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🔍 Content is being verified for accuracy (Last updated: 27 October 2025)

This documentation page is currently being written and reviewed.

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Common examples of repositories#

Here is a detailed list of commonly used CVMFS repositories and their primary purposes:

CVMFS repository reference#

CERN repositories:#

Repository Main Project Description
alice.cern.ch ALICE Experiment Software and data for the ALICE heavy-ion physics experiment.
ams.cern.ch AMS Experiment Software for the Alpha Magnetic Spectrometer space station detector.
atlas.cern.ch ATLAS Experiment Primary software repository for the ATLAS collaboration.
atlas-condb.cern.ch ATLAS Conditions Conditions database for ATLAS detector calibration.
atlas-nightlies.cern.ch ATLAS Development Nightly builds of ATLAS software.
cernvm-prod.cern.ch CernVM Project CernVM-FS server and client software.
cms.cern.ch CMS Experiment Main repository for CMS software (CMSSW).
grid.cern.ch WLCG Worldwide LHC Computing Grid middleware.
lhcb.cern.ch LHCb Experiment Primary software for the LHCb experiment.
lhcb-condb.cern.ch LHCb Conditions LHCb conditions database.
sft.cern.ch CERN SFT LCG Software Stacks.
sft-nightlies.cern.ch CERN SFT Development Nightly builds of SFT software.
unpacked.cern.ch CERN Unpacked container images. See the CVMFS documentation for details.

Open Science Grid (OSG) repositories#

Repository Main Project Description
config-osg.opensciencegrid.org OSG Config OSG CVMFS configuration repository. See the Open Science Grid website for details.
dunedaq.opensciencegrid.org DUNE DAQ Data Acquisition framework for the Deep Underground Neutrino Experiment (DUNE).
dune.opensciencegrid.org DUNE Experiment Deep Underground Neutrino Experiment.
fermilab.opensciencegrid.org Fermilab General-purpose Fermilab software.
gm2.opensciencegrid.org Muon g-2 Muon g-2 experiment.
icecube.opensciencegrid.org IceCube IceCube Neutrino Observatory.
larsoft.opensciencegrid.org LArSoft Liquid Argon TPC software toolkit. See the LArSoft website for details.
lz.opensciencegrid.org LZ Experiment LUX-ZEPLIN (LZ) dark matter detector.
minerva.opensciencegrid.org MINERvA MINERvA neutrino-nucleus scattering experiment.
mu2e.opensciencegrid.org Mu2e Mu2e muon-to-electron conversion experiment.
nova.opensciencegrid.org NOvA Experiment NuMI Off-Axis electron neutrino appearance experiment.
oasis.opensciencegrid.org OSG OASIS OSG Application Software Service.
spt.opensciencegrid.org South Pole Telescope Cosmic microwave background studies.
uboone.opensciencegrid.org MicroBooNE MicroBooNE liquid argon neutrino experiment.

Other collaborations#

Repository Main Project Description
software.eessi.io European Environment for Scientific Software Installations EESSI provides a common stack of optimized scientific software installations that work on any Linux distribution, and currently supports both x86_64 (AMD/Intel) and aarch64 (Arm 64-bit) systems
sw.lsst.eu Vera Rubin Observatory Large Synoptic Survey Telescope software

Example application#

When configuring your CVMFS session, select the repositories that are relevant to your research field. For example:

For High-Energy Physics:#

  • LHC Experiments: Use your collaboration's repository (atlas.cern.ch, cms.cern.ch, alice.cern.ch, lhcb.cern.ch)
  • General software: Include sft.cern.ch for compilers and libraries
  • Configuration: Always include cvmfs-config.cern.ch

For Neutrino Physics:#

  • Long-baseline: dune.opensciencegrid.org, nova.opensciencegrid.org
  • Short-baseline: uboone.opensciencegrid.org, minerva.opensciencegrid.org
  • Toolkits: larsoft.opensciencegrid.org for LArTPC experiments

For Astrophysics/Cosmology:#

  • icecube.opensciencegrid.org (neutrino astronomy)
  • spt.opensciencegrid.org (cosmic microwave background)
  • sw.lsst.eu (optical astronomy)
  • lz.opensciencegrid.org (dark matter searches)

General Scientific Computing:#

  • sft.cern.ch - Comprehensive scientific software stack
  • oasis.opensciencegrid.org - OSG community software
  • grid.cern.ch - Grid computing tools

You can always add more repositories later by creating a new persistent image, but starting with the correct set will save you time and storage space.