You can find the up-to-date list of my astrophysics publications from NASA ADS here.
Consistency of DES, HSC and KiDS lensing with BOSS clustering: We present new measurements of the excess surface mass density profiles using the three state-of-the-art lensing surveys and jointly analyse with galaxy clustering to assess the consistency on small and large-scales [Amon and Robertson et al 2022].
Dark Energy Survey Year 3 Cosmology from Cosmic Shear: I led and coordinated the Dark Energy Survey Year 3 cosmic shear lensing analysis using the most powerful data until present, of 100 million galaxies [Amon et al 2021].
Dark Energy Survey Year 3 Cosmology from Weak Lensing and Clustering 3x2pt: I played a pivotal role in the Dark Energy Survey Year 3 combined lensing and clustering cosmology analysis, leading the weak lensing results and coordinating three analysis teams to the most precise cosmological constraints of its kind [DES Collaboration 2021].
Dark Energy Survey Deep Fields: I co-coordinated this team, responsible for the processing and validation of the deep, optical+NIR fields, crucial for the Year 3 analysis. 
Dark Energy Survey Year 3 Redshift Analysis: I used machine learning and data science techniques to develop new statistical methods for accurate weak lensing measurements, especially for estimating and calibrating photometric redshifts for the Dark Energy Survey [15, 14].
Dark Energy Survey Year 3 PSF and shear calibration: I have worked on validating the Dark Energy Survey’s Year 3 galaxy catalogue. Specifically, I tested the shape calibration, point spread function modelling and image simulations and co-coordinate the shear testing team [11,12,13].
Vera Rubin Observatory Dark Energy Science Collaboration Commissioning: I was part of a small team preparing a note recommending target fields for commissioning, on behalf of the DESC .
Kilo-Degree Survey (KiDS) : I was a core member of the KiDS 450 sq. deg. analysis. KiDS is a large optical imaging survey, designed primarily for weak-lensing. Its exquisite quality data is taken from the VLT Survey Telescope at the ESO Paranal Observatory [ 1, 2, 3, 4, 5].