Difference: SimpleSpectrumLineDMRFC (8 vs. 9)

Revision 92009-09-04 - JesusSalgado

 
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SSLDM RFC Discussion

Review period: 2009 July 21 – 2009 September 15 (Extended!)

July 20, 2009 Page created to encapsulate the discussion of the Simple Spectrum Line DM RFC process.

See http://www.ivoa.net/Documents/SSLDM/20090714/

SSLDM Use Case:

The main use of the SSLDM is to provide data model support to the Simple Line Access Protocol, so to allow the comsuption of Spectral Line List databases using a common/standard interface.

SSLDM"> SLAP Implementations using SSLDM:

  • SLAP Server Name: IASD
    • Type: Observational
    • Publisher: ESA
    • Service Description: SLAP Access to ISO Astronomical Spectral Lines Database
    • Contact: ESA-VO team
    • Spectral Coverage: IR
    • Number of Records: 300 transitions
    • Comment: Client: VOSpec

  • SLAP Name: LERMA
    • Type: Theoretical
    • Publisher: Observatoire de Paris
    • Service Description: LERMA SLAP access to the CDMS and JPL molecules correlated to the Basecol database
    • Contact: N. Moreau & M.L. Dubernet
    • Spectral Coverage: millimetric, sub-millimetric
    • Number of Records: 37500 transitions
    • Comment: Client developed by N. Moreau

  • SLAP Name: NIST
Changed:
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<
    • Type: Theoretical
    • Publisher: National Institute of Standards
>
>
    • Type: Observational
    • Publisher: National Institute of Standards and Technology
 
    • Contact: Yuri Ralchencko
    • Service Description: SLAP Access to NIST Atomic Spectra Database
    • Spectral Coverage: Multiple Coverage
Changed:
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<
    • Number of Records: 142000 transitions !!
>
>
    • Number of Records: 144000 transitions
 
  • SLAP Name: CIELO
    • Type: Observational
    • Publisher: ESA
    • Service Description: SLAP Access to XMM-Newton observed spectral lines from CIELO Database
    • Contact: M. Guainazzi & the rest of ESA-VO team
    • Spectral Coverage: X-Ray
    • Number of Records: 2700 transitions

  • SLAP Name: CHIANTI
    • Type: Observational
    • Publisher: Astrogrid using ESAVO DALToolkit
    • Contact: Kevin Benson
    • Service Description: A database for astrophysical emission line spectroscopy
    • Spectral Coverage: Multiple Coverage

SLAP-like Implementations using SSLDM:

  • SLAP Name: ALMA internal SLAP
    • Type: Observational
    • Publisher: ALMA Archive Group at The University of Manchester
    • Contact: Stewart Williams, Andrew Markwick-Kemper, Sandra Etoka & Gary Fuller
    • Service Description: Internal SLAP services to propagate line list within the project. IVOA spectral line list data model used in database schema
    • Spectral Coverage: Radio
    • Client: Splatalogue
    • Not fully compliant reason: It contains unidentified lines

Comments:


RFC period comments from Working and Interest Groups

Applications

Data Access Layer

Data Modeling

Grid & Web Services

Resource Registry

Semantics

VO Event

VO Query Language

VOTable

Data Curation & Preservation

OGF Astro-RG

Question translated from SLAP RFC pages:

(4) Page 16 (SLAP document), expression of the quantum states; it is unclear to me how this document is going to express the quantum states for the inversion lines (e.g., NH3) or molecules with internal rotation (e.g., CH3OH, (CH3)2O).

-- MasatoshiOhishi

Theory

TCG


TCG Review: Working and Interest Groups

Note that the space for RFC comments from the working groups was intended to spur early review of the document. A formal approval is still requested from each of the WG and IG heads.

Applications

Data Access Layer

Data Modeling

Grid & Web Services

Resource Registry

Semantics

VO Event

VO Query Language

VOTable

Data Curation & Preservation

OGF Astro-RG

Theory

TCG


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