If you make use of herculens, please cite Galan et al. 2022. This work presents the global architecture of the tool, and applies it to reconstruct a pixelated lens potential with wavelets.
@ARTICLE{Galan2022_herculens,
author = {{Galan}, A. and {Vernardos}, G. and {Peel}, A. and {Courbin}, F. and {Starck}, J. -L.},
title = "{Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses}",
journal = {\aap},
keywords = {galaxies: structure, dark matter, methods: data analysis, gravitation, gravitational lensing: strong, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
year = 2022,
month = dec,
volume = {668},
eid = {A155},
pages = {A155},
doi = {10.1051/0004-6361/202244464},
archivePrefix = {arXiv},
eprint = {2207.05763},
primaryClass = {astro-ph.IM},
adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...668A.155G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
In addition, if you combine herculens with nifty, please cite Galan et al. 2024.
@ARTICLE{Galan2024_herculens_nifty,
author = {{Galan}, A. and {Caminha}, G.~B. and {Knollm{\"u}ller}, J. and {Roth}, J. and {Suyu}, S.~H.},
title = "{El Gordo needs El Anzuelo: Probing the structure of cluster members with multi-band extended arcs in JWST data}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2024,
month = feb,
eid = {arXiv:2402.18636},
pages = {arXiv:2402.18636},
doi = {10.48550/arXiv.2402.18636},
archivePrefix = {arXiv},
eprint = {2402.18636},
primaryClass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv240218636G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}