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Docker files and images for various LISA DPC applications

Supports de l'école ASTROINFO2021 du 29 novembre au 10 décembre 2021.

Les documents, les énoncés et les images utilisés par les participants de l'ANF école informatique 2019

Welcome to the main data repository for the AstroInfo 2023 school

Dépot de cours et de code pour l'ANF "Concepts et utilisation du Machine Learning pour Informaticiens" ayant lieu du 21 au 25 septembre 2020 à Orsay

HiPeRTA is a C++ library implementing the real-time analysis low-level reconstruction algorithms of the Cherenkov Telescope Array (CTA). The real-time analysis is used by the Science Alert Generation (SAG) subsystem of the Array Control And Data Acquisition (ACADA) of CTAO for data quality and science monitoring and science alert generation.

MICRO project public combined fit code

Tutoriels sur la virtualisation et les notebooks

Notebook associated to the technical note LISA-LCST-SGS-TN-001 (applicable document for ESA and reference for the Science Req. Doc.) summarizing computation of the noise power spectral density, LISA’s sensitivity curve and signal-to-noise ratio.

Python Traps and Pitfalls, a half-day course for the PHENIICS doctoral school.

Code for estimating the confusion noise signal from GWs emitted from the compact Galactic Binaries, as measured by LISA.