1 / 11

Publishing FITS files and VOtables in the VO with Saada

Publishing FITS files and VOtables in the VO with Saada. Laurent MICHEL. Observatoire Astronomique de Strasbourg (Fr) Saada: http://amwdb.u-strasbg.fr/saada. Handling Collections. 2. Handling Heterogeneous Data. 1. Output: A SaadaDB. Input: FITS files.

lovey
Download Presentation

Publishing FITS files and VOtables in the VO with Saada

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Publishing FITS files and VOtables in the VO with Saada Laurent MICHEL Observatoire Astronomique de Strasbourg (Fr) Saada: http://amwdb.u-strasbg.fr/saada

  2. Handling Collections 2 Handling Heterogeneous Data 1 Output: A SaadaDB Input: FITS files Data Collection Observations spectrum No code to write spectre spectre spectre spectrum plots misc image table table table table table plots spectre vectors table spectrum images misc misc Liste d’objets table table images spectre Data Collection Simulations image image misc table spectre spectre spectrum plots plots plots misc images image table table Querying Heterogeneous Data Handling Relations 4 3 Saada in One Slide

  3. Demo Steps • Building a SAADA database dedicated to M104 • 3 FITS spectra (Faint HST and INES) • 2 FITS images Galex and Chandra • Running the native SSA and SIA • UCD use • UCD setup • Query Constraints expressed with UCDs

  4. Database creation After having created a PSQL database, the SaadaDB BEIJING is created with spectral coordinates expressed in eV

  5. BEIJING SaadaDB setup Creation of the data collection Sombrero

  6. BEIJING SaadaDB setup • Setup of the product configuration Ines • load all FITS spectra found in directory ines • RA keyword will be taken as right ascension • DEC keyword will be taken as declination • OBJECT keyword will be taken as instance name • All Spectra will be put into the same class (Ines)

  7. Data loading • Loading of the product configuration Ines • Class (table) can be modified while loading process • Data are searched in the FamousGalaxies directory

  8. Database browsing The BEIJING SaadaDB can be accessed at http://localhost:8080/BEIJING after the script tomcatdeploy has been run.

  9. BEIJING SaadaDB VOportal The BEIJING SaadaDB includes a native SIAP/CS/SSAP VO portal.

  10. UCD setup (not shown) The UCD editor relies on the CDS assignator. Saada supports UCD based queries

  11. UCD based queries (not shown) • This is the (beta) SCC portal of the XMM-Newton catalogue. • 10E6 archival sources extracted from 184 different catalogues • Selection of any sources having an heliocentric velocity greater than 100000km/h

More Related