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Angel Ruiz committed Jun 14, 2024
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165 changes: 165 additions & 0 deletions .gitignore
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32 changes: 32 additions & 0 deletions LICENSE
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The Clear BSD License

Copyright (c) 2024 Angel Ruiz
All rights reserved.

Redistribution and use in source and binary forms, with or without
modification, are permitted (subject to the limitations in the disclaimer
below) provided that the following conditions are met:

* Redistributions of source code must retain the above copyright notice,
this list of conditions and the following disclaimer.

* Redistributions in binary form must reproduce the above copyright
notice, this list of conditions and the following disclaimer in the
documentation and/or other materials provided with the distribution.

* Neither the name of the copyright holder nor the names of its
contributors may be used to endorse or promote products derived from this
software without specific prior written permission.

NO EXPRESS OR IMPLIED LICENSES TO ANY PARTY'S PATENT RIGHTS ARE GRANTED BY
THIS LICENSE. THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND
CONTRIBUTORS "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR
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ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
POSSIBILITY OF SUCH DAMAGE.
31 changes: 31 additions & 0 deletions README.md
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# Energy Conversion Factors for X-ray Astronomy

`ecfxa` is a Python package providing tools for the estimation
of ECFs for different astronomical X-ray missions. Currently
we include XMM-Newton/EPIC, Swift/XRT and eROSITA. ECFs where
calculated consistently for the different missions using the most
updated calibration files at the date of the package release of t
version of the package.

X-ray sources detected through photon counter cameras are characterized
by count-rates at a given energy band. These count-rates (CR) can be
converted into physical fluxes using the calibrated response of the
detector and assuming an specific spectral model via:

FLUX = CR / ECF

where the ECF (Energy Conversion Factor) encapsulate the information
about the response and spectral model for the given energy band.
For an in-depth explanation of ECF and how they are calculated see
[Mateos et al. 2009](https://doi.org/10.1051/0004-6361/200811409)
or the [eROSITA ECF tutorial](https://erosita.mpe.mpg.de/dr1/eSASS4DR1/eSASS4DR1_arfrmf/eROSITA_ECF_tutorial.pdf).

Details about our ECF calculations for the different missions can
be found in the [corresponding Jupyter notebooks](https://github.com/ruizca/ecfxa/calc/) included
in this repository.

Examples
--------

We provide a [Jupyter notebook with examples](https://github.com/ruizca/ecfxa/docs/example.ipynb)
on how to use ecfxa for different X-ray missions.
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