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afterglowpy

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afterglowpy - pypi Package Compare versions

Comparing version
0.6.2
to
0.6.3
+8
-4
afterglowpy.egg-info/PKG-INFO
Metadata-Version: 2.1
Name: afterglowpy
Version: 0.6.2
Version: 0.6.3
Summary: GRB Afterglow Models

@@ -9,9 +9,13 @@ Home-page: https://github.com/geoffryan/afterglowpy

License: MIT
Description: # Semi-analytic GRB Afterglow models
Project-URL: Source Code, https://github.com/geoffryan/afterglowpy
Project-URL: Documentation, https://afterglowpy.readthedocs.io
Description: # Numeric GRB Afterglow models
A Python module to calculate GRB afterglow light curves and spectra. Details of the methods can be found in Ryan et al 2019. Builds on [van Eerten & MacFadyen 2010](https://arxiv.org/abs/1006.5125) and [van Eerten 2018](https://arxiv.org/abs/1801.01848). This code is under active development.
A Python 3 module to calculate GRB afterglow light curves and spectra. Details of the methods can be found in [Ryan et al 2019](https://arxiv.org/abs/1909.11691). Builds on [van Eerten & MacFadyen 2010](https://arxiv.org/abs/1006.5125) and [van Eerten 2018](https://arxiv.org/abs/1801.01848). This code is under active development.
Documentation available at <https://afterglowpy.readthedocs.io/>
## Attribution
If you use this code in a publication, please refer to the package by name and cite "Ryan, G., van Eerten, H., Troja, E., and Piro, L. (in prep)". A publication describing the code is forthcoming in the very near future.
If you use this code in a publication, please refer to the package by name and cite "Ryan, G., van Eerten, H., Piro, L. and Troja, E., 2019, arXiv:1910.11691" [arXiv link](https://arxiv.org/abs/1909.11691).

@@ -18,0 +22,0 @@ ## Features

@@ -11,4 +11,6 @@ #!/usr/bin/env python

__all__ = ["__version__", shock, cocoon, jet, fluxDensity, intensity,
Hz2eV, Msun, c, cgs2mJy, day2sec, eV2Hz, ee, h, hbar, mJy2cgs,
me, mp, parsec, sec2day, sigmaT]
__all__ = ['__version__',
'shock', 'cocoon', 'jet', 'fluxDensity', 'intensity',
'Hz2eV', 'Msun', 'c', 'cgs2mJy', 'day2sec', 'eV2Hz', 'ee', 'h',
'hbar', 'mJy2cgs',
'me', 'mp', 'parsec', 'sec2day', 'sigmaT']

@@ -5,2 +5,2 @@ #!/usr/bin/env python

__short_version__ = '0.6'
__version__ = '0.6.2'
__version__ = '0.6.3'
Metadata-Version: 2.1
Name: afterglowpy
Version: 0.6.2
Version: 0.6.3
Summary: GRB Afterglow Models

@@ -9,9 +9,13 @@ Home-page: https://github.com/geoffryan/afterglowpy

License: MIT
Description: # Semi-analytic GRB Afterglow models
Project-URL: Source Code, https://github.com/geoffryan/afterglowpy
Project-URL: Documentation, https://afterglowpy.readthedocs.io
Description: # Numeric GRB Afterglow models
A Python module to calculate GRB afterglow light curves and spectra. Details of the methods can be found in Ryan et al 2019. Builds on [van Eerten & MacFadyen 2010](https://arxiv.org/abs/1006.5125) and [van Eerten 2018](https://arxiv.org/abs/1801.01848). This code is under active development.
A Python 3 module to calculate GRB afterglow light curves and spectra. Details of the methods can be found in [Ryan et al 2019](https://arxiv.org/abs/1909.11691). Builds on [van Eerten & MacFadyen 2010](https://arxiv.org/abs/1006.5125) and [van Eerten 2018](https://arxiv.org/abs/1801.01848). This code is under active development.
Documentation available at <https://afterglowpy.readthedocs.io/>
## Attribution
If you use this code in a publication, please refer to the package by name and cite "Ryan, G., van Eerten, H., Troja, E., and Piro, L. (in prep)". A publication describing the code is forthcoming in the very near future.
If you use this code in a publication, please refer to the package by name and cite "Ryan, G., van Eerten, H., Piro, L. and Troja, E., 2019, arXiv:1910.11691" [arXiv link](https://arxiv.org/abs/1909.11691).

@@ -18,0 +22,0 @@ ## Features

@@ -1,8 +0,10 @@

# Semi-analytic GRB Afterglow models
# Numeric GRB Afterglow models
A Python module to calculate GRB afterglow light curves and spectra. Details of the methods can be found in Ryan et al 2019. Builds on [van Eerten & MacFadyen 2010](https://arxiv.org/abs/1006.5125) and [van Eerten 2018](https://arxiv.org/abs/1801.01848). This code is under active development.
A Python 3 module to calculate GRB afterglow light curves and spectra. Details of the methods can be found in [Ryan et al 2019](https://arxiv.org/abs/1909.11691). Builds on [van Eerten & MacFadyen 2010](https://arxiv.org/abs/1006.5125) and [van Eerten 2018](https://arxiv.org/abs/1801.01848). This code is under active development.
Documentation available at <https://afterglowpy.readthedocs.io/>
## Attribution
If you use this code in a publication, please refer to the package by name and cite "Ryan, G., van Eerten, H., Troja, E., and Piro, L. (in prep)". A publication describing the code is forthcoming in the very near future.
If you use this code in a publication, please refer to the package by name and cite "Ryan, G., van Eerten, H., Piro, L. and Troja, E., 2019, arXiv:1910.11691" [arXiv link](https://arxiv.org/abs/1909.11691).

@@ -9,0 +11,0 @@ ## Features

@@ -55,3 +55,6 @@ from setuptools import setup, Extension

'docs': ['numpydoc']
}
},
project_urls={
"Source Code": "https://github.com/geoffryan/afterglowpy",
"Documentation": "https://afterglowpy.readthedocs.io"}
)