Publication List
- Euclid Collaboration, Bose et al. (2024), Modelling spectroscopic clustering on mildly nonlinear scales in beyond-LCDM models. In preparation.
- DES Collaboration, Karina Rojas et al. (2023), The impact of human expert visual inspection on the discovery of strong gravitational lenses, Mon.Not.Roy.Astron.Soc. 523 (2023) 3, 4413-4430, arXiv 2301.03670 [astro-ph.GA].
- de la Bella, L. F. and Amara, A. and Birrer, S. and Hartley, W.G. and Sudek, P. (2021), Quenching and Galaxy Demographics, arXiv 2112.11110. Submitted to MNRAS.
- Sudek, P. and de la Bella, L. F. and Amara, A. and Hartley, W.G. (2021), The Sensitivity of the Redshift Distribution to Galaxy Demographics, MNRAS doi 10.1093, arXiv 2112.11345.
- Adam Amara, Lucia F. de la Bella, Simon Birrer, Sarah Bridle, Juan Pablo Cordero, Ginevra Favole, Ian Harrison, Ian W.Harry, William G. Hartley, Coleman Krawczyk, Andrew Lundgren, Brian Nord, Laura K. Nuttall, Richard P. Rollins, Philipp Sudek, Sut-Ieng Tam, Nicolas Tessore, Arthur E. Tolley, Keiichi Umetsu, Andrew R. Williamson, Laura Wolz (2021). SkyPy: A package for modelling the Universe. JOSS doi 10.21105/joss.03056, arXiv 2109.06172.
- Lucia F. de la Bella, Nicolas Tessore and Sarah Bridle, (2020). The unequal-time matter power spectrum: impact on weak lensing observables, JCAP doi 10.1088/1475-7516/2021/08/001 , arXiv 2011.06185.
- Lucia Fonseca de la Bella, David Parkinson, Donough Regan y David Seery, (2018). Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure, JCAP doi 10.1088/1475-7516/2020/07/011, arXiv 1805.12394.
- Lucia Fonseca de la Bella, Donough Regan, David Seery and Shaun Hotchkiss, (2017). The matter power spectrum in redshift space using effective field theory, JCAP doi 10.1088/1475-7516, arXiv 1704.05309.
- Jeronimo Cortez, Lucia Fonseca, Daniel Martin-de Blas, Guillermo A. Mena Marugán, (2012). Uniqueness of the Fock quantization of scalar fields under mode preserving canonical transformations varying in time. PRD doi 10.1103/PhyRevD.87.044013, arXiv 1212.3947.