Within this use case you learn about the difference between intrinsic
linear size and apparent angular size, a difference that is frequently
at the center of astronomical problems. Star clusters are the objects
used to illustrate this difference. You also learn some basic facts
about star clusters, whose distribution in space has helped us to
understand the structure of our Milky Way. Thanks to Aladin, you will
be able to explore their distribution on the sky on your own.
This draft standard describes a means to present usage examples for
TAP services in a way that is partially machine readable while
primarily being consumable by humans. This is now part of DALI;
identifiers created as fragments into this record are invalid and must
now point to fragments of http://www.ivoa.net/rdf/examples.
The tutorial uses VOSA to analyse members of the Collinder 69 open
cluster by crossmatching a given local set of objects and accesses VO
services to crossmatch the objects with 2MASS to receive colors. The
resulting SEDs are analysed using different fit functions.
Within this use case you learn about the constellations of the
Zodiac, i.e. those crossed by the apparent path of the Sun during the
year. Together with some characteristics the orbital motion of the
Earth, in this use case you also find a short excursion into history
of astronomy. The use case also introduces the precession of the
equinoxes.
Within this use case you discover the shape and thickness of the disc
of our own Galaxy by counting stars within and around the Milky Way.
With the use of both Aladin and Stellarium you draw the line
corresponding to the disc of the Milky Way in a coordinate diagram.
GAVO's ADQL reference card briefly gives an overview of the SQL
dialect used in the VO. It is available as a PDFfile and as Scribus
source under the CC-BY license.
The GAVO puzzlers are little training problems solvable by standard
VO techniques (data discovery, SIAP, Cone Search, TAP). They assume
some familiarity with common astronomical concepts (they were
originally given out during meetings of the German Astronomische
Gesellschaft) but are designed to be solvable using common, standard
tools and in reasonable time. Solutions are also given.