Welcome to SEDobs’s documentation!¶
What is SEDobs?¶
SEDobs is a program that aims at using state of the art theoretical gelaxy SED (spectral energy distribution) to create simulated observation of distant galaxies. It used BC03 and M05 theoretical models and allows the user to configure the simulated observation that are needed. For a given simulated galaxy, the user is able to simulate multi-spectral and multi-photometric observations. Number of inputs are needed and described in Configuration. The outputs are very easy and directly usable, they are described in Outputs. To get started with the use of SEDobs you must install it Installation. And carefully look at the Getting started and Configuration pages to understand how to use it.
Contribute! SEDobs is not perfect! It has been primarily developed for my private research and I decided to release in the spirit of making the research process as transparent as possible and in the hope it can be used by other people. If you have any comment or anything you would like to be added to SEDobs, or, even better, if you want to modify you can either do it yourself or please feel free to contact us! —> @ email@example.com
SEDobs is a free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, version 3 of the License.
SEDobs is distributed without any warranty; without even the implied warranty of merchantability or fitness for a particular purpose. See the GNU General Public License for more details.
You should have received a copy of the GNU General Public License along with the program. If not, see http://www.gnu.org/licenses/ .