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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.chfor 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.orgfor 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 stackoasis.opensciencegrid.org- OSG community softwaregrid.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.