.. FastResponseAnalysis documentation master file, created by sphinx-quickstart on Mon Dec 4 10:43:46 2023. You can adapt this file completely to your liking, but it should at least contain the root `toctree` directive. IceCube Fast Response Analysis (FRA) ===================================== :: ******************************************************************************** _____ _ ____ | ___|_ _ ___| |_ | _ \ ___ ___ _ __ ___ _ __ ___ ___ | |_ / _` / __| __| | |_) / _ \/ __| '_ \ / _ \| '_ \/ __|/ _ \ | _| (_| \__ \ |_ | _ < __/\__ \ |_) | (_) | | | \__ \ __/ |_| \__,_|___/\__| |_| \_\___||___/ .__/ \___/|_| |_|___/\___| |_| _ _ _ / \ _ __ __ _| |_ _ ___(_)___ / _ \ | '_ \ / _` | | | | / __| / __| / ___ \| | | | (_| | | |_| \__ \ \__ \ /_/ \_\_| |_|\__,_|_|\__, |___/_|___/ |___/ ******************************************************************************** The **Fast Response Analysis** is a tool for rapid response to astrophysical transients with the IceCube Neutrino Observatory. It uses a transient maximum likelihood method to rapidly respond to astrophysical events in real time. The current implementation houses the code for responding to: * Generic externally triggered transients (eg. bright GRBs, AGN flares, novae, etc) * IceCube alert events * Gravitational Wave events This documentation describes the Fast Response Package. For a description of the physics, see `R. Abbasi et al 2021 ApJ 910 4 `_ (for external transients), `R. Abbasi et al 2023 ApJ 951 45 `_ (for alert events), and `R. Abbasi et al 2023 ApJ 944 80 `_ (for gravitational wave events). (Top graphic made with `PyFiglet `_) Contents ============ .. toctree:: :maxdepth: 2 getting_started fra alert ext gw reports web_utils plotting Index ================== * :ref:`genindex` * :ref:`modindex` * :ref:`search`