Download - VAMDC Portal Demo

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Page 1: VAMDC Portal Demo

VAMDC demo

2/24/2012 Vienna

by Nikolai Piskunov and Kevin Benson

Page 2: VAMDC Portal Demo

VAMDC infrastructure

Node software DB

Node software DB

Database Node

Node software DB

Registry VOSI

. . .

Monitoring . . .

Applications XSAMS

VAMDC Core Infrastructure

Client Applications

Format converters

Format converters

Legacy Applications

Format converters

Applications capable of combining, extracting and processing data from all

VAMDC member databases

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VAMDC demo

1. Portal functionality

2. Test queries

3. XSAMS manipulation

4. Use case for stellar astrophysics (Gaia)

5. Automating workflow

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Demos 1-3

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1.1 Portal functionality

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Status and description of VAMDC databases

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1.2 Portal functionality

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Preview of VAMDC databases capable of responding to a query on specific ions

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2.1 Collision query

2/24/2012 Vienna Finding data of collisional cross-sections for CO and H

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2.2 Spectral line query

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Finding radiative transitions of CO in the 4.5-5 μ region

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3.1 XSAMS content preview

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Selecting ”consumer” converter (BibTeX) for XSAMS received from HITRAN

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3.2 XSAMS content preview

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A fragment of ”consumer” converter presentation of radiative transitions and states as cross-linked tables

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Not quite …

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• Goal: Deriving stellar parameters from observations

• Data and tools involved:

4.1 Stellar astrophysics

Atomic and molecular

data

Stellar models Opacities

RT solver

EOS

SME

Stellar parameters

Spectral synthesis

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• Querying VAMDC

• Converting XSAMS to SME line list format

• Starting SME

• Importing observations

• Importing line list

• Running SME

• Visualizing the results

4.2 What happens

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4.3 Querying VAMDC

Getting a list of atomic transitions in a given spectral region for low excitation atomic energy levels

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4.4 Converting XSAMS to SME input

Using “consumer” converter to create in input for “Spectroscopy Made Easy” (SME) tool

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4.5 Running SME on real observations

SME derives stellar parameters based on VAMDC data

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4.6 Results of SME fit

Resulting SME spectral synthesis compared with the observations

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The end

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5. Automating workflow

Demo 4 was repeated in automatic mode using Taverna workflow system