Citation

If using gwfast please cite the GitHub repository and the release papers arXiv:2207.02771 and arXiv:2207.06910.

Release papers

Here you find the \({\rm BibT}_{\rm \Large E}{\rm X}\) records of the release papers

@article{Iacovelli:2022bbs,
  author = "Iacovelli, Francesco and Mancarella, Michele and Foffa, Stefano and Maggiore, Michele",
  title = "{Forecasting the Detection Capabilities of Third-generation Gravitational-wave Detectors Using GWFAST}",
  eprint = "2207.02771",
  archivePrefix = "arXiv",
  primaryClass = "gr-qc",
  doi = "10.3847/1538-4357/ac9cd4",
  journal = "Astrophys. J.",
  volume = "941",
  number = "2",
  pages = "208",
  year = "2022"
}

@article{Iacovelli:2022mbg,
  author = "Iacovelli, Francesco and Mancarella, Michele and Foffa, Stefano and Maggiore, Michele",
  title = "{GWFAST: A Fisher Information Matrix Python Code for Third-generation Gravitational-wave Detectors}",
  eprint = "2207.06910",
  archivePrefix = "arXiv",
  primaryClass = "astro-ph.IM",
  doi = "10.3847/1538-4365/ac9129",
  journal = "Astrophys. J. Supp.",
  volume = "263",
  number = "1",
  pages = "2",
  year = "2022"
}

Additional references

Here we list some other papers that made use of gwfast

    1. Kole, F. Iacovelli, M. Mancarella, N. Produit, (2022). Adding Gamma-ray Polarimetry to the Multi-Messenger Era. A&A 669, A77 (2023). arXiv:2211.12403.

    1. Branchesi, M. Maggiore et al., (2023). Science with the Einstein Telescope: a comparison of different designs. arXiv:2303.15923.

    1. Mancarella, F. Iacovelli, D. Gerosa, (2023). Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors. arXiv:2303.16323.

    1. Franciolini, F. Iacovelli, M. Mancarella et al., (2023). Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics. arXiv:2304.03160.

Acknowledgments

We are grateful to Marica Branchesi, Jan Harms, Ulyana Dupletsa, Samuele Ronchini and the GSSI group for extremely useful discussions and comparisons of our respective codes (see GWFish) and results, all along this project. We also thank Ssohrab Borhanian and B. S. Sathyaprakash for comparisons with GWBENCH, and Andrea Maselli, Ik Siong Heng, Mauro Pieroni and the members of the ET Observational Science Board (OSB) Div. 9 for hosting discussions about comparisons of Fisher codes.

For a repository of papers relevant for ET, produced in the context of the activities of the ET OSB, see https://www.et-gw.eu/index.php/observational-science-board?view=article&id=161.

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