- Indico style
- Indico style - inline minutes
- Indico style - numbered
- Indico style - numbered + minutes
- Indico Weeks View
Introduzione generale
Nei prossimi meeting vi chiederei se a rotazione di fare una presentazione sulle attività in svolgimento per aggiornare tutti e anche per avere un quadro dell'avanzamento e delle necessità.
OGGI: presentazione su Flagship "pipeline" PSGE da parte di Valentina e Roberto.
Scadenze
Riunione dello spoke board 19/02
| Durata temporale | Mese di progetto | Scadenze per invio report scientifico ad HUB |
Milestone 6 | Mag 23 – Ago 23 | M9-M12 | DONE! |
Milestone 7 | Set 23 – Feb 24 | M13-M18 | 20 Marzo 2024 |
Milestone 8 | Mar 24 – Giu 24 | M19-M22 | 15 Luglio 2024 |
Milestone 9 | Lug 24 – Ott 24 | M23-M26 | 20 Novembre 2024 |
Milestone 10 | Nov 24 – Ago 25 | M27-M36 | 20 Marzo 2025 (report intermedio) Report finale a Settembre2025 (deadline tbc) |
Scuole e conferenze
Incoming:
Past schools or conferences (to recover material)
AoB
TEMI dei BANDI a CASCATA spoke2
Aree Tematiche Finanziate (per beneficiari privati):
1- Data Management PoCs/pilots with Spoke 2 solutions in industrial environments (datalake, distributed computing, …).
2- Solutions, implementation and deployment of a computing PoC based on the ARM architecture.
3- Porting and optimization (on GPU, on FPGA, on CPU) of algorithms of interest of AstroParticle experiments.
4- Realization of tools and pilots for the Space Economy domain, using the infrastructure of the ICSC (portals, market exchange, algorithms, services, …).
5- Heterogeneous industrial use cases on the Spoke 2 platforms (GPU + FPGA + ARM).
6- Profiling, code engineering and code quality on Spoke 2 code repositories.
Aree Tematiche Finanziate (per beneficiari pubblici):
1- Development of data acquisition and trigger strategies in the context high background, rare event experiment, using acceleration on hybrid CPU/FPGA architectures, in the context of the activities of the Spoke2 in ICSC.
2- Development of a multipurpose/multi experiment high level cloud infrastructure for small/medium astroparticle experiments, on the infrastructure of ICSC and for the benefit of Spoke 2 use cases.
3- Development of a GPU library for massively parallelized simulations of QCD and QCD+QED on the lattice in the context of the activities of the Spoke2 in ICSC.
4- Development and performance optimization of typical simulation codes in HEP and Astro, for the use cases of Spoke 2.
5- Advanced algorithms for GW experiments (Virgo and ET) in the context of the activities of the Spoke2 in ICSC.
6- Studying the quantum Boltzmann equation neutrino flavour conversion in a dense environment in the context of the activities of the Spoke2 in ICSC.
7- Development of algorithms for boosted topologies at LHC/FCC, in the context of the activities of the Spoke2 in ICSC.
8- Accelerated analysis of Astrophysical data in the Photon Counting Big Data era, in the context of the activities of the Spoke2 in ICSC .
STATO INNOVATION GRANTS
ALTRE INFORMAZIONI UTILI
Missione svolta nell’ambito delle attività del progetto Centro Nazional HPC, Big Data e Quantum Computing CN_00000013, Spoke 2 “Fundamental research and space economy” CUP C53C22000350006"
Updated report da Francesco Visconti:
https://docs.google.com/document/d/1oeTfViJJEk_bIlTsztzICpC2jt2JKcFYTIRiIzvBhmM/edit
(riportato in fondo)
Report Alessia Spolon
riporto qui il mio report:
- Report: stiamo facendo dei tests sul banco ottico in laboratorio ad Asiago per raccogliere dei dati su cui verificare le procedure ed i codici di riduzione-analisi. I test sono quasi finiti e a Marzo iniziamo ad adattare le procedure per l'analisi. Questa attività ha la priorità, perché abbiamo bisogno di dati 'veri', non simulati e questa e’ la finestra programmata per ottenerli.
- Bandi a cascata: Luca contattera’ Antonio e Marco nei prossimi giorni per pa
ok! avevo problemi con indico prima .. sto cercando di risolvere!
- Centro Nazionale HPC: Spoke 10 - Quantum Computing
The testing is focused particularly on ensuring that we can accurately interpolate the grid parameters when generating the light curve. For this, we are currently coordinating with experts of nmma (Pang and Ragosta) and the author of the kilonova models (Bulla).
Once deployed correctly, we will begin to test the kilonova model interface to our existing GW+afterglow Python fitting routine.
Documento aggiornamento attività INAF OAR - Responsabile: F. Visconti
Participants: Michele Mastropietro, Ciro Bigongiari, Saverio Lombardi, Francesco Gabriele Saturni, Antonio Stamerra