The Process of Data Formation for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter
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- Relative Yield of Thermal and Nonthermal Emission during Weak Flares Observed by STIX during 2021 September 20–25The Astrophysical Journal, Vol. 964, No. 2 | 27 March 2024
- The STIX Imaging ConceptSolar Physics, Vol. 298, No. 10 | 4 October 2023
- Mapped Variably Scaled Kernels: Applications to Solar ImagingComputational Science and Its Applications – ICCSA 2023 Workshops | 29 June 2023
- Approximation of discontinuous inverse operators with neural networksInverse Problems, Vol. 38, No. 10 | 26 August 2022
- RHESSI and STIXHard X-Ray Imaging of Solar Flares | 16 October 2021
- Imaging from STIX visibility amplitudesAstronomy & Astrophysics, Vol. 656 | 14 December 2021
- Feature augmentation for the inversion of the Fourier transform with limited dataInverse Problems, Vol. 37, No. 10 | 27 August 2021
- Visibility Interpolation in Solar Hard X-Ray Imaging: Application to RHESSI and STIXThe Astrophysical Journal, Vol. 919, No. 2 | 4 October 2021
- The non-Fourier image reconstruction method for the STIX instrumentOpen Astronomy, Vol. 29, No. 1 | 31 December 2020
- Count-based imaging model for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar OrbiterAstronomy & Astrophysics, Vol. 624 | 25 April 2019
- Solar hard X-ray imaging by means of compressed sensing and finite isotropic wavelet transformAstronomy & Astrophysics, Vol. 615 | 13 July 2018
- Compressed sensing and finite isotropic wavelets for the STIX reconstruction problem2017 International Conference on Sampling Theory and Applications (SampTA) | 1 Jul 2017
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