CyberinfraV1, PascalFrancis, Corpus, bibRecord, 000143

Building archives in the virtual observatory era

Identifieur interne : 000143 ( PascalFrancis/Corpus ); précédent : 000142; suivant : 000144

Building archives in the virtual observatory era

Auteurs : Raymond L. Plante ; Gretchen Greene ; Robert J. Hanisch ; Thomas A. Mcglynn ; Christopher J. Miller ; Doug Tody ; Richard White

Source :

Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.

RBID : Pascal:11-0004507

Descripteurs français

Pascal (Inist)
- Découverte connaissance, Interopérabilité, Archive, Astrophysique, Application spatiale, ., Visualisation donnée.

English descriptors

KwdEn :
- Archive, Astrophysics, Data visualization, Interoperability, Knowledge discovery, Space application.

Abstract

Broad support for Virtual Observatory (VO) standards by astronomical archives is critical for the success of the VO as a research platform. Indeed, a number of effective data discovery, visualization, and integration tools have been created which rely on this broad support. Thus, to an archive, the motivation for supporting VO standards is strong. However, we are now seeing a growing trend among archive developers towards leveraging VO standards and technologies not just to provide interoperability with the VO, but also to support an archive's internal needs and the needs of the archive's primary user base. We examine the motivation for choosing VO technologies for implementing an archive's functionality and list several current examples, including from the Hubble Legacy Archive, NASA HEASARC, NOAO, and NRAO. We will also speculate on the effect that VO will have on some of the ambitious observatory projects planned for the near future.

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 Building archives in the virtual observatory era`
A09	`01`	`1`	`ENG`	`@1 Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States`
A11	`01`	`1`		`@1 PLANTE (Raymond L.)`
A11	`02`	`1`		`@1 GREENE (Gretchen)`
A11	`03`	`1`		`@1 HANISCH (Robert J.)`
A11	`04`	`1`		`@1 MCGLYNN (Thomas A.)`
A11	`05`	`1`		`@1 MILLER (Christopher J.)`
A11	`06`	`1`		`@1 TODY (Doug)`
A11	`07`	`1`		`@1 WHITE (Richard)`
A12	`01`	`1`		`@1 RADZIWILL (Nicole M.) @9 ed.`
A12	`02`	`1`		`@1 BRIDGER (Alan) @9 ed.`
A14	`01`			`@1 National Center for Supercomputing Applications, University of Illinois, 1205 W. Clark St. @2 Urbana, IL 61801 @3 USA @Z 1 aut.`
A14	`02`			`@1 Space Telescope Science Institution, 3700 San Martin Drive @2 Baltimore, MD 21218 @3 USA @Z 2 aut. @Z 3 aut. @Z 7 aut.`
A14	`03`			`@1 NASA Goddard Space Flight Center @2 Greenbelt, MD 20771 @3 USA @Z 4 aut.`
A14	`04`			`@1 Department of Astronomy, University of Michigan @2 Ann Arbor, MI 48109 @3 USA @Z 5 aut.`
A14	`05`			`@1 National Radio Astronomy Observatory @2 Socorro, NM @3 USA @Z 6 aut.`
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A43	`01`			`@1 INIST @2 21760 @5 354000174702880170`
A44				`@0 0000 @1 © 2011 INIST-CNRS. All rights reserved.`
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C02	`01`	`X`		`@0 001D02B04`
C03	`01`	`X`	`FRE`	`@0 Découverte connaissance @5 06`
C03	`01`	`X`	`ENG`	`@0 Knowledge discovery @5 06`
C03	`01`	`X`	`SPA`	`@0 Descubrimiento conocimiento @5 06`
C03	`02`	`X`	`FRE`	`@0 Interopérabilité @5 07`
C03	`02`	`X`	`ENG`	`@0 Interoperability @5 07`
C03	`02`	`X`	`SPA`	`@0 Interoperabilidad @5 07`
C03	`03`	`X`	`FRE`	`@0 Archive @5 18`
C03	`03`	`X`	`ENG`	`@0 Archive @5 18`
C03	`03`	`X`	`SPA`	`@0 Archivo @5 18`
C03	`04`	`X`	`FRE`	`@0 Astrophysique @5 19`
C03	`04`	`X`	`ENG`	`@0 Astrophysics @5 19`
C03	`04`	`X`	`SPA`	`@0 Astrofísica @5 19`
C03	`05`	`X`	`FRE`	`@0 Application spatiale @5 23`
C03	`05`	`X`	`ENG`	`@0 Space application @5 23`
C03	`05`	`X`	`SPA`	`@0 Aplicación espacial @5 23`
C03	`06`	`X`	`FRE`	`@0 . @4 INC @5 82`
C03	`07`	`X`	`FRE`	`@0 Visualisation donnée @4 CD @5 96`
C03	`07`	`X`	`ENG`	`@0 Data visualization @4 CD @5 96`
C03	`07`	`X`	`SPA`	`@0 Visualización de datos @4 CD @5 96`
N21				`@1 003`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

A30	`01`	`1`	`ENG`	`@1 Software and cyberinfrastructure for astronomy @3 San Diego CA USA @4 2010`

Format Inist (serveur)

NO :	PASCAL 11-0004507 INIST
ET :	Building archives in the virtual observatory era
AU :	PLANTE (Raymond L.); GREENE (Gretchen); HANISCH (Robert J.); MCGLYNN (Thomas A.); MILLER (Christopher J.); TODY (Doug); WHITE (Richard); RADZIWILL (Nicole M.); BRIDGER (Alan)
AF :	National Center for Supercomputing Applications, University of Illinois, 1205 W. Clark St./Urbana, IL 61801/Etats-Unis (1 aut.); Space Telescope Science Institution, 3700 San Martin Drive/Baltimore, MD 21218/Etats-Unis (2 aut., 3 aut., 7 aut.); NASA Goddard Space Flight Center/Greenbelt, MD 20771/Etats-Unis (4 aut.); Department of Astronomy, University of Michigan/Ann Arbor, MI 48109/Etats-Unis (5 aut.); National Radio Astronomy Observatory/Socorro, NM/Etats-Unis (6 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; 77400K.1-77400K.12; Bibl. 33 ref.
LA :	Anglais
EA :	Broad support for Virtual Observatory (VO) standards by astronomical archives is critical for the success of the VO as a research platform. Indeed, a number of effective data discovery, visualization, and integration tools have been created which rely on this broad support. Thus, to an archive, the motivation for supporting VO standards is strong. However, we are now seeing a growing trend among archive developers towards leveraging VO standards and technologies not just to provide interoperability with the VO, but also to support an archive's internal needs and the needs of the archive's primary user base. We examine the motivation for choosing VO technologies for implementing an archive's functionality and list several current examples, including from the Hubble Legacy Archive, NASA HEASARC, NOAO, and NRAO. We will also speculate on the effect that VO will have on some of the ambitious observatory projects planned for the near future.
CC :	001D02B04
FD :	Découverte connaissance; Interopérabilité; Archive; Astrophysique; Application spatiale; .; Visualisation donnée
ED :	Knowledge discovery; Interoperability; Archive; Astrophysics; Space application; Data visualization
SD :	Descubrimiento conocimiento; Interoperabilidad; Archivo; Astrofísica; Aplicación espacial; Visualización de datos
LO :	INIST-21760.354000174702880170
ID :	11-0004507

Links to Exploration step

Pascal:11-0004507

Le document en format XML

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<front><div type="abstract" xml:lang="en">Broad support for Virtual Observatory (VO) standards by astronomical archives is critical for the success of the VO as a research platform. Indeed, a number of effective data discovery, visualization, and integration tools have been created which rely on this broad support. Thus, to an archive, the motivation for supporting VO standards is strong. However, we are now seeing a growing trend among archive developers towards leveraging VO standards and technologies not just to provide interoperability with the VO, but also to support an archive's internal needs and the needs of the archive's primary user base. We examine the motivation for choosing VO technologies for implementing an archive's functionality and list several current examples, including from the Hubble Legacy Archive, NASA HEASARC, NOAO, and NRAO. We will also speculate on the effect that VO will have on some of the ambitious observatory projects planned for the near future.</div>
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<fC01 i1="01" l="ENG"><s0>Broad support for Virtual Observatory (VO) standards by astronomical archives is critical for the success of the VO as a research platform. Indeed, a number of effective data discovery, visualization, and integration tools have been created which rely on this broad support. Thus, to an archive, the motivation for supporting VO standards is strong. However, we are now seeing a growing trend among archive developers towards leveraging VO standards and technologies not just to provide interoperability with the VO, but also to support an archive's internal needs and the needs of the archive's primary user base. We examine the motivation for choosing VO technologies for implementing an archive's functionality and list several current examples, including from the Hubble Legacy Archive, NASA HEASARC, NOAO, and NRAO. We will also speculate on the effect that VO will have on some of the ambitious observatory projects planned for the near future.</s0>
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<s5>19</s5>
</fC03>
<fC03 i1="04" i2="X" l="ENG"><s0>Astrophysics</s0>
<s5>19</s5>
</fC03>
<fC03 i1="04" i2="X" l="SPA"><s0>Astrofísica</s0>
<s5>19</s5>
</fC03>
<fC03 i1="05" i2="X" l="FRE"><s0>Application spatiale</s0>
<s5>23</s5>
</fC03>
<fC03 i1="05" i2="X" l="ENG"><s0>Space application</s0>
<s5>23</s5>
</fC03>
<fC03 i1="05" i2="X" l="SPA"><s0>Aplicación espacial</s0>
<s5>23</s5>
</fC03>
<fC03 i1="06" i2="X" l="FRE"><s0>.</s0>
<s4>INC</s4>
<s5>82</s5>
</fC03>
<fC03 i1="07" i2="X" l="FRE"><s0>Visualisation donnée</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03>
<fC03 i1="07" i2="X" l="ENG"><s0>Data visualization</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03>
<fC03 i1="07" i2="X" l="SPA"><s0>Visualización de datos</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03>
<fN21><s1>003</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
<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>
</pR>
</standard>
<server><NO>PASCAL 11-0004507 INIST</NO>
<ET>Building archives in the virtual observatory era</ET>
<AU>PLANTE (Raymond L.); GREENE (Gretchen); HANISCH (Robert J.); MCGLYNN (Thomas A.); MILLER (Christopher J.); TODY (Doug); WHITE (Richard); RADZIWILL (Nicole M.); BRIDGER (Alan)</AU>
<AF>National Center for Supercomputing Applications, University of Illinois, 1205 W. Clark St./Urbana, IL 61801/Etats-Unis (1 aut.); Space Telescope Science Institution, 3700 San Martin Drive/Baltimore, MD 21218/Etats-Unis (2 aut., 3 aut., 7 aut.); NASA Goddard Space Flight Center/Greenbelt, MD 20771/Etats-Unis (4 aut.); Department of Astronomy, University of Michigan/Ann Arbor, MI 48109/Etats-Unis (5 aut.); National Radio Astronomy Observatory/Socorro, NM/Etats-Unis (6 aut.)</AF>
<DT>Publication en série; Congrès; Niveau analytique</DT>
<SO>Proceedings of SPIE, the International Society for Optical Engineering; ISSN 0277-786X; Coden PSISDG; Etats-Unis; Da. 2010; Vol. 7740; No. p. 2; 77400K.1-77400K.12; Bibl. 33 ref.</SO>
<LA>Anglais</LA>
<EA>Broad support for Virtual Observatory (VO) standards by astronomical archives is critical for the success of the VO as a research platform. Indeed, a number of effective data discovery, visualization, and integration tools have been created which rely on this broad support. Thus, to an archive, the motivation for supporting VO standards is strong. However, we are now seeing a growing trend among archive developers towards leveraging VO standards and technologies not just to provide interoperability with the VO, but also to support an archive's internal needs and the needs of the archive's primary user base. We examine the motivation for choosing VO technologies for implementing an archive's functionality and list several current examples, including from the Hubble Legacy Archive, NASA HEASARC, NOAO, and NRAO. We will also speculate on the effect that VO will have on some of the ambitious observatory projects planned for the near future.</EA>
<CC>001D02B04</CC>
<FD>Découverte connaissance; Interopérabilité; Archive; Astrophysique; Application spatiale; .; Visualisation donnée</FD>
<ED>Knowledge discovery; Interoperability; Archive; Astrophysics; Space application; Data visualization</ED>
<SD>Descubrimiento conocimiento; Interoperabilidad; Archivo; Astrofísica; Aplicación espacial; Visualización de datos</SD>
<LO>INIST-21760.354000174702880170</LO>
<ID>11-0004507</ID>
</server>
</inist>
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Building archives in the virtual observatory era

Building archives in the virtual observatory era

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