afterglowpy
Advanced tools
| 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' |
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| 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 |
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@@ -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 |
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@@ -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"} | ||
| ) |
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