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Welcome to Binary_SED_Fitting's documentation!
==============================================
Fitting stellar SEDs for single and multi-component systems.
GitHub: `Binary_SED_Fitting `__
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Requirements
~~~~~~~~~~~~~
* ``python`` >= 3.12.2
* ``astropy`` >= 6.0.1
* ``matplotlib`` >= 3.8.4
* ``numpy`` >= 1.26.4
* ``pandas`` >= 2.2.1
* ``scipy`` >= 1.13.0
* ``xarray`` >= 2024.3.0
- Installation: ``python3 -m pip install xarray``
- Install optional dependencies for handling I/O: ``python3 -m pip install "xarray[io]"``
Installation
~~~~~~~~~~~~
- Add the ``binary_sed_fitting.py`` to your working directory.
- ⚠️ Edit the ``DIR_MODELS`` in the ``binary_sed_fitting.py`` file according to where your model files are located
- Download the required models from `Google Drive `__.
More information about how to make these model files is given in `models_and_tools `__.
- Currently supported spectral models:
- ``kurucz_synthetic_photometry.nc`` (Kurucz 2003IAUS..210P.A20C)
- ``koester_synthetic_photometry.nc`` (Koester 2010MmSAI..81..921K)
- ``kurucz_uvblue_synthetic_photometry.nc`` (Hybrid Kurucz_UVBLUE 2005ApJ...626..411R)
- Isochrones: ``master_isochrone.csv`` (`Parsec isochrones `__)
- WD cooling curves: ``master_Bergeron_WD.csv`` (`Bergeron models `__)
Caution
~~~~~~~
⚠️ The software is under active development.
The code has been designed for 3 component SEDs.
However, only double component fitting is thoroughly tested.
Citation
~~~~~~~~
This code is developed by Vikrant V. Jadhav (Universität Bonn).
If you use the code, please refer to Jadhav et al. (2021), *UOCS. IV.
Discovery of diverse hot companions to blue stragglers in the old open
cluster King 2*, Journal of Astrophysics and Astronomy, Volume 42, Issue
2, article id.89 (https://doi.org/10.1007/s12036-021-09746-y)
.. toctree::
:maxdepth: 2
:caption: Contents:
Home
getting_started
modules
changlog
Indices and tables
==================
* :ref:`genindex`
* :ref:`modindex`
* :ref:`search`