- 22 May, 2013 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 13 May, 2013 2 commits
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Yannick Roehlly authored
Rename it to dustatt_calzleit in preparation of a power law module.
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Yannick Roehlly authored
* Multiplicate the Calzetti-Leitherer continuum by a power law. * Add a UV bump. * The luminosity under 91.2 nm to 0. * Extrapolate the continuum over 2200 nm until attenuation reach 0.
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- 10 May, 2013 1 commit
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Yannick Roehlly authored
Oops, this should have been corrected a long time ago.
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- 29 Apr, 2013 2 commits
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Yannick Roehlly authored
By default, an exception is raised when adding an existing key to the info dictionary. Make it possible to bypass this, for instance to add age if we want to combine various SFH.
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Yannick Roehlly authored
If we redshift a SED using a module, we must not redshift the wavelength to compute the λ, Fν array tuple. Thus we make it optional and not default.
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- 23 Apr, 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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- 20 Apr, 2013 2 commits
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Yannick Roehlly authored
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Yannick Roehlly authored
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- 08 Apr, 2013 1 commit
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Yannick Roehlly authored
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- 03 Apr, 2013 15 commits
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Yannick Roehlly authored
Convert the warehouse a its own module and use submodules for each "back-end". Also, make the back-end configurable with a parameter of the psum analysis module.
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Yannick Roehlly authored
It's better (for now) to use only get_from_cache and get None when the object is not cached.
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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
As there is a specific module to redshift the spectrum, do not automatically apply the redshift when computing a flux.
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Yannick Roehlly authored
The redshifting module must be separated from the main modules producing the restframe SED, because the redshift parameter is taken directly from the observation list. Nevertheless, it is still a SED creation module because one may want to use it for testing various redshifts.
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Yannick Roehlly authored
Simplify some module names: dh2002_ir > dh2002 sfh_2exp > sfh2exp
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Yannick Roehlly authored
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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 1 commit
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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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