128 research outputs found
An Innovative Science Gateway for the Cherenkov Telescope Array
The Cherenkov Telescope Array (CTA) is an initiative to build the next generation, ground-based gamma-ray observatories. We present a prototype workspace developed at INAF that aims at providing innovative solutions for the CTA community. The workspace leverages open source technologies providing web access to a set of tools widely used by the CTA community. Two different user interaction models, connected to an authentication and authorization infrastructure, have been implemented in this workspace. The first one is a workflow management system accessed via a science gateway (based on the Liferay platform) and the second one is an interactive virtual desktop environment. The integrated workflow system allows to run applications used in astronomy and physics researches into distributed computing infrastructures (ranging from clusters to grids and clouds). The interactive desktop environment allows to use many software packages without any installation on local desktops exploiting their native graphical user interfaces. The science gateway and the interactive desktop environment are connected to the authentication and authorization infrastructure composed by a Shibboleth identity provider and a Grouper authorization solution. The Grouper released attributes are consumed by the science gateway to authorize the access to specific web resources and the role management mechanism in Liferay provides the attribute-role mapping
An Innovative Workspace for The Cherenkov Telescope Array
The Cherenkov Telescope Array (CTA) is an initiative to build the next
generation, ground-based gamma-ray observatories. We present a prototype
workspace developed at INAF that aims at providing innovative solutions for the
CTA community. The workspace leverages open source technologies providing web
access to a set of tools widely used by the CTA community. Two different user
interaction models, connected to an authentication and authorization
infrastructure, have been implemented in this workspace. The first one is a
workflow management system accessed via a science gateway (based on the Liferay
platform) and the second one is an interactive virtual desktop environment. The
integrated workflow system allows to run applications used in astronomy and
physics researches into distributed computing infrastructures (ranging from
clusters to grids and clouds). The interactive desktop environment allows to
use many software packages without any installation on local desktops
exploiting their native graphical user interfaces. The science gateway and the
interactive desktop environment are connected to the authentication and
authorization infrastructure composed by a Shibboleth identity provider and a
Grouper authorization solution. The Grouper released attributes are consumed by
the science gateway to authorize the access to specific web resources and the
role management mechanism in Liferay provides the attribute-role mapping
Software design for the control system for Small-Size Telescopes with single-mirror of the Cherenkov Telescope Array
The Small-Size Telescope with single-mirror (SST-1M) is a 4 m Davies-Cotton
telescope and is among the proposed telescope designs for the Cherenkov
Telescope Array (CTA). It is conceived to provide the high-energy ( few TeV)
coverage. The SST-1M contains proven technology for the telescope structure and
innovative electronics and photosensors for the camera. Its design is meant to
be simple, low-budget and easy-to-build industrially.
Each device subsystem of an SST-1M telescope is made visible to CTA through a
dedicated industrial standard server. The software is being developed in
collaboration with the CTA Medium-Size Telescopes to ensure compatibility and
uniformity of the array control. Early operations of the SST-1M prototype will
be performed with a subset of the CTA central array control system based on the
Alma Common Software (ACS). The triggered event data are time stamped,
formatted and finally transmitted to the CTA data acquisition.
The software system developed to control the devices of an SST-1M telescope
is described, as well as the interface between the telescope abstraction to the
CTA central control and the data acquisition system.Comment: In Proceedings of the 34th International Cosmic Ray Conference
(ICRC2015), The Hague, The Netherlands. All CTA contributions at
arXiv:1508.0589
ASTRI Mini-Array Software Product Breakdown Structure
This document contains the ASTRI Mini-Array Software PBS. This document applies to all application- and domain-level software for the MA software project
ASTRI Mini-Array Glossary
The ASTRI Mini-Array (MA) is an INAF ground-based project to construct, deploy and operate a set of nine identical dual-mirror Cherenkov gamma-ray telescopes, and several other auxiliary equipment and infrastructures. The ASTRI Mini-Array scientific objective is to exploit the imaging atmospheric Cherenkov technique to measure the energy, direction and arrival time of gamma-ray photons arriving at the Earth from astrophysical sources.
This document lists acronyms and the glossary of the projec
INDIGO MidnightBlue Service Catalogue
INDIGO-DataCloud is co-founded by the Horizon 2020Framework Programme.Peer reviewe
Cloud access to interoperable IVOA-compliant VOSpace storage
Handling, processing and archiving the huge amount of data produced by the new generation of experiments and instruments in Astronomy and Astrophysics are among the more exciting challenges to address in designing the future data management infrastructures and computing services. We investigated the feasibility of a data management and computation infrastructure, available world-wide, with the aim of merging the FAIR data management
provided by IVOA standards with the efficiency and reliability of a cloud approach. Our work involved the Canadian Advanced Network for Astronomy
Research (CANFAR) infrastructure and the European EGI federated cloud
(EFC). We designed and deployed a pilot data management and computation
infrastructure that provides IVOA-compliant VOSpace storage resources and
wide access to interoperable federated clouds. In this paper, we detail the
main user requirements covered, the technical choices and the implemented
solutions and we describe the resulting Hybrid cloud Worldwide infrastructure, its benefits and limitation
The Pierre Auger Cosmic Ray Observatory
The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2 , 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.Facultad de Ciencias Exacta
The Pierre Auger Cosmic Ray Observatory
The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2 , 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.Facultad de Ciencias Exacta
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