Example Suite for "Astronomical Measurements Model", version 1.0: The following examples are produced by the modeler using a home-grown python utility called 'voefg' (Virtual Observatory Example File Generator). Additional examples generated by an independently developed DSL-based package called 'jovial' can be found here: Example Suite Summary: Flavor ----- ------------------------------------------------------------- vot VOTable-1.3 standard syntax avot VOTable-1.3 annotated with VO-DML/Mapping syntax xml XML - validates using test_meas_v1.0.xsd which adds serializable elements to the base Meas model schema xxx An internal DOC format XML/DOM structure representing the instances generated when interpreting the template ================================================================================ cartesian_position. Cartesian position for detector coordinates (detx,dety,detz) with Ellipsoid error. o Includes: Position, Error, Ellipsoid ecliptic_position. Standard Ecliptic position (elon,elat) with Symmetrical error. o Includes: Position, Error, Symmetrical equatorial_position. Standard Equatorial position (RA,DEC) in ICRS with Elliptical error. o Includes: Position, Error, Ellipse galactic_position. Standard Galactic position (l,b) with Symmetrical error. o Includes: Position, Error, Symmetrical generic_measure. Stellar magnitude with Symmetrical error. o Includes: GenericMeasure, Error, Symmetrical generic_position1D. For positions not covered by the specialized types, this example illustrates Chandra Mirror Spherical Coordinates (MSC) = [r, Theta, Phi] where: R = radial from reference pixel to object (typically excluded: ie. 1) Theta = off-axis angle (0.0:30.0 arcmin) Phi = Azimuth (0.0:360.0 deg) and includes the [R] coordinate with error and full description of the coordinate space. o Includes: Position, Error, Asymmetrical1D generic_position2D. For positions not covered by the specialized types, this example illustrates Chandra Mirror Spherical Coordinates (MSC) = [r, Theta, Phi] where: R = radial from reference pixel to object (typically excluded: ie. 1) Theta = off-axis angle (0.0:30.0 arcmin) Phi = Azimuth (0.0:360.0 deg) and includes the [Theta,Phi] coordinates with error and full description of the coordinate space. o Includes: Position, Error, Asymmetrical2D generic_position3D. For positions not covered by the specialized types, this example illustrates Chandra Mirror Spherical Coordinates (MSC) = [r, Theta, Phi] where: R = radial from reference pixel to object (typically excluded: ie. 1) Theta = off-axis angle (0.0:30.0 arcmin) Phi = Azimuth (0.0:360.0 deg) and includes the [R,Theta,Phi] coordinates with error and full description of the coordinate space. o Includes: Position, Error, Asymmetrical3D generic_velocity1D. generic_velocity2D. generic_velocity3D. Patterned off the generic position examples, with Velocity measures instead of Position. Errors are given as BoundsND. o Includes: Velocity, Error, Bounds1D o Includes: Velocity, Error, Bounds2D o Includes: Velocity, Error, Bounds3D polarization. Polarization state - representative value of PolStokes.Q, but could be any of the PolState types. There is no Frame or Error associated with this type. o Includes: Polarization proper_motion. Shows the proper motion of a star in an ICRS coordinate system o Includes: ProperMotion time. This example illustrates the most complex Time form. It shows event time as an offset from a reference MJD date with Symmetric error. o Includes: Time, Error, Symmetrical