Saluti e presentazione Workshop

• Riccardo Smareglia

software@INAF

• Bianca Garilli

Sviluppi dell'infrastruttura informatica e dei servizi INAF

• Nanni Mauro

IDEM/Edu-Roam e Servizi di autenticazione

• Franco Tinarelli

Presentazione CRIS-INAF

• Ervin Konomi

Una esperienza di virtualizzazione dei servizi

• Michele Gatti

: La virtualizzazione dei PC dell' amministrazione e dei Servizi. Problematiche e Goal di un percorso legato all'alleggerimento dell' IT managemet amministrativo che permette una maggiore e veloce interazione con l'utente.

Realizzare infrastrutture da zero: opportunita' e problemi

• Porceddu Ignazio (OA Cagliari)

Sicurezza in rete 1/2

• Simona Venuti (GARR) (GARR-Cert)

Formazione

Sicurezza in rete (2/2)

• Simona Venuti (GARR) (GARR-Cert)

Formazione

Reti IPv6 (1/2)

• Franco Tinarelli

Reti IPv6 (2/2)

• Franco Tinarelli

Saluti Direttore OA Cagliari

• Andrea Possenti

Indagine sul calcolo INAF

• Giuliano Taffoni

Presente e futuro della rete Garr

• Massimo Carboni (GARR) (GARR)

Presentazione CRS4

• Lidia Leoni (CRSA)

Presentazione CINECA

• Giovanni Erbacci (CINECA)

HPC projects in Astrophysics at INAF/OAPa: current challenges and future perspectives

• Salvatore Orlando

Tavola Rotonda: La gestione degli incidenti di sicurezza

• Mauro Nanni

Simulating the cradle of stars with graphics processing units

• Michela Mapelli

Simulating young star clusters is a challenge for computational astrophysics. Three main aspects must be accounted for: (i) the hydro-dynamics of the parent molecular cloud, (ii) the dynamics of the newly formed stars, and (iii) the evolution of stars and binary systems. The hydro-dynamical treatment of the gas is particularly demanding because it requires both very high resolution and a suitable cooling function. Given the high density that can be reached in the core of dense young star clusters, the stellar component requires direct-summation N-body integrators, coupled with up-to-date recipes for stellar evolution and stellar winds. Our new group at the Observatory of Padova is involved in the most innovative simulations of molecular clouds and young star clusters. We make use of special purpose hardware, especially graphics processing units (GPUs), to meet the challenge of coupling collisional stellar dynamics and stellar evolution. In this talk, I will present our new tool for stellar evolution in direct-summation N-body codes, which is based on the new Padova stellar evolution tracks. I will also discuss some of our most recent results about star cluster formation and evolution, in the frame of our FIRB 2012 project, and of our most recent CINECA projects.

Attività di HPC presso INAF - OATo: simulazioni MHD di plasmi astrofisici

• Claudio Zanni

Simulations of cosmic structures: a challenge for coding and HPC architectures

• Giuseppe Murante

I will describe the kind of cosmological simulations performed by our hpc group in Trieste, ranging from galaxies to galaxy clusters to cosmological volumes. I will briefly discuss our main simulation code, and its future planned developement. In this context, I will also discuss our needs, and our wishes, in terms of hardware and hardware architectures.

DELL

• paolo Bianco

HPC and BigData solutions in research: the IBM vision

• Marco Briscolini

Oracle & "La Macchina delle Stelle"

• Ezio caudera (Oracle Italia)

How Oracle can help in providing a structured, consolidated system for the INAF knowledge sharing

La Commissione Calcolo e Reti nell'INFN. Cos'è, come funziona e che ruoli ha.

• Dario Menasce

Grid and Cloud Computing at INFN

• Davide Salomoni

Archivi astronomici In Italia - IA2 e varie

• Riccardo Smareglia

DHTCS @ INAF

• Giuliano Taffoni

Euclid

• Fabio Pasian

GAIA: "prototipo metodologico" per le missioni spaziali del futuro

• Mario Lattanzi

3D visual analytics systems for ViaLactea project

• Fabio Vitello

The control software of the Sardinia Radio Telescope

• Andrea Orlati

During this presentation we address the past, present and future of Nuraghe, the control software designed for the Sardinia Radio Telescope. We provide an overview on the requirements, the problems which were faced and the design solutions adopted along the years. The current status, with the SRT astronomical validation in execution, and our development plan are also described.

ACID - Astro & Physics Cloud Interactive Desktop

• Piero Massimino

The Astronomical & Physics Cloud Interactive Desktop (ACID) has been developed for the prototype of CTA Science Gateway in Catania, Italy. ACID is based on a web environment that, avoiding any installation on a local PC, allows the use of plenty of software packages for both on-line and off-line analysis of astrophysical data. The users are able to exploit, if applicable, the native Graphical User Interface (GUI) of the tools available in the ACID environment. The ACID environment exploited by the Science Gateway offers two modes of usage: interactively to perform an on-line analysis through the VNC desktop and the native GUIs or shell environment of the programs; Distributed Computing Infrastructure (DCI) to perform an off-line analysis through a workflow submission. For the interactive usage of the remote software, ACID exploits an ad hoc VNC-based User Interface (VUI). Each type of analysis can be exploited through the CTA Science Gateway based on Liferay and WS-PGRADE/gUSE. Data file sharing is ensured by ownCloud technology. All of these functionalities can be also used through iOS and Android devices.

Infrastrutture Hardware e Software del centro dati VST

• Aniello Grado

Il VLT Survey Telescope e' un telescopio con uno specchio primario da 2.6 m, caratterizzato da un campo di vista di 1 grado quadrato ed una risoluzione di 0.21 arcsec/pixel che e' operativo dal settebre 2011 sul Cerro Paranal. Per supportare la comunita' scientifica dell'INAF che fa uso dei dati VST e' stato realizzato presso l'Osservatorio Astronomico di Capodimonte il centro dati VSTceN. Attualmente esso fornisce immagini completamente calibrate e pronte per essere sfruttare scientitificamente a 10 survey che sfruttano il tempo garantito INAF, OmegaCam ed il tempo garantito cileno. Verranno mostrate le infrastrutture HW, la pipeline, denominata VST-Tube, sviluppata per processare le immagini del VST insieme ai primi risultati scientifici.

Pipeline fotometriche per la gestione dei dati di imaging da LBT per la partnership italiana

• Vincenzo Testa

Sistemi integrati per la gestione di dati spettroscopici: LBT, VIPERS, VANDELS

• Paolo Franzetti

GAIA: Dal Tera al Peta il "social network" nella Galassia

• Roberto Morbidelli

An Innovative Proposal for the CTA Science Gateway

• Pietro Massimino

This CTA science gateway prototype presents a graphical user interface based on a workflow-oriented framework (gUSE/WS-PGRADE). It is equipped with a flexible SSO (SAML based) Authentication and Authorization access control. An interactive desktop environment: the Astronomical & Physics Cloud Interactive Desktop (ACID) is available through the science gateway.The user will be able to exploit the native graphical interface of the tools provided by the ACID environment. A cloud data service shares and synchronizes data files and output results between the user desktop and the science gateway.

The Serra La Nave ICT equipment of the ASTRI SST-2M telescope prototype for the Cherenkov Telescope Array

• Fulvio Giannotti

: ASTRI is an Italian flagship project whose first goal is the realization of an end-to-end telescope prototype, named ASTRI SST-2M, for the Cherenkov Telescope Array (CTA). The prototype will be installed in Italy during Fall 2014. A second goal will be the realization of the ASTRI/CTA mini-array which will be composed of seven SST-2M telescopes placed at the CTA Southern Site. The Information and Communication Technology (ICT) equipment necessary to drive the infrastructure for the ASTRI SST-2M prototype is being designed as a complete and stand-alone computer centre. The design goal is to obtain a basic ICT equipment that might be scaled, with a low level of redundancy, for the ASTRI/CTA mini-array, taking into account the necessary control, monitor and alarm system requirements. The ICT equipment envisaged at the Serra La Nave (SLN) observing station in Italy, where the ASTRI SST-2M telescope prototype will operate, includes computers servers and workstations, network devices, an uninterruptable power supply system, and air conditioning systems. This talk presents the proposed general schema of the SLN Computer Centre and Control Room, describing in particular the Local Area Network (LAN) schema, the computing and storage system, and the system for the telescope control. In particular will be shown HW and SW solutions already implemented, giving particular emphasis to the control system and remote monitoring.

Sistema di controllo e supervisione con il framework Alma Common Software (ACS)

• Sergio Poppi

Data post-processing with CASA package

• Francesco Bedosti

An overview of the deployment of Common Astronomy Software Applications package at the italian ALMA Regional Center.

Correlazione VLBI con software DiFX

• Matteo Stagni

A oltre un anno dall'installazione del software di correlazione DiFX verranno illustrate problematiche, casi ed elementi di gestione e trattamento dei dati radioastronomici e geodinamici degli esperimenti effettuati coinvolgendo le antenne italiane di Medicina, Noto, Matera e SRT.

Digital Backend in Radio-Astronomy

• Andrea Melis

Nuove Potenzialita' Osservative Dei Radiotelescopi IRA

• Simona Righini

Negli ultimi anni i radiotelescopi dell'Istituto di Radioastronomia hanno visto un major upgrade del sistema osservativo, che ne ha migliorato le prestazioni di circa tre ordini di grandezza in termini di sensibilità osservativa single-dish. Per sfruttare appieno queste nuove potenzialità i radiotelescopi si stanno dotando di moderni strumenti software dedicati alle varie fasi osservative, (preparazione delle osservazioni, ispezione, elaborazione e analisi dei dati). E' inoltre in costruzione un moderno archivio dati consultabile via web. In questo talk presentiamo i recenti sviluppi software, le collaborazioni nazionali e internazionali nel cui ambito essi sono stati realizzati, nonché le attività future.