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 WalkerSource :
-
Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.
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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A05 | | | | @2 7740 |
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A06 | | | | @3 p. 2 |
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A08 | 01 | 1 | ENG | @1 An observation execution system for next-generation large telescopes |
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A09 | 01 | 1 | ENG | @1 Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States |
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A11 | 01 | 1 | | @1 GILLIES (Kim) |
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A11 | 02 | 1 | | @1 WALKER (Shane) |
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A12 | 01 | 1 | | @1 RADZIWILL (Nicole M.) @9 ed. |
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A12 | 02 | 1 | | @1 BRIDGER (Alan) @9 ed. |
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A14 | 01 | | | @1 Space Telescope Science Institute, 3700 San Martin Drive @2 Baltimore, MD, 21218 @3 USA @Z 1 aut. |
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A14 | 02 | | | @1 Gemini Observatory, Southern Operations Center, Casilla 603 @2 La Serena @3 CHL @Z 2 aut. |
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A21 | | | | @1 2010 |
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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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C03 | 03 | X | FRE | @0 Télescope @5 18 |
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C03 | 03 | X | ENG | @0 Telescope @5 18 |
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C03 | 03 | X | SPA | @0 Telescopio @5 18 |
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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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