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Angel Ruiz
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# Byte-compiled / optimized / DLL files | ||
__pycache__/ | ||
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# PyInstaller | ||
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The Clear BSD License | ||
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Copyright (c) 2024 Angel Ruiz | ||
All rights reserved. | ||
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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: | ||
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* Redistributions of source code must retain the above copyright notice, | ||
this list of conditions and the following disclaimer. | ||
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* 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. | ||
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* 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. | ||
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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 | ||
LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A | ||
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POSSIBILITY OF SUCH DAMAGE. |
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# Energy Conversion Factors for X-ray Astronomy | ||
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`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. | ||
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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: | ||
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FLUX = CR / ECF | ||
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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). | ||
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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. | ||
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Examples | ||
-------- | ||
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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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