bh87coord 1082. 1290. 750. 10 1 1 0 0
The reported fraction of cluster area is `1.01` where it can never be larger t…