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@@ -3,19 +3,7 @@ User-friendly package implementing GW waveform models in pure python, thus enabl
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Developed by [Francesco Iacovelli](<https://github.com/FrancescoIacovelli>).
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This package is released together with the paper [](<>). When making use of it, please cite the paper and the present git repository. Bibtex:
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```
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@article{Iacovelli,
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author = "Iacovelli, Francesco and Mancarella, Michele and Foffa, Stefano and Maggiore, Michele",
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title = "{}",
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eprint = "",
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archivePrefix = "arXiv",
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primaryClass = "astro-ph.CO",
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month = "6",
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year = "2022",
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}
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```
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This package is released together with the papers [arXiv:2207.02771](<https://arxiv.org/abs/2207.02771>) and [arXiv:2207.06910](<https://arxiv.org/abs/2207.06910>), where detail of implementations and results can be found.
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## Code Organization
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The organisation of the repository is the following:
If using this software, please cite this repository and the papers [arXiv:2207.02771](<https://arxiv.org/abs/2207.02771>) and [arXiv:2207.06910](<https://arxiv.org/abs/2207.06910>). Bibtex:
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```
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@article{Iacovelli:2022bbs,
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author = "Iacovelli, Francesco and Mancarella, Michele and Foffa, Stefano and Maggiore, Michele",
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title = "{Forecasting the detection capabilities of third-generation gravitational-wave detectors using GWFAST}",
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eprint = "2207.02771",
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archivePrefix = "arXiv",
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primaryClass = "gr-qc",
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month = "7",
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year = "2022"
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}
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```
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```
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@article{Iacovelli:2022mbg,
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author = "Iacovelli, Francesco and Mancarella, Michele and Foffa, Stefano and Maggiore, Michele",
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title = "{Supplement to "Forecasting the detection capabilities of third-generation gravitational-wave detectors using GWFAST": how to GWFAST}",
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eprint = "2207.06910",
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archivePrefix = "arXiv",
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primaryClass = "astro-ph.IM",
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month = "7",
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year = "2022"
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}
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```
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## Bibliography
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1. A. Buonanno et al. (2009) [arXiv:0907.0700](<https://arxiv.org/abs/0907.0700>)
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2. P. Ajith (2011) [arXiv:1107.1267](<https://arxiv.org/abs/1107.1267>)
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