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Hello!. International Virtual Observatory Alliance Ajit Kembhavi, IUCAA, Pune.

Jan 16, 2016

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Page 1: Hello!. International Virtual Observatory Alliance Ajit Kembhavi, IUCAA, Pune.

Hello!

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International Virtual Observatory Alliance

Ajit Kembhavi, IUCAA, Pune

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The Astronomer Vermeer 1632-1675

Data Storage and Retrieval

The Library of Alexandria 3rd Century BC

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Star Positions

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Stars in the Milky Way

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The Hertzsprung-Russell Diagram

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The Data Avalanche

• An increasing number of telescopes and large area detectors are producing immense amounts of data through imaging and spectroscopic surveys.

• Terabytes of data are now available, and Petabytes will soon be available from frequent all sky imaging.

• Vast databases are also being produced through simulations.

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Wavelength Coverage

• The data spans the electromagnetic spectrum from the radio to the gamma-ray region.

• Obtaining, analysing and interpreting the data in different wavebands involves highly specialised instruments and techniques.

• The astronomer needs new tools for using this wealth of data in multiwavelength studies.

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Virtual Observatories

• Manage vast data resources and provide these on-line to astronomers and other users.

• Provide tools for data analysis, visualization and mining.

• Develop interoperability concepts to make different databases seamless.

• Empower astronomers by providing sophisticated query and computational tools, and computing grids for producing new science.

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VO Schema

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Interactions

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The Alliance

Members of the IVOA

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IVOA Technology Initiatives

The IVOA has identified six major technical initiatives to fulfill the scientific goal of the VO concept.

IVOA-LISTS

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• REGISTRIES: These collect metadata about about data resources and information services into a queryable database. The registry is distributed. A variety of industry standards are being investigated.

• DATA MODELS: This initiative aims to define the common elements of astronomical data structures and to provide a framework to describe their relationships.

• UNIFORM CONTENT DESCRIPTORS: These will provide the common language for for metadata definitions for the VO.

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• DATA ACCESS LAYER: This provides a standardized access mechanisms to distributed data objects. Initial prototypes are a Cone Search Protocol and a simple Image Access Protocol.

• VO QUERY LANGUAGE: This will provide a standard query language which will go beyond the limitations of SQL.

• VOTable: This is an XML mark-up standard or astronomical tables.

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VOTable

• This is a new data exchange standard produced through efforts led by Francois Ochsenbien of CDS, Strasbourg and Roy Williams of Caltech.

• VOTable is in XML format. Physical quantities come with sophisticated semantic information.

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VOTable

• The format enables computers to easily parse the information and communicate it to other computers.

• Federation and joining of information become possible and Grid computing is easier.

• VOTable parsers have been developed in Perl, Java and C++.

• Enhancements and extensions are being considered.

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VOTable Data

The data part in a VOTable may be represented using one of three different formats:

– FITS : VOTable can be used either to encapsulate FITS files, or to re-encode the metadata.

– BINARY : Supported for efficiency and ease of programming, no FITS library is required, and the streaming paradigm is supported.

– TABLEDATA : Pure XML format for small tables.

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Science Initiatives

• Many IVOA projects have active Science Working Groups consisting of astronomers from a broad cross-section of the community representing all wavelengths.

• The focus here is to develop a clear perception of the scientific requirements of a VO.

• Projects within the working groups will develop new capabilities for VO based analysis.

• This will enable the community to create new research programs and to publish their data and research in a more pervasive and scientifically useful manner.

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NVO-People

Caltech, Fermilab, JHU, NASA/HEARC, Microsoft, NCSA/UIUC, NOAO, NRAO, Raytheon ITS, SDSC/UCSD, SAO/CXC, STScI, UPenn, UPitts/CMU, UWis, USC, USNO, USRA, CVO

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Registry and DIS

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Terapix

Jodrell Bank

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AVO Prototype Demo

Astrogrid:

Astronomy Catalogue Extractor

AVO: Aladin+SED

VO-India:VOPlot

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CVO Collaborations

• There are three major projects at the CVO involving collaborations with other VO.

• CVO is collaborating with the German Astrophysical VO to incorporate ROSAT X-ray data and catalogues into the CVO system.

• CVO is collaborating with the Australian VO.to incorporate 2Qz and 2DF galaxy spectra into the CVO database.

• CVO is an associate member of NVO and is have put in place some components of the NVO galaxy morphology demo.

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Australian –VO Collaborations

• The distributed volume renderer (dvr) software, is a tool for rendering large volumetric data sets using the combined memory and processing resources of Beowulf like clusters.

• A collaboration between the Melbourne site of Aus-VO and AstroGrid aims to develop the existing dvr software into a grid-based volume rendering service.

• Users will be able to select FITS-format cubes from a number of "Data Centres",have the data transferred to a chosen rendering cluster, and then proceed to visualise the volume of data remotely (See Demo).

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Virtual Observatory - India

IUCAA

Persistent Systems

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VO-India Projects

• VOTable Parser in C++; Streaming data• Web based FITS browser• Visualizer for VIZIER• Statistical packages for VIZIER and beyond• GALics data bases• Data mirror sites• Scientific data mining• Applications beyond astronomy

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The VOPLOT Collaboration

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The VOPlot Collaboration

• The idea for VOPlot was developed through a discussion between VO-I and CDS.

• VOPlot was developed by PSPL and IUCAA and was integrated into Vizier with the help of CDS.

• It was then decided to integrate VOPlot with Aladin, an interface was agreed on, and the integration is now complete.

• The collaboration was carried through a few short visits, phone calls and E-mail.

• Main persons: Sonali Kale et al (PSPL), Pierre Fernique and Francois Ochsenbien. (CDS).

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