Commit 4f422dc6 authored by Yannick Roehlly's avatar Yannick Roehlly

Rework TODO and use emacs org-mode

parent 22713dec
* Tasks
** TODO Check the age of the Universe at observation redshift.
In the psum module, when dealing with an observation, only use the models aged
less than the age of the Universe at observation redshift.
** TODO Deal with observation without values in some filters.
** TODO SED serialisation.
Code SED serialisation to store them in a database without pickling the whole
object.
** TODO Enhance the management of array parameters.
When a parameter is an array (like the filters for which the attenuation is
computed in the attenuation modules) the user must use the "eval ..."
notation. Try to find a better notation. Implement the generation for default
parameters. Maybe use tuples instead of arrays.
** TODO Homogenise the metallicity numbering. .
Use the one for which the "solar" metallicity is 0.02.
** TODO Code the creation of mock catalogues.
** TODO Create some plot to check the fit quality:
- plot giving for each band the ratio between the observed flux and the best
sed flux.
- colour plots (colours chosen by the user) comparing the colour ranges
covered by the simulation and the colours of the observed galaxies.)
** TODO Write documentation.
** TODO Code IGM effect module.
Make the IGM module only add the IGM effect and use the SED redshifting
method.
** TODO Make the IGM module work with a list (or range) of redshift.
This will allow the use of pcigale to compute photometric redshifts.
** TODO Enhance the interpolation method.
Work on interpolation method to try to avoir the "wave effect" when plotting
in logarithmic scale.
** TODO Change attenuations computed by attenuation modules.
Compute both continuum and total attenuation in the filters in the attenuation
modules.
** TODO Deal with lines in the same way as continuum contributions.
Transform the way lines are stored to be more coherent with the way the
continuum is dealt with. Maybe something like line_wavelength (1D array),
line_width (nD array) and line_fluxes (nD array).
* Check the age of the Universe at observation redshift.
* Deal with observation without values in some filters.
* Code the theoretical SED serialisation and the database to store them.
* When a default parameter is an array, use the "eval ..." the the generated
ini file.
* Change metallicity numbering (ex. 0.02 for solar).
* Code the creation of mock catalogues.
* Create some plot to check the fit quality:
- plot giving for each band the ratio between the observed flux and the best
sed flux.
- colour plots (colours chosen by the user) comparing the colour ranges
covered by the simulation and the colours of the observed galaxies.)
* Write documentation.
* Code IGM effect module.
* Make the IGM effect a module separated from the main SED creation modules
and applied according to the redshift of the observation.
* Make the IGM module work with a list (or range) of redshift to allow the
use of pcigale to compute photometric redshifts.
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