Design of modular C++ observatory control system: from observatories to laboratories and back
Identifieur interne :
000189 ( PascalFrancis/Curation );
précédent :
000188;
suivant :
000190
Design of modular C++ observatory control system: from observatories to laboratories and back
Auteurs : Petr Kubanek [
République tchèque,
Espagne] ;
Michael Prouza [
République tchèque] ;
Ronan Cunniffe [
Espagne] ;
Markus Wildi [
Suisse] ;
Jan Strobl [
République tchèque] ;
Ivan Kotov [
États-Unis] ;
Paul O'Connor [
États-Unis] ;
Martin Jelinek [
Espagne] ;
Antonio De Ugarte Postigo [
Italie]
Source :
-
Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.
RBID : Pascal:11-0070228
Descripteurs français
English descriptors
Abstract
For almost a decade we have been developing an open source control system tor autonomous observatories called Remote Telescope System, 2nd version - RTS2. The system is currently used to operate about dozen observatories. It was designed from the beginning as the ultimate tool for autonomously performing any possible observing plan on any hardware. Its modular design allows exactly this and enables even more. Currently it is used to control not only observatories but also CCD testing laboratories. We present the internal design of this open source observatory and laboratory control package, and discuss its overall structure. We emphasise new developments and our experiences building a community of users and developers of the package. Design of the system modularity is explained in detail, and various approaches to software reuse are discussed, with a demonstration of how the best solution emerged. We describe problems that were encountered as mirror sizes and associated operational complexity grew. We also describe how the system is being used at a CCD testing laboratory, and detail the quick transition from previously unsupported hardware to fully automated operation. We discuss how the system's evolution has affected code design, and present unexpected benefits it is brought. Our experience with use of open source code and libraries are discussed.
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| A11 | 08 | 1 | | @1 JELINEK (Martin) |
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| A11 | 09 | 1 | | @1 DE UGARTE POSTIGO (Antonio) |
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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 Institute of Physics, Academy of Sciences @2 Praha @3 CZE @Z 1 aut. @Z 2 aut. |
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| A14 | 02 | | | @1 Image Processign Laboratory, Universitat de València @2 Valencia @3 ESP @Z 1 aut. |
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| C01 | 01 | | ENG | @0 For almost a decade we have been developing an open source control system tor autonomous observatories called Remote Telescope System, 2nd version - RTS2. The system is currently used to operate about dozen observatories. It was designed from the beginning as the ultimate tool for autonomously performing any possible observing plan on any hardware. Its modular design allows exactly this and enables even more. Currently it is used to control not only observatories but also CCD testing laboratories. We present the internal design of this open source observatory and laboratory control package, and discuss its overall structure. We emphasise new developments and our experiences building a community of users and developers of the package. Design of the system modularity is explained in detail, and various approaches to software reuse are discussed, with a demonstration of how the best solution emerged. We describe problems that were encountered as mirror sizes and associated operational complexity grew. We also describe how the system is being used at a CCD testing laboratory, and detail the quick transition from previously unsupported hardware to fully automated operation. We discuss how the system's evolution has affected code design, and present unexpected benefits it is brought. Our experience with use of open source code and libraries are discussed. |
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| C03 | 02 | X | FRE | @0 Logiciel libre @5 07 |
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| C03 | 07 | 3 | ENG | @0 Mirrors @5 21 |
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| A30 | 01 | 1 | ENG | @1 Software and cyberinfrastructure for astronomy @3 San Diego CA USA @4 2010 |
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Le document en format XML
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<author><name sortKey="Kubanek, Petr" sort="Kubanek, Petr" uniqKey="Kubanek P" first="Petr" last="Kubanek">Petr Kubanek</name>
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<s3>CZE</s3>
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<sZ>4 aut.</sZ>
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</affiliation><author><name sortKey="Strobl, Jan" sort="Strobl, Jan" uniqKey="Strobl J" first="Jan" last="Strobl">Jan Strobl</name>
<affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Astronomical Institute, Academy of Sciences</s1>
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<affiliation wicri:level="1"><inist:fA14 i1="06"><s1>Brookhaven National Laboratory</s1>
<s2>Upton, NY</s2>
<s3>USA</s3>
<sZ>6 aut.</sZ>
<sZ>7 aut.</sZ>
</inist:fA14><country>États-Unis</country>
</affiliation><author><name sortKey="Jelinek, Martin" sort="Jelinek, Martin" uniqKey="Jelinek M" first="Martin" last="Jelinek">Martin Jelinek</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Instituto de Astrofísica de Andalúcia CSIC</s1>
<s2>Granada</s2>
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<sZ>3 aut.</sZ>
<sZ>8 aut.</sZ>
</inist:fA14><country>Espagne</country>
</affiliation><author><name sortKey="De Ugarte Postigo, Antonio" sort="De Ugarte Postigo, Antonio" uniqKey="De Ugarte Postigo A" first="Antonio" last="De Ugarte Postigo">Antonio De Ugarte Postigo</name>
<affiliation wicri:level="1"><inist:fA14 i1="07"><s1>INAF-Osservatorio Astronomico di Brera</s1>
<s2>Merate</s2>
<s3>ITA</s3>
<sZ>9 aut.</sZ>
</inist:fA14><country>Italie</country>
</affiliation><series><title level="j" type="main">Proceedings of SPIE, the International Society for Optical Engineering</title>
<title level="j" type="abbreviated">Proc. SPIE Int. Soc. Opt. Eng.</title>
<idno type="ISSN">0277-786X</idno>
<imprint><date when="2010">2010</date>
</imprint><seriesStmt><title level="j" type="main">Proceedings of SPIE, the International Society for Optical Engineering</title>
<title level="j" type="abbreviated">Proc. SPIE Int. Soc. Opt. Eng.</title>
<idno type="ISSN">0277-786X</idno>
</seriesStmt><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Metering</term>
<term>Mirrors</term>
<term>Modular design</term>
<term>Modular system</term>
<term>Open source software</term>
<term>Software maintenance</term>
<term>Software reusability</term>
<term>Telescopes</term>
</keywords><keywords scheme="Pascal" xml:lang="fr"><term>Système modulaire</term>
<term>Logiciel libre</term>
<term>Mesure</term>
<term>Conception modulaire</term>
<term>Maintenance logiciel</term>
<term>Télescope</term>
<term>Miroir</term>
<term>Réutilisation logiciel</term>
</keywords><front><div type="abstract" xml:lang="en">For almost a decade we have been developing an open source control system tor autonomous observatories called Remote Telescope System, 2<sup>nd</sup>
version - RTS2. The system is currently used to operate about dozen observatories. It was designed from the beginning as the ultimate tool for autonomously performing any possible observing plan on any hardware. Its modular design allows exactly this and enables even more. Currently it is used to control not only observatories but also CCD testing laboratories. We present the internal design of this open source observatory and laboratory control package, and discuss its overall structure. We emphasise new developments and our experiences building a community of users and developers of the package. Design of the system modularity is explained in detail, and various approaches to software reuse are discussed, with a demonstration of how the best solution emerged. We describe problems that were encountered as mirror sizes and associated operational complexity grew. We also describe how the system is being used at a CCD testing laboratory, and detail the quick transition from previously unsupported hardware to fully automated operation. We discuss how the system's evolution has affected code design, and present unexpected benefits it is brought. Our experience with use of open source code and libraries are discussed.</div><inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0277-786X</s0>
</fA01><fA02 i1="01"><s0>PSISDG</s0>
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</fA06><fA08 i1="01" i2="1" l="ENG"><s1>Design of modular C++ observatory control system: from observatories to laboratories and back</s1>
</fA08><fA09 i1="01" i2="1" l="ENG"><s1>Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States</s1>
</fA09><fA11 i1="01" i2="1"><s1>KUBANEK (Petr)</s1>
</fA11><fA11 i1="02" i2="1"><s1>PROUZA (Michael)</s1>
</fA11><fA11 i1="03" i2="1"><s1>CUNNIFFE (Ronan)</s1>
</fA11><fA11 i1="04" i2="1"><s1>WILDI (Markus)</s1>
</fA11><fA11 i1="05" i2="1"><s1>STROBL (Jan)</s1>
</fA11><fA11 i1="06" i2="1"><s1>KOTOV (Ivan)</s1>
</fA11><fA11 i1="07" i2="1"><s1>O'CONNOR (Paul)</s1>
</fA11><fA11 i1="08" i2="1"><s1>JELINEK (Martin)</s1>
</fA11><fA11 i1="09" i2="1"><s1>DE UGARTE POSTIGO (Antonio)</s1>
</fA11><fA12 i1="01" i2="1"><s1>RADZIWILL (Nicole M.)</s1>
<s9>ed.</s9>
</fA12><fA12 i1="02" i2="1"><s1>BRIDGER (Alan)</s1>
<s9>ed.</s9>
</fA12><fA14 i1="01"><s1>Institute of Physics, Academy of Sciences</s1>
<s2>Praha</s2>
<s3>CZE</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</fA14><fA14 i1="02"><s1>Image Processign Laboratory, Universitat de València</s1>
<s2>Valencia</s2>
<s3>ESP</s3>
<sZ>1 aut.</sZ>
</fA14><fA14 i1="03"><s1>Instituto de Astrofísica de Andalúcia CSIC</s1>
<s2>Granada</s2>
<s3>ESP</s3>
<sZ>1 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>8 aut.</sZ>
</fA14><fA14 i1="04"><s1>Observatory Vermes</s1>
<s3>CHE</s3>
<sZ>4 aut.</sZ>
</fA14><fA14 i1="05"><s1>Astronomical Institute, Academy of Sciences</s1>
<s2>Ondřejov</s2>
<s3>CZE</s3>
<sZ>5 aut.</sZ>
</fA14><fA14 i1="06"><s1>Brookhaven National Laboratory</s1>
<s2>Upton, NY</s2>
<s3>USA</s3>
<sZ>6 aut.</sZ>
<sZ>7 aut.</sZ>
</fA14><fA14 i1="07"><s1>INAF-Osservatorio Astronomico di Brera</s1>
<s2>Merate</s2>
<s3>ITA</s3>
<sZ>9 aut.</sZ>
</fA14><fA18 i1="01" i2="1"><s1>SPIE</s1>
<s3>USA</s3>
<s9>org-cong.</s9>
</fA18><fA18 i1="02" i2="1"><s1>American Astronomical Society</s1>
<s3>USA</s3>
<s9>org-cong.</s9>
</fA18><fA20><s2>77401V.1-77401V.12</s2>
</fA20><fA21><s1>2010</s1>
</fA21><fA23 i1="01"><s0>ENG</s0>
</fA23><fA25 i1="01"><s1>SPIE</s1>
<s2>Bellingham, Wash.</s2>
</fA25><fA26 i1="01"><s0>978-0-8194-8230-3</s0>
</fA26><fA26 i1="02"><s0>0-8194-8230-7</s0>
</fA26><fA43 i1="01"><s1>INIST</s1>
<s2>21760</s2>
<s5>354000174702880630</s5>
</fA43><fA44><s0>0000</s0>
<s1>© 2011 INIST-CNRS. All rights reserved.</s1>
</fA44><fA45><s0>7 ref.</s0>
</fA45><fA47 i1="01" i2="1"><s0>11-0070228</s0>
</fA47><fA60><s1>P</s1>
<s2>C</s2>
</fA60><fA64 i1="01" i2="1"><s0>Proceedings of SPIE, the International Society for Optical Engineering</s0>
</fA64><fA66 i1="01"><s0>USA</s0>
</fA66><fC01 i1="01" l="ENG"><s0>For almost a decade we have been developing an open source control system tor autonomous observatories called Remote Telescope System, 2<sup>nd</sup>
version - RTS2. The system is currently used to operate about dozen observatories. It was designed from the beginning as the ultimate tool for autonomously performing any possible observing plan on any hardware. Its modular design allows exactly this and enables even more. Currently it is used to control not only observatories but also CCD testing laboratories. We present the internal design of this open source observatory and laboratory control package, and discuss its overall structure. We emphasise new developments and our experiences building a community of users and developers of the package. Design of the system modularity is explained in detail, and various approaches to software reuse are discussed, with a demonstration of how the best solution emerged. We describe problems that were encountered as mirror sizes and associated operational complexity grew. We also describe how the system is being used at a CCD testing laboratory, and detail the quick transition from previously unsupported hardware to fully automated operation. We discuss how the system's evolution has affected code design, and present unexpected benefits it is brought. Our experience with use of open source code and libraries are discussed.</s0><fC02 i1="01" i2="3"><s0>001E03A55C</s0>
</fC02><fC02 i1="02" i2="X"><s0>001D02B09</s0>
</fC02><fC03 i1="01" i2="X" l="FRE"><s0>Système modulaire</s0>
<s5>06</s5>
</fC03><fC03 i1="01" i2="X" l="ENG"><s0>Modular system</s0>
<s5>06</s5>
</fC03><fC03 i1="01" i2="X" l="SPA"><s0>Sistema modular</s0>
<s5>06</s5>
</fC03><fC03 i1="02" i2="X" l="FRE"><s0>Logiciel libre</s0>
<s5>07</s5>
</fC03><fC03 i1="02" i2="X" l="ENG"><s0>Open source software</s0>
<s5>07</s5>
</fC03><fC03 i1="02" i2="X" l="SPA"><s0>Software libre</s0>
<s5>07</s5>
</fC03><fC03 i1="03" i2="3" l="FRE"><s0>Mesure</s0>
<s5>08</s5>
</fC03><fC03 i1="03" i2="3" l="ENG"><s0>Metering</s0>
<s5>08</s5>
</fC03><fC03 i1="04" i2="X" l="FRE"><s0>Conception modulaire</s0>
<s5>18</s5>
</fC03><fC03 i1="04" i2="X" l="ENG"><s0>Modular design</s0>
<s5>18</s5>
</fC03><fC03 i1="04" i2="X" l="SPA"><s0>Concepción modular</s0>
<s5>18</s5>
</fC03><fC03 i1="05" i2="3" l="FRE"><s0>Maintenance logiciel</s0>
<s5>19</s5>
</fC03><fC03 i1="05" i2="3" l="ENG"><s0>Software maintenance</s0>
<s5>19</s5>
</fC03><fC03 i1="06" i2="3" l="FRE"><s0>Télescope</s0>
<s5>20</s5>
</fC03><fC03 i1="06" i2="3" l="ENG"><s0>Telescopes</s0>
<s5>20</s5>
</fC03><fC03 i1="07" i2="3" l="FRE"><s0>Miroir</s0>
<s5>21</s5>
</fC03><fC03 i1="07" i2="3" l="ENG"><s0>Mirrors</s0>
<s5>21</s5>
</fC03><fC03 i1="08" i2="3" l="FRE"><s0>Réutilisation logiciel</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03><fC03 i1="08" i2="3" l="ENG"><s0>Software reusability</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03><fC03 i1="08" i2="3" l="SPA"><s0>Reutilización de logicial</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03><fN21><s1>045</s1>
</fN21><fN44 i1="01"><s1>OTO</s1>
</fN44><fN82><s1>OTO</s1>
</fN82><pR><fA30 i1="01" i2="1" l="ENG"><s1>Software and cyberinfrastructure for astronomy</s1>
<s3>San Diego CA USA</s3>
<s4>2010</s4>
</fA30>
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