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GammaLearn

Authors: Jacquemont, Mikael; Vuillaume, Thomas; Trivellato, Thomas;
Abstract

GammaLearn Release v0.7.4 The main changes in this release concern the automatization of the releases: publication to Zenodo, generation of docker containers and pypi packages. Changelog: - cleaner install and auto upload to pypi - Package nets and experiments example settings as package data - Include GammaPhysNet in GammaLearn - allow gammalearn --version - Autoencoders in glearn - Fix calls to .item() - Replace GpuStatsMonitor with DeviceStatsMonitor and accelerator with strategy - Zenodo automated publication of releases - using setuptools_scm to determine version from git tag and distance to tag - Documentation - Docker containers - Harmonise GammaLearn headline - Add metadata as codemeta file - fix classification metrics import

GammaLearn is a collaborative project to apply deep learning to the analysis of low-level Imaging Atmospheric Cherenkov Telescopes such as CTA. It provides a framework to easily train and apply models from a configuration file. Learn more at https://purl.org/gammalearn

Keywords

iact, cta, deep learning, telescope, cherenkov

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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