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The LHC experiments represent more than three quarters of the total resources funded at CNAF. They heavily use the Grid technology, on top of which they have built experiment-specific services to better support data management, job management and monitoring. Besides LHC, the following experiments belonging to the High Energy Physics, Astrophysics and astro-particle domains are also supported at CNAF: AGATA, AMS-02, ARGO-YBJ, ASFIN, Auger, BELLEII, Borexino, COSMO_WNEXT, CDF, COMPASS, COSINUS, CSES-LimadouALICE, ATLAS, CMS, LHCB, Belle2, CDF, Compass, KLOE, LCHf, LHCB TIER2, NA62, PADME, AMS2, ARGO, AUGER, Borexino, CTA, CUORE, CupidDAMPE, DAMPEDARKSIDE, DarkSide-50ENUBET, EuclidEUCLID, FAMUFERMI/GLAST, FAZIAGerda, Fermi-LATHerd, FOOTIcarus, GerdaJUNO, ICARUSKM3, JunoLHAASO, KLOELIMADOU, KM3NeTLSPE, KM3NeT/NEMO, LHAASO, LHC-f, MAGIC, NA62, NEWCHIM, NEWSdm, nTOF, OPERA, PADME, PAMELA, TRISTAN, Virgo, XENON. Support to the BaBar and SuperB experiment was dismissed during 2014LUCIFER/CUPID, MAGIC, NEWS, Opera, PAMELA, Tristan, Virgo, Xenon100, Agata/GAMMA, ASFIN, FAMU, FOOT, JLAB12, NEWCHIM/FARCOS, nTOF, Nuclex/Fazia.
Groups belonging to the Computational Chemistry and Biomedical domains access the center in an opportunistic way through Grid services. Moreover, local theoretical physics and astronomy groups access the Tier-1 resources and services. Most of these non-LHC user communities use Grid technologies at some level, but in a few cases the activities are performed only locally or using ad-hoc tools. For a more complete description, please refer to the User Support page[4].
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