Next: FIT/ROMAFOT Up: The Automatic Path Previous: SEARCH/ROMAFOT . ... This command groups the objects automatically. ... To group remaining objects, one can execute the command once more with the same catalogue and intermediate table, but with an increased maximum number of objects per window and a reduced AR (in the sense just explained). ... The user is trying to group noise peaks. ... After having grouped the objects, the user tries to fit the subframes by executing the command FIT/ROMAFOT . ...

... JavaScript 1.1 Plugin objects are predefined JavaScript objects that you access through the navigator.plugins array. A Plugin object is a plug-in installed on the client. ... For example, the following code displays the type and description properties of the first Plugin object's first MimeType object. myPlugin=navigator.plugins[0] . ... Description . ... The following code assigns shorthand variables for the predefined LiveAudio properties. var myPluginName = navigator.plugins["LiveAudio"].name . ...

... VMS users have the following compilers available: C, C++, Pascal, FORTRAN, and MACRO--which is a low-level language. ... Create a source file containing valid program statements as defined by the language. ... Run the program. ... FORT RECALC $ LINK RECALC $ RUN RECALC When you write your programs, your source files should always have a file type that identifies the programming language being used. ... Users create a source file of MACRO statements and then compile, link, and run, the file. ...

... Animation . Arrow . ... I created the first animation by running Script-Fu / Animators / Fire on the head of an arrow. ... I merged the animation with the background image, and specified a final X offset of -128 (the background is 128 pixels wide). This results in an animation with a nice moving background. Note that you can also use a background that is wider than the image, as long as you specify the width of the background for the final X offset if you want the final animation to loop. ...

... Classes . ... casa . casa::ObjectPool< T, Key > . ... get (const Key key=Key()) . ... The default key and stack, and the last referenced one (for caching purposes). ... template<class T, class Key> . ... Create the pool. template<class T, class Key> . ... Delete the pool. template<class T, class Key> . ... Decimate the stacks and remove any map entry that is completely unused. template<class T, class Key> . ... const Key . ... Get the object stack for the given key. template<class T, class Key> . ...

Keep the size of the tarfile to a minimum by excluding files that can be recreated from files contained in the tarfile. Examples are: .o (object) files that can be recreated by compiling the program source code.dvi files produced by processing TeX and LaTeX source files.ps (postscript) files generated by drawing and publishing packages. After you have created a tarfile, you can then reduce its size by using the compress command. ... This will create a file called project.tar.Z . ...

Next: ZGSC (Compressed GSC) and XSKYMAP . ... This is a preliminary report on an investigation of the quality and properties of plates digitized during creation of the Guide Star Catalog (GSC). The results will be vital for reclassifying GSC objects. ... Many objects are measured on more than one plate, and thus have multiple catalog entries. ... Among the shortcomings of the GSC are: biased magnitudes and incorrect classifications for certain objects, presence of artifact objects. ...

... Load the CD ROM into your reader (assumed to be mounted as /cdrom), and set the location of the disk and with eincdpar ei> eincdpar.ipcevt4="/cdrom/" Then use ecd2pros to create the QPOE file; ei> ecd2pros input FITS file name OR sequence number: 2952 Einstein instrument (hri|ipc): ipc datatype of FITS file (event|image|slew|unscreened): event root name for output files (.): i2952 Using FITS file /cdrom/data/23h/i2357s64.xpa to create QPOE file. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Risks Comparable to NEOs . ... The Increasing Rate of Discovery of Asteroids . ... Comet and Asteroid Collision Probabilities . ... Extreme albedo comets and the impact hazard (PDF Format) . ... Asteroid Impact Animations . ... Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids - 2002 . ... The Spaceguard Survey Report, 1992 (PDF) . Tsunami from Asteroid/Comet Impacts . ...

Projectile Motion: In Aristotle's view, objects moved parallel to the Earth's surface until it was time (i.e. it was their destiny) to fall back to the earth . Aristotle believed that the "natural" state of massive objects was to seek the center of the Earth. When a stone is launched, an impetus is given to it to disturb it from its natural condition. ... Archimedes' catapults lobbed quarter-ton stones at the attacking Roman ships, quickly destroying the clumsy Roman siege engine. ...

MRO Delay Line Socket Initialisation Protocol for Delay Line Computers E. B. Seneta bodie@mrao.cam.ac.uk rev 1.0 13 October 2006 Cavendish Laboratory JJ Thomson Avenue Cambridge CB3 0HE UK Objective To describe the protocol by which network connections are to be made and broken between delay line computers. Scope This document describes how to make and break network connections for the purpose of sending and receiving delay line command, command data, status and telemetry messages. ...