Requirements from astronomy in the Virtual Observatory era
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Transcript Requirements from astronomy in the Virtual Observatory era
Requirements from astronomy
in the Virtual Observatory era
Bob Mann
Institute for Astronomy & NeSC
University of Edinburgh
Outline of talk
What is the Virtual Observatory (VObs)?
– How is it changing astronomy?
Who in astronomy needs e-Science skills?
–
–
–
–
Data centre staff
VObs middleware developers
Data analysis tool developers
Research astronomers
Summary
– What skills are needed?
– How can these requirements be met?
What is the
Virtual Observatory?
A goal:
– An interoperable federation of the world’s
astronomical data sources
A standards agency/coordination body:
– International Virtual Observatory Alliance
– Its members are VObs projects in Australia,
Canada, China, France, Germany, Hungary,
India, Italy, Japan, Korea, Russia, Spain,
UK, USA, and the EU.
Why is the VObs needed?
We observe across the whole electromagnetic spectrum
ROSAT ~keV DSS Optical 2MASS 2m IRAS 25m
IRAS 100m
GB 6cm
NVSS 20cm WENSS 92cm
Different views of a local spiral galaxy
– Need all of them to understand its physics fully
– The databases holding them are located all over the world
Schematic of the VObs
DB 1
DB 2
DB 3
DB 4
DB 5
App 1 Compute
Resource 1
Registry
Workflow
App 2
App 4
User
Portal
App 3
Compute
Resource 2
App 5
What services will the
Virtual Observatory need?
Data discovery
– Looking up metadata in a registry
Data access
– With/without authentication & authorization
Data integration
– Cross-matching entries in databases
Data manipulation
– Data mining, data analysis, etc
Data centre staff
DB 1
DB 2
DB 3
DB 4
DB 5
App 1 Compute
Resource 1
Registry
• Data Curation:
•Provenance, DBMS design and operations
• Data Access
• Security, Registry Metadata, Web Services
• Data Manipulation
• User-uploaded code, job scheduling
VObs middleware developers
DB 1
DB 2
Web/Grid services for the discovery,
transport and integration of data
Workflow & service composition
Metadata and service registration
Registry
Job management
Workflow
App 3
Security
Compute
Resource 2
Portal
Data analysis tool developers
DB 1
Data Access:
• OGSA-DAI/data access web services
Service Registration
Registry
Integration into workflows
Workflow
Job submission
App 3
Compute
Resource 2
Research astronomers
DB 1
DB 2
Initially:
• Use of portal
Soon:
Registry
Workflow
• Script and tool development
using APIs, local job control,
wrapping apps as web services
App 4
User
Portal
Compute
Resource 2
App 5
Summary of skills needed
Web/Grid services for data discovery,
access, integration and manipulation
Metadata for data & service registration
Data curation – provenance, preservation
Workflow creation and execution
Job control – local and remote
Security
How can these needs be met? (1)
Learning through experience
– Difficult: fast moving field; where to start?
Danger of learning the wrong technologies
– Inefficient: undirected training can be slow
Hiring people with appropriate skills
– Not many people with e-Science skills yet
…and expensive to employ on research grants
– Really need astronomers for some jobs
Danger of losing scientific direction to projects
How can these needs be met? (2)
Existing staff: training courses
– Can be expensive and time-consuming
– Need to budget time and money for them
Funders need to understand their necessity
Future staff: education
– Astronomers: MSc-level courses – either
as MSc or as part of PhD training
– IT specialists: inclusion of e-science
content in CS degree programmes