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| Paper: |
Demonstrating the Practical Advantages of the Scalable and Interoperable
Astronomical Framework FASE: Applications to EUCLID Simulations and LUCIFER Data
Reduction |
| Volume: |
461, Astronomical Data Analysis Software and Systems XXI |
| Page: |
753 |
| Authors: |
Paioro, L.; Garilli, B.; Franzetti, P.; Fumana, M.; Scodeggio, M.; Grosbøl, P.; Tody, D.; Surace, C. |
| Abstract: |
The European OPTICON Networks 3.6 and 9.2 in collaboration with the Virtual
Observatory, during the last years have produced a detailed document,
designing the requirements and the architecture of a future scalable and
interoperable desktop framework for the astronomical software (FASE). A first
reference implementation of the FASE framework has been developed at INAF-IASF
Milano and applied to different projects we are involved in: a) the simulation
software developed to study the performance of the EUCLID NISP instrument; b) the
LBT LUCIFER instrument reduction pipeline used by the Italian community. An
application involving graphical capabilities is also being developed exploiting
FASE facilities. We show how the main architectural concepts of the FASE framework
have been successfully applied to the software mentioned above, providing easy
to use and install interoperable software, equipped with distributed and
scalable capabilities. See also Grosbøl et al. (2012). |
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