The Cherenkov Telescope Array Observatory Top Level Use Cases

被引：3

作者：

Bulgarelli, A. ^{[1
]}

Kosack, K. ^{[2
]}

Hinton, J. ^{[12
]}

Tosti, G. ^{[4
]}

Schwanke, U. ^{[5
]}

Schwarz, J. ^{[6
]}

Colome, P. ^{[34
,35
]}

Conforti, V. ^{[1
]}

Khelifi, B. ^{[7
]}

Goullon, J. ^{[8
]}

Ong, R. ^{[9
]}

Markoffm, S. ^{[10
]}

Contreras, J. L. ^{[42
]}

Lucarelli, F. ^{[18
]}

Antonelli, L. A. ^{[18
]}

Bigongiari, C. ^{[22
,23
]}

Boisson, C. ^{[27
]}

Bosnjak, Z. ^{[44
]}

Brau-Nogue, S. ^{[19
]}

Carosi, A. ^{[18
]}

Chen, A. ^{[16
]}

Cotter, G. ^{[25
]}

Covino, S. ^{[6
]}

Danie, M. ^{[36
]}

De Cesare, G. ^{[1
]}

de Ona Wilhelmi, E. ^{[26
]}

Della Volpe, M. ^{[33
]}

Di Pierro, F. ^{[22
,23
]}

Fioretti, V. ^{[1
]}

Fuessling, M. ^{[13
]}

Garczarczyk, M. ^{[3
]}

Gaug, M. ^{[17
]}

Glicenstein, J. F. ^{[32
]}

Goldoni, P. ^{[7
]}

Goetz, D. ^{[2
]}

Grandil, P. ^{[1
]}

Heller, M. ^{[33
]}

Hermann, G. ^{[37
]}

Inoue, S. ^{[43
]}

Knodlseder, J. ^{[19
]}

Lenain, J. -P. ^{[28
]}

Lindfors, E. ^{[29
]}

Lombardi, S. ^{[18
]}

Luque-Escamilla, P. ^{[38
]}

Maier, G. ^{[3
]}

Marisaldil, M. ^{[1
]}

Mundell, C. ^{[39
]}

Neyroud, N. ^{[15
]}

Noda, K. ^{[40
]}

O'Brien, P. ^{[41
]}

机构：

[1] INAF IASF Bologna, Bologna, Italy

[2] CEA Saclay, Irfu SAp, Bat 709, F-91191 Gif Sur Yvette, France

[3] DESY, Zeuthen, Germany

[4] Univ Perugia, Dept Phys & Geol, Via A Pascoli, I-06121 Perugia, Italy

[5] Humboldt Univ, Inst Phys, Berlin, Germany

[6] INAF Osservatorio Astron Brera, Milan, Italy

[7] CNRS, IN2P3, APC, Paris, France

[8] CTA Project Off, Heidelberg, Germany

[9] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90024 USA

[10] Univ Amsterdam, API GRAPPA, Amsterdam, Netherlands

[11] CEA Saclay, Irfu SPP, Bat 141, F-91191 Gif Sur Yvette, France

[12] MPI Kernphys, D-69029 Heidelberg, Germany

[13] Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany

[14] INAF IASF Palermo, Palermo, Italy

[15] Univ Savoie, Lab Annecy Le Vieux Phys Particules, Chambery, France

[16] Univ Witwatersrand, Johannesburg, South Africa

[17] Univ Autonoma Barcelona, Dept Fis, Fis Radiac, Bellaterra 08193, Spain

[18] Osserv Astron Roma, INAF, Rome, Italy

[19] CNRS IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France

[20] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[21] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53706 USA

[22] Ist Nazl Fis Nucl, Osservatorio Astrofis Torino, Via P Giuria 1, I-10125 Turin, Italy

[23] Ist Nazl Fis Nucl, Via P Giuria 1, I-10125 Turin, Italy

[24] Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Dept Astron & Meteorol, Marti & Franques 1, E-08028 Barcelona, Spain

[25] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England

[26] Inst Space Sci CSIC IEEC, E-08193 Barcelona, Spain

[27] Univ Paris Diderot, PSL, CNRS, LUTH,Obs Paris, Paris, France

[28] Sorbonne Univ, UPMC Univ Paris 06, Univ Paris Diderot, Sorbonne Paris Cite,CNRS,LPNHE, 4 Pl Jussieu, F-75252 Paris 5, France

[29] Univ Turku, Dept Phys & Astron, SF-20500 Turku, Finland

[30] CNRS, IPAG, F-38000 Grenoble, France

[31] Univ Paris Diderot, CNRS, PSL Res Univ, GEPI,Observ Paris, Pl Jules Janssen, F-92195 Meudon, France

[32] Sorbonne Paris Cite, Pl Jules Janssen, F-92195 Meudon, France

[33] Univ Geneva, DPNC, 24 Quai Ernest Ansermet, CH-1211 Geneva, Switzerland

[34] Inst Ciencies Espai ICE CSIC, Barcelona, Spain

[35] Inst Estudis Espacials Catalunya IEEC, Barcelona, Spain

[36] Univ Liverpool, Dept Phys, Liverpool L69 3BX, Merseyside, England

[37] Max Planck Inst Kernphys, POB 103980, D-69029 Heidelberg, Germany

[38] Univ Jaen, Escuela Politecn Super Jaen, Dept Ingn Mecan & Minera, Campus Las Lagunillas A3-008, Jaen 23071, Spain

[39] Univ Bath, Dept Phys, Bath, Avon, England

[40] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[41] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England

[42] Univ Complutense Madrid, Fac CC Fis, GAE, E-28040 Madrid, Spain

[43] RIKEN, Wako, Saitama, Japan

[44] Univ Rijeka, Dept Phys, Rijeka, Croatia

来源：

SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY IV | 2016年 / 9913卷

关键词：

Big Science; Cherenkov Telescope Array Observatory; Use Cases; Requirements; CRAB-NEBULA;

D O I：

10.1117/12.2232224

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Today the scientific community is facing an increasing complexity of the scientific projects, from both a technological and a management point of view. The reason for this is in the advance of science itself, where new experiments with unprecedented levels of accuracy, precision and coverage (time and spatial) are realised. Astronomy is one of the fields of the physical sciences where a strong interaction between the scientists, the instrument and software developers is necessary to achieve the goals of any Big Science Project. The Cherenkov Telescope Array (CTA) will be the largest ground-based very high-energy gamma-ray observatory of the next decades. To achieve the full potential of the CTA Observatory, the system must be put into place to enable users to operate the telescopes productively. The software will cover all stages of the CTA system, from the preparation of the observing proposals to the final data reduction, and must also fit into the overall system. Scientists, engineers, operators and others will use the system to operate the Observatory, hence they should be involved in the design process from the beginning. We have organised a workgroup and a workflow for the definition of the CTA Top Level Use Cases in the context of the Requirement Management activities of the CTA Observatory. Scientists, instrument and software developers are collaborating and sharing information to provide a common and general understanding of the Observatory from a functional point of view. Scientists that will use the CTA Observatory will provide mainly Science Driven Use Cases, whereas software engineers will subsequently provide more detailed Use Cases, comments and feedbacks. The main purposes are to define observing modes and strategies, and to provide a framework for the flow down of the Use Cases and requirements to check missing requirements and the already developed Use-Case models at CTA sub-system level. Use Cases will also provide the basis for the definition of the Acceptance Test Plan for the validation of the overall CTA system. In this contribution we present the organisation and the workflow of the Top Level Use Cases workgroup.

引用

页数：12

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