Here is a Complete list of my publications.

Selection of these publications to which my contribution was most significant and that illustrate the evolution of my work:
- Perotto, L., Ponthieu, N., Macias-Perez, J. F., et al, (2020). This paper presents the commissioning of NIKA2, all the tests that we performed to characterize the instrument and its performances.

- Ritacco, A., Ponthieu, N., Catalano, A., et al (2017). This paper presents the performances of the polarization module adapated to NIKA1. It validates the implementation of a fast and continuously rotating half wave plate to reject the atmospherical contribution. It is the paper summarizing most of the work done by Alessia Ritacco during her thesis, when I was her co-supervisor.

- Ponthieu, N., Grain, J., Lagache, G., (2011). This paper presents the algorithm that I developed to compute the angular power spectrum of diffuse emission in the presence of complex masks and for arbitrary high resolution maps. It was used twice to characterize the Cosmic Infrared Background anisotropies using the Planck data in Planck collab. (2011) and Planck collab. (2014).

- Shimon, M., Keating, B., Ponthieu, N., Hivon, E., (2008). This paper presents the semi-analytical formalism that I used to constrain the scanning strategies and to simulate the polarization specific systematic effects of the EPIC, SAMPAN, Bpol/COrE satellite projects, as well as the balloon borne EBEX and the ground based BICEP telescopes.

- Ponthieu, N., Macias-Perez, J. F., Tristram, M. et al, (2005). This paper presents the first estimation of the angular power spectrum of the polarized thermal emission of galactic dust and assess its impact as a contaminant to CMB measures.

- Benoit, A., Ade, P., Amblard, A. et al, (2004). This paper presents the results of the analysis I contributed to during my thesis. It was the first evidence of polarized thermal emission by dust on scales larger than the degree.