Poster + Paper
18 June 2024 Towards image synthesis with photon counting stellar intensity interferometry
Alessia Spolon, Michele Fiori, Luca Zampieri, Marco Landoni
Author Affiliations +
Conference Poster
Abstract
Stellar intensity interferometry (SII) is based on the correlation of the light intensity fluctuations of a star detected at two or more telescopes, with no need to combine the collected photons directly. A measurement of the correlation in full ”photon-counting mode” was experimented with fast photon counters in Italy (2016-2020) and is currently being adapted to the ASTRI Mini-Array. Performing image synthesis with ”photon-counting” SII requires a series of preparatory activities that involve the optimization of the pipelines for the treatment of time series acquired at extremely high photon rates, the development of efficient and innovative algorithms for the cross-correlation of the arrival times in large time series and the development of a preliminary version of a dedicated pipeline for the synthesis of images starting from interferometric data. Here we present the project and the present status of the activities.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Alessia Spolon, Michele Fiori, Luca Zampieri, and Marco Landoni "Towards image synthesis with photon counting stellar intensity interferometry", Proc. SPIE 12996, Unconventional Optical Imaging IV, 129960Y (18 June 2024); https://doi.org/10.1117/12.3029384
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Telescopes

Stellar interferometry

Simulations

Algorithm development

Photon counting

Atmospheric Cherenkov telescopes

RELATED CONTENT


Back to Top