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An observation execution system for next-generation large telescopes

Identifieur interne : 000142 ( PascalFrancis/Corpus ); précédent : 000141; suivant : 000143

An observation execution system for next-generation large telescopes

Auteurs : Kim Gillies ; Shane Walker

Source :

RBID : Pascal:11-0004508

Descripteurs français

English descriptors

Abstract

The telescope development projects of the 1990's produced a set of capable 8-10m telescopes that are now in operations across the northern and southern hemispheres. This was the first generation of telescopes to benefit from carefully engineered software systems, yet several years of 8m operations have revealed weaknesses in a common architecture employed by many of them. Today engineers are working on the next generation of telescopes, the extremely large telescopes (ELTs), along with their software systems. It is our view that many of the fundamental assumptions about how software systems for 8-m class large telescopes should be constructed are not optimal for the next generation of extremely large telescopes. In fact, these ideas may constrain the solution space and result in overly complex software and increased development costs. This paper points out issues with current architecture solutions and how they impact the software needed for extremely large telescopes. It then provides the outline of a new approach for the design of the software running at the telescope that is targeted towards the development issues of ELTs and large telescope operations.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

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A06       @3 p. 2
A08 01  1  ENG  @1 An observation execution system for next-generation large telescopes
A09 01  1  ENG  @1 Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States
A11 01  1    @1 GILLIES (Kim)
A11 02  1    @1 WALKER (Shane)
A12 01  1    @1 RADZIWILL (Nicole M.) @9 ed.
A12 02  1    @1 BRIDGER (Alan) @9 ed.
A14 01      @1 Space Telescope Science Institute, 3700 San Martin Drive @2 Baltimore, MD, 21218 @3 USA @Z 1 aut.
A14 02      @1 Gemini Observatory, Southern Operations Center, Casilla 603 @2 La Serena @3 CHL @Z 2 aut.
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A44       @0 0000 @1 © 2011 INIST-CNRS. All rights reserved.
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A60       @1 P @2 C
A61       @0 A
A64 01  1    @0 Proceedings of SPIE, the International Society for Optical Engineering
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C01 01    ENG  @0 The telescope development projects of the 1990's produced a set of capable 8-10m telescopes that are now in operations across the northern and southern hemispheres. This was the first generation of telescopes to benefit from carefully engineered software systems, yet several years of 8m operations have revealed weaknesses in a common architecture employed by many of them. Today engineers are working on the next generation of telescopes, the extremely large telescopes (ELTs), along with their software systems. It is our view that many of the fundamental assumptions about how software systems for 8-m class large telescopes should be constructed are not optimal for the next generation of extremely large telescopes. In fact, these ideas may constrain the solution space and result in overly complex software and increased development costs. This paper points out issues with current architecture solutions and how they impact the software needed for extremely large telescopes. It then provides the outline of a new approach for the design of the software running at the telescope that is targeted towards the development issues of ELTs and large telescope operations.
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Format Inist (serveur)

NO : PASCAL 11-0004508 INIST
ET : An observation execution system for next-generation large telescopes
AU : GILLIES (Kim); WALKER (Shane); RADZIWILL (Nicole M.); BRIDGER (Alan)
AF : Space Telescope Science Institute, 3700 San Martin Drive/Baltimore, MD, 21218/Etats-Unis (1 aut.); Gemini Observatory, Southern Operations Center, Casilla 603/La Serena/Chili (2 aut.)
DT : Publication en série; Congrès; Niveau analytique
SO : Proceedings of SPIE, the International Society for Optical Engineering; ISSN 0277-786X; Coden PSISDG; Etats-Unis; Da. 2010; Vol. 7740; No. p. 2; 77400Q.1-77400Q.12; Bibl. 9 ref.
LA : Anglais
EA : The telescope development projects of the 1990's produced a set of capable 8-10m telescopes that are now in operations across the northern and southern hemispheres. This was the first generation of telescopes to benefit from carefully engineered software systems, yet several years of 8m operations have revealed weaknesses in a common architecture employed by many of them. Today engineers are working on the next generation of telescopes, the extremely large telescopes (ELTs), along with their software systems. It is our view that many of the fundamental assumptions about how software systems for 8-m class large telescopes should be constructed are not optimal for the next generation of extremely large telescopes. In fact, these ideas may constrain the solution space and result in overly complex software and increased development costs. This paper points out issues with current architecture solutions and how they impact the software needed for extremely large telescopes. It then provides the outline of a new approach for the design of the software running at the telescope that is targeted towards the development issues of ELTs and large telescope operations.
CC : 001D02B09
FD : Développement produit; Développement logiciel; Télescope; Hémisphère; Coût développement
ED : Product development; Software development; Telescope; Hemisphere; Development cost
SD : Desarrollo producto; Desarrollo logicial; Telescopio; Hemisferio
LO : INIST-21760.354000174702880230
ID : 11-0004508

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Pascal:11-0004508

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