-  Note
-  This web site runs actually under twiki and will be saved statically in the comming weeks. If you want to bookmark this web site, please use the following url which will be permanent: http://www.jmmc.fr/VltiSchool2010 One copy of the key informations will also be saved under the European Interferometry web site . .
 Two lines as a very short Introduction of the Virtual Observatory 
The Astronomical Virtual Observatory aims to offer tools to astronomers that breaks down the difficulties of making all work together: 
-  make data access and discovery easy even if it is too big to fit onto your local machine
-  make tools able to make more that the sum of what each of one can do, thanks to the interoperability
This effort is driven by local national and international communities. Please visit the WWW.IVOA.NET web site.
 Objective of this tutorial 
To give a first overview of VO standards and VO tools, we install onto the local server of the school a copy of one comming catalogue provided by JMMC : 
 Jmmc Stellar Diameter Catalog. This tutorial also uses 
Topcat and 
Aladin
 Get the catalog content of one particular sky area 
 
-  Launch topcat ( $ topcat-full)
-  Enter menu: VO->Cone Search
-  Copy  following ( too long but for demo ) url into field  Cone Search URL:  http://server.org:8080/jsdc-dsa/SubmitCone?DSACATTAB=jsdc.v1_0b3  
-  Define ( by hand ) RA DEC and search radius
 
 Do some plots 
 Sky Plot 
 
-  Select your data in the table list of the main topcat window 
-  Enter menu: Graphics->Sky
-  Assert that Longitude Axis is racolumn  and Latitude isdeccolumn
-  Try the Plot points with radial as well as angular coordinatesbutton and fill theRadial Axisfield with1/plx
-  Enjoy your cone Search by rotating the plot with the mouse.
-  Try to add auxiliary axis  and some other various features....
 
You can do bigger or smaller 
Cone Searches . and use it into the 
Table Combo box of the plots.
 2D Plot 
 
-  Select your data in the table list of the main topcat window and press  
-  Menu: Graphics->Plot
-  Fill X AxiswithVmagandY AxiswithBmag -Vmag
 
 Send data to another VO program 
 
-  Launch Aladin ( $ Aladin) do not launch the old scisoft do not launch the old scisoftaladinversion but useAladin
-  Come back to Topcat
-  Select your data in the table list of the main topcat window
-  Enter menu: Interop->Send table to...->aladin
-  Try to select one area into aladin and view the selection into one 2D plot of topcat : this is the simplest interoperability level.
 Execute your own script on each star selected into Topcat 
 
-  Select your data in the table list of the main topcat window
-  Define one new Activation Actionfrom  theCurrent Table Propertiespanel
-  Choose Execute Custum Codeand fill withexec("computeVisibility.py",toString(LDD),toString(e_LDD))
-  Click into one row of the table or onto one graphic and read the konsoleoutput
 Exercises 
 Multi Conesearch 
How many stars of the JSDC JMMC catalog are located to a maximum distance of 1 degrees of the 
list of sources already seen 
in one previous tutorial . 
 
Note: It is easy to add new coordinates columns in many coord systems :  
-  Select your table in the main topcat window
-  Enter Menu Views->Column info
-  Just add new sky coordinates.
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Proposed by the JMMC technical team
  
 
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