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From space to specs : Requirements for 4MOST

Schnurr, Olivier (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
Walcher, C. Jakob (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
Chiappini, Cristina (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
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Schwope, Axel D. (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
Bellido-Tirado, Olga (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
Haynes, Roger (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
Feltzing, Sofia (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
McMahon, Richard (author)
University of Cambridge
de Jong, Roelof S. (author)
Leibniz Institute for Astrophysics Potsdam (AIP)
Ansorge, Wolfgang (author)
RAMS-CON Management Consultants
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 (creator_code:org_t)
SPIE, 2014
2014
English 9 s.
In: Modeling, Systems Engineering, and Project Management for Astronomy VI. - : SPIE. - 1996-756X .- 0277-786X. - 9780819496188 ; 9150
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • 4MOST,1 the 4m Multi-Object spectrographic Survey Telescope, is an upcoming optical, fiber-fed, MOS facility for the VISTA telescope at ESO's Cero Paranal Observatory (Chile). The preliminary design of 4MOST features 2,400 fibers split into a low-resolution (1,600 fibers, 390-900 nm, R > 5; 000) and a high-resolution channel (800 fibers, three arms, ∼20-25 nm coverage each, R > 18; 000) with an Echidna-style positioner, and covering a hexagonal field of view of ∼4.1 sqdeg. 4MOST's main science goals encompass massive (tens of millions of spectra), all-Southern sky (> 18; 000 sqdeg) surveys following up both the Gaia (optical) and eROSITA (X-ray) space missions, plus cosmological science that complements missions such as e.g. Euclid. In a novel approach, observations of these science cases, which are very different from another, are to be carried out in parallel (i.e., simultaneously); thus, from the very different science requirements, key user requirements have to be identified, stringently formulated, and condensed into a coherent set of system specifications. Clearly, identifying common grounds and thereby significantly reducing complexity in both the formulated requirements and the final 4MOST facility, is a very challenging task. In this paper, we will present science and user requirements, and how the latter flow down from the former, and eventually further down to the system-specification level. Special emphasis will be put on the identification of key requirements and their validation and verification protocols, so that significant trade-offs can be done as early on in the design phase as possible, with as little impact as possible on the science capabilities upstream.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

4MOST
ESO
Requirements engineering
Requirements management
VISTA

Publication and Content Type

kon (subject category)
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