Virtual Observatory & LIGO Roy Williams California Institute of Technology.
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Transcript of Virtual Observatory & LIGO Roy Williams California Institute of Technology.
![Page 1: Virtual Observatory & LIGO Roy Williams California Institute of Technology.](https://reader036.fdocuments.in/reader036/viewer/2022083008/56649e9e5503460f94b9f343/html5/thumbnails/1.jpg)
Virtual Observatory& LIGO
Roy WilliamsCalifornia Institute of Technology
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IVOA is a standards organization
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VO StandardsSimple Cone Search
Simple Image AccessSimple Spectral Access
Space-Time Coordinate MetadataSpectral Data Model
Unified Content DescriptorsVocabularies in the Virtual Observatory
VOTable Format Specification Sky Event Reporting Metadata (VOEvent)
Table Access ProtocolAstronomical Data Query Language
VOSpaceAuthentication Mechanisms
Asynchronous Service PatternIVOA Support Interfaces
IVOA IdentifiersRegistry Interfaces
VOResource: Registry RecordVOResource Schema Extension
fetch data by sky position
data models
service infrastructure
registry
semantics
data exchange
relational/region queries
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Virtual Observatory• model: survey owners make their own VO service
– + new VO-hosted repository if funded • sharing:
– standard services form data grid– VO registry– connections to literature
• analysis: – old tools refitted + new tools in cloud– everyone wants something different
• publication: – connection with journals+data, ADS and semantics
• preservation: – responsibility is with data centers– they hate making good metadata
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Virtual Observatory
• organization: through standard services and VO registry, service validation
• users: more people using surveys for publication • institutions: astronomy data centers
– IPAC, STSCI, HEASARC, etc• new communities: don't like standard services
(too complex, too simple)• standards: http://ivoa.net/Documents/• US project: http://us-vo.org/
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LIGO• Laser Interferometric Gravitational Wave Observatory• to detect the gravitational waves (GW’s) predicted by Einstein’s general theory of relativity (GR).
• NSF requirement for open data• but data is difficult to understand
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LIGO open data
• size ~600 TB per year• plan is to work with OAIS• replication:
– Hanford WA, Livingston LA, Pasadena CA, Milwaukee WI
• analysis is not supported, rather "rich viewing”• preservation
– getting the good metadata out of scientists heads
• designated community– professional astronomers– educated layperson
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LIGO open data
• sharing: VERY carefully. Data is very difficult to understand.• international: US Ligo with French/Italian Virgo.
– Differences on open data question• new communities will have a steep learning curve!• other purposes: PEM channels
– Seismometers Accelerometers Tiltmeters Magnetometers Microphones Radio receivers Weather stations
• http://www.ligo.org/