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The Seismic Plus Portal
E. Michel, C. Renié, K. Belkacem,M. Abed/ SPACEINN-WP3-meeting-1 21-22/10/2013 Observatoire de
Paris
Motivations & Objectives
• A large number of seismic data sources (stellar and solar) now
available (CoRoT, Kepler, SDO, etc...)
• Complementary data also necessary and numerous (spectroscopy,
interferometry, etc...)
Issue: data bases are scattered and inhomogeneous
✓ Difficult to fully exploit, need for visibility
✓ Hinders a broad community use of seismic data
Major objectives of the Portal:
✓ Coordinated access to the large variety of data sources available
✓ Provide tools to handle and combine data for a broad scientific
community
Motivations & Objectives
The Seismic Plus is intended to gather in a same well identified
place:
• Homogeneous description of the data available from various sources:
- sources of seismic data (space or ground-based) for stars and the
Sun
- sources of complementary data (space or ground-based)
commonly used in complement to seismic data to lead
interpretational studies
(e.g. fund parameters, astrometric & spectroscopic sources, models
& numerical simulation sources…)
• Tools to access and combine data from these different sources and
possibly produce new outputs
The Portal overall architecture
Three different levels have been defined (L0,L1,L2)
L0: Standard description
of the data sources
L1: Where-is-what?
(WIW)
L2: Data Access &
Handling
Access to
databases
Data Handling (tools)
The Portal overall architecture – L0
L0: Description of the data sources and tools available at the Portal
• This level is intended to provide us with a standard and
homogeneous description of available databases and tools available
at the Portal
- L0.0 : a ‘multi-approach’ presentation
Considering the potentially large number of sources, presentation
according to keywords…
• For each data source, two sub-levels of description are considered:
- L0.1 : Some general text explaining the main content of the
database (following a standard scheme tbd)
e.g.: The GAUDI database provides access to high resolution spectra collected
between XX/XX/XX and XX/XX/XX, in the framework of the COROT GroundBased Seismology Programme, it contains ...
The Portal overall architecture – L0
L0: Description of the data sources and tools available at the Portal
- L0.1.1 : Field descriptions
e.g.: description of the fields as a table
needs some VO
stuff
screen shot of the field description of KEPLER KOI
(http://archive.stsci.edu/search_fields.php?mission=keple
r_koi)
L0 - Census of data sources:
CoRoT archive -- KASOC archive / Kepler archive -- Ground-based
✓Time series: CoRoT complementary archive -- SOHO -- SOHO/VIRGO/PMO6V -SOHO/VIRGO/DIARAD -- SOHO/VIRGOS/SPM –SOHO/GolfSOHO/MDI -SOHO/…LASCO,CELIAS/MTOF/PM/CTOF/STOF/HSTOF/SEM…? -SDO -- SDO/HMI -- SDO/AIA ? -- SDO/… -- GONG -- Bison -- MARK-I
PASTEL -- APOGEE -- P2F -- Hipparcos&Tycho
✓Fundamental parameters: catalogue –(GAIA) -- SSI Stellar Seismic
(Teff, Fe/H, L,pi,…)
Indices
APOGEE (Sloan Digital Survey) -- GAUDI -✓Spectra:
Gaia ESO Survey (GES) -- TBL Legacy -(observed & theoretical):
POLLUX
✓Stellar models:
(Teff, Fe/H, L,pi,…)
Stellar and solar models and
oscillation parameters
• In blue, database within the SPACEINN project
• CF list circulated for inquiry within SpaceInn consortium (aug. 2013)
L0 - Census of tools available in the Portal:
• Tools will appear at different levels of the portal
• They will be whether implemented in the portal or an access will
be provided for already existing tools
Examples :
- Tools to be implemented:
a broad community will be interested in accessing seismic estimates of
masses, radii for a large number of stars
SSI (seismic
indices)
Database of groundbased obs (Teff)
Tool
=
scaling relations
Output
=
seismic masses,
radii
L0 - Census of tools available in the Portal:
Examples :
- Already existing
tools:
visualize specific data to evaluate their
interest (look at a spectrum, an image, a
time series…)
One can use already existing tools such as TOPCAT
(Tool for OPerations on Catalogues And Tables,
http://www.star.bris.ac.uk/~mbt/topcat/)
The portal will use/give access to this tool - no implementation needed
The Portal overall architecture – L1
L1: Where-Is-What? (WIW)
For a given request (e.g., a list of stars), it provides (at least):
The Gaudi data base
provides access to high
resolution spectra
collected from XX/…
- list of sources where data exist,
- Access to description of the source content
star
Source 1
Star 1
X
Star 2
X
…
Star n
Source 2
…
Source n
X
X
X
X
…
…
…
X
X
Possible types of requests – L1
✓For stars:
• List of stars (use of a cross-identifyer, CDS)
• Selection by coordinates + magnitude range
• Type of star (main-sequence / red-giant / etc...)
• Type of variable star (solar-like pulsator / delta-scuti /
etc...)
• Other?
✓For the Sun:
✓For stars & the
Sun:
• period(s) of time
•remarquable events(high activity,…)
• Obs technique/Spectral domain ?
• Coordinates (for resolved observation of the Sun)
• Other?
• Data type (e.g. time series / spectro / imagery / etc...)
• Other?
The Portal overall architecture – L2
L2: Data access & Handling
Data Access from selected sources to :
• Visualize specific data to evaluate their interest (look at a
spectrum, an image, a time series…)
• Download them on his personal computer to exploit them
(according to a list, a selection by position or magnitude…)
Quick look image: light-curve,
spectrum,… if exist
Download data from source n
Download data for star n
star
Source 1
Star 1
X
Star 2
X
…
Star n
Source 2
…
Source n
X
X
…
…
…
X
X
X
X
X
X
X
The Portal overall architecture – L2
L2: Data access & Handling
Data Handling :
• Use tools made available at the portal to produce new
output data from the combination or analysis of input data
New output
TOOL n
star
Source 1
Star 1
X
Star 2
X
…
Star n
Source 2
…
Source n
X
X
…
…
…
X
X
X
X
X
X
X
The Portal – technical options
Portal / Data source interface
The Seismic Plus
portal
Query
VOTable
XML
?
Data Access Layer service
Data archive
Data description
Data access
Tools
VO standard, protocol and format :
TAP : Table Access Protocol
SSA : Simple Spectra Access
…
Specific to data archive
The Portal – technical options
VO standard, protocol and format
For example Table Access Protocol (TAP)
Defines Web service protocol for accessing general table data:
Data queries for data access
Metadata queries for data description
Testing DaCHS framework (TAP implementation developped by the German VO)
with SSI database.
Visibility in VO registries and VO tools like TOPCAT, VOSPEC
Help to define a common language, vocabulary
Make portal developments and maintenance easier
Knowledge and support from OV-Paris
Location near the database
The Portal – Planning & needs
Manpower :
• PI: Eric Michel (Kevin Belkacem)
• Project Manager: Christian Renié
• VO expertise: OVPARIS/Pierre Le Sidaner
• Portal develop.: Mahfoudh Abed (CDD SpaceInn)
Planning :
-deliverable D3.1, month 12: Set of data access and tools to be implemented
The Portal – Planning & needs
Deliverables :
Planning :
• (First) list of data sources and tools -> december 2013
• Need to have balanced (ambitious/reasonable) lists
• Need efficient feed-back from data sources
managers: YOU + others
• Portal Opening (< month 30)