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TutoVoIntro
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%INCLUDE{"SchoolMenuBar"}% %TOC% ---+ 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 : [[JMMCSearchCalCDSCatalogReadme][ Jmmc Stellar Diameter Catalog]]. This tutorial also uses *Topcat* and *Aladin* ---+ Get the catalog content of one particular sky area 1 Launch topcat ( ==$ topcat-full== ) 1 Enter menu: =VO= -> =Cone Search= 1 Copy following ( too long but for demo ) url into field =Cone Search URL= : http://server.org:8080/jsdc-dsa/SubmitCone?DSACATTAB=jsdc.v1_0b3 1 Define ( by hand ) RA DEC and search radius ---+ Do some plots ---++ Sky Plot 1 Select your data in the table list of the main topcat window 1 Enter menu: =Graphics= -> =Sky= 1 Assert that Longitude Axis is =ra= column and Latitude is =dec= column 1 Try the =Plot points with radial as well as angular coordinates= button and fill the =Radial Axis= field with =1/plx= 1 Enjoy your cone Search by rotating the plot with the mouse. 1 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 1 Select your data in the table list of the main topcat window and press 1 Menu: =Graphics= -> =Plot= 1 Fill =X Axis= with =Vmag= and =Y Axis= with =Bmag -Vmag= ---+ Send data to another VO program 1 Launch Aladin ( ==$ Aladin== ) %X% do not launch the old scisoft =aladin= version but use ==Aladin== 1 Come back to Topcat 1 Select your data in the table list of the main topcat window 1 Enter menu: =Interop= -> =Send table to...= -> =aladin= 1 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 1 Select your data in the table list of the main topcat window 1 Define one new =Activation Action= from the =Current Table Properties= panel 1 Choose =Execute Custum Code= and fill with =exec("computeVisibility.py",toString(LDD),toString(e_LDD))= 1 Click into one row of the table or onto one graphic and read the =konsole= output ---+ Exercises ---++ Multi Conesearch How many stars of the JSDC JMMC catalog are located to a maximum distance of 1 degrees of the [[%ATTACHURL%/sources.vot][list of sources]] already seen [[Tuto2ObservationPreparation][in one previous tutorial]] . * [[%ATTACHURL%/sources.vot][sources.vot]]: List of sources into votable format Note: It is easy to add new coordinates columns in many coord systems : 1 Select your table in the main topcat window 1 Enter Menu =Views= -> =Column info= 1 Just add new sky coordinates. <!-- too complex to be computed inside topcat Compute visibility Compute one new column that compute the VIS2 in K band for each stars for a maximum interferometer baseline of 200m. --> -- Proposed by the JMMC technical team
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2010-05-19 - 16:42
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List of sources into votable format
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