Usual method to evaluate and classify the extaction from an image
Characterisation of the image (quality, PSFs, stability, noise)
Do we need to implement some new storing standards ?
Think about lack of characterisation standard
Noise model definition : very long work
Scientifical quality will depend on the noise model definition
Does the DM includes poisson noise
E. Slezak : ask M. Louys and F. Bonnarel (J. MacDowell) to check if there is something included inthe DM Char. If not : Write note concerning the inclusion of the poisson noise in Char model
Cross use of the images (mosaic) (checking form and flux)
Fusion of images multiwavelength images
Extraction of sources and targets from images
Spectroscopy (P. Prugniel)
find common bricks to different scientifical use cases and easy to implement (for spectrum and observation)
bricks to be built separately included in a "pipeline"
compare models and observations (minimisation tools)
models : stellar athmosphere and stellar population
adjust resolution, redshift and extension
in Montpellier, grid of spectrum which will be accessible soon
lake in DM : characterisation (ok, ongoing work), observation models (we need other information like provenance DM), ...
workflow work depends on provenance
use Dalia (comparison tool, F. Boone) at the end of the workflow process ?
Theory (F. Le Petit)
Simulations codes, 2 codes which will work together, in a first step outside workflows (takes a few days)
Asynchroneous code
Send code to distant from local interfaces to AstroGRID (done with F. Roy)
Results is sent to MySpace in FITS format (interfaces made by J. Normand)
What we hope : extraction could be accessed for part of the data
SNAP (Single Numerical Access Protocol)
Not completely tested now. Version 0.1 to be discussed in China
For cosmologic data to get simulations snapshots (for example with VisIVO)
Question : is it possible to extand it to other simulations (schedule : simulation presentation in Beijing, other domains in Cambridge)
The DM will be presented in China, but still in progress, does not includes limitations
The community is not ready for being interested in Workflow and is mainly concerned on Access Protocol
Synthetical spectra (L. Chevallier)
Using Titan and NOAR for Compton heating.
separation of interface and computing space
TITAN & NOAR should be one brick
pause during the iteration
question concerning the implementation of old softwares with a VO layer in workflows
case of a brick composed by other bricks : do we use on brick or give the details
Tools
News from AÏDA (A. Schaaff)
a trainee is working on the tool packaging
a 6 month trainee will start in September a work around VO (future) standards like Characterisation in the case of workflow and AÏDA will be the testing platform
future evolutions
bricks of bricks (possibility to use macros for macro loops)
"optional links" (run and check afterwards for next optional computation)
following the second meeting demo (prototype), the plugin has been redifined by C. Pestel
new possibilities and facilities, easy to use compared to the script mode
IVOA participation.
note (E. Slezak) in DM concerning noise. check with Mireille and Francois to verify if something is needed or already planned in Characterisation
participate to theory group (provenance model), P. Prugniel and F. Le Petit
usecases not needed in this meeting but they can be added on the WEB pages of the IVOA (F. Le Petit, E. Slesak, P. Prugniel, L. Chevallier and J. Berthier)
interactions with Paul harrison for Application model (A. Schaaff)
plugin aladin-JLOW in apps group (T. Boch)
Working group visibility
posters at SF2A (Grenoble, L. Chevallier-A. Schaaff? ) - JENAM (Ierevan, C. Surace?)- ADASS XVII (Londres, A. Schaaff?)
VOTech : work around AÏDA and JLOW in current cyle, link with standards (characterisation, ...) in the following cycle
Main ongoing work
interoperability of languages (AstroGrid, WEBCOM-G, AÏDA, ...), check with STIC community what are the finalities of the exchanges between workflows. What could be the best approach for standardisation. (contact J. Montagnat)
Bricks
extraction of subparts in n dimesions hypercube
separation of structures in n dimensions hypercube