- 03 Apr, 2013 5 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Rename m2005_sfh to m2005 as it does not deal with the star formation history.
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Yannick Roehlly authored
The Marasont 2005 module is modified to use the output of a star formation history module. The SFH is now a complete SFR vs time tuple (taken from the SED information dictionary) and the age of the galaxy is defined by this SFH (the maximum time). The Maraston 2005 data class is also changed to make the convolution in such SFH.
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 21 Mar, 2013 1 commit
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Yannick Roehlly authored
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- 02 Mar, 2013 1 commit
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Yannick Roehlly authored
Instead of writing all the computation table at once, write one table per observation as a FITS file.
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- 27 Feb, 2013 3 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 18 Feb, 2013 6 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Use pyfits and save table to fits files as python-vo is not available on pypi.
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Yannick Roehlly authored
Correct dependendy installation.
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Yannick Roehlly authored
Correct dependency installation.
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 11 Feb, 2013 4 commits
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Yannick Roehlly authored
Now there is a statistical module and a script to configure and run the analysis.
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Yannick Roehlly authored
We use the probability density function to compute the expected value and the standard deviation for the parameters.
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Yannick Roehlly authored
Switch to the complete formula to compute the probability associated with the chi-square. This is only useful if the raw probability has a meaning.
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Yannick Roehlly authored
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- 07 Feb, 2013 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 06 Feb, 2013 18 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
Only useful for debug.
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
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Yannick Roehlly authored
Make the statistical analysis module behave the same way as the SED creation module so that one can easily develop and use another one.
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Yannick Roehlly authored
Create all the outputs in a "out/" directory and don't run the analysis if it yet exists.
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Yannick Roehlly authored
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Yannick Roehlly authored
Add the best SED plot and the value vs chi2 plot for each model for each analysed variable.
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Yannick Roehlly authored
s/[Pp]arametre/[Pp]arameter/g s/[Dd]ictionnary/[Dd]ictionary/g
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Yannick Roehlly authored
A list is added to the SED object to store the key names from the info dictionary whose values are proportional to the galaxy mass. This is used by the statistical module to multiplicate the value by the galaxy mass (correction factor) in the analysis.
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Yannick Roehlly authored
Dictionary associating to each "output" parameter its description.
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Yannick Roehlly authored
Suppress the 'unit' part of the tuple associated to each parametre in the parametre_list dictionary of the SED modules. It's not useful. It's better to indicate the unit in the description text.
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Yannick Roehlly authored
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Yannick Roehlly authored
- Make the list of the analysed variables configurable. - Compute the weighted average and standard deviation for these variables. - Write the variable analysis results to a file.
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Yannick Roehlly authored
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