PSI Tier-3 Physics Groups Overview
Note: Each group has a home page on this wiki that can be reached by the link in the
Name column.
Name |
Responsible |
Members |
Guest |
susy |
Leonardo Sala |
Filip Moortgat, Pascal Nef, Luc Pape, Frédéric Ronga, Benjamin Stieger, Konstantinos Theofilatos, Bruno Casal, Marco-Andrea Buchmann, Pablo Martinez |
Saeid Paktinat Mehdiabadi, Santiago Folgueras |
qcd |
? |
Matthias Weber |
|
pixel |
Danek Kotlinski |
Sibille Jennifer, Valeria Radicci, Cameron Bravo, Tilman Rohe |
|
higgs |
? |
Thomas Punz, Mauro Donega, Marco Peruzzi, Daniel Meister |
|
ewk |
? |
Carmelo Marchica, Ann-Karin Sanchez |
Milos Dordevic |
ecal |
? |
|
|
b-physics |
Urs Langenegger |
Christoph Nägeli, Hans-Christian Kästli, Christoph Grab, Jose.Lazo-Flores, Frank Meier, Andreas Schatti, Lukas Wehrli, Alice Bean, Lukas Baeni, Carlotta Favaro |
Bora Akgun, Luca Martini |
Policies for the resource allocation on the PSI Tier-3
These policies were agreed upon in the
first Steering board Meeting
- We organize the users along Physics Groups
- For the purpose of the cluster organization, every user must be mapped exactly to one physics group (even though the user may work for several).
- The resources available to a physics group consist of the added up resources of its members. How these resources are used is up to the physics group's internal organization.
- Each physics group has one Responsible User who
- takes care of managing the group's resources (e.g. deciding what data sets to delete).
- is the single point of contact for the cluster administrators for organizational issues.
- can propose a guest user (see below).
- The resources are equipartitioned between users
- Each group may define one guest user who may be an external user (i.e. not belonging to ETHZ, PSI, or UniZ).
- The guest user will not get own resources, but he can use the group's resources
- The group's Responsible User is responsible for the guest user.
- The Guest user's account will be of limited duration