TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• TUI:Telescope:Slew Window:Options:Mag PM
• TCC User's Guide
• TUI:Telescope:User Catalogs

... The function is accessible, if the file with the image is open, and Ю identification of a star field is made. ... a) Load a first image by the command " Open ", and others by the command " Open +". b) Make an identification of the field. c) Open the menu " File ", select " Next " or press . ... It is necessary tree or more images. a) Load the first image by the command " Open" , and others by the command " Open + ". b) Open the menu " Marking ", select "Detect moving objects" or press - . ...

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... Field size . Object name . ... Map size . ... Field size: the approximate size of the map in the Y direction. ... Galaxies: . ... Galaxies, which size exceeds some value depending on the field and map sizes, are displayed with their real positional angles and sizes by 25m isophote. ... In the "tools" fields there are links to the several famous AVO (Astrophysical Virtual Observatory) resources: NED and Simbad databases and DSS2 (Palomar Digitized Sky Survey) images of the corresponding sky area. ...

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... 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 . ...

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... Class . ... FIELD | ... METHOD . ... java.lang.Object ij.plugin.filter.Profiler . ... PlugInFilter . public class Profiler . ... This method is called once when the filter is loaded. ... This method should return a flag word that specifies the filters capabilities. ... ImageJ will lock the image before calling this method and unlock it when the filter is finished. For PlugInFilters specifying the NO_IMAGE_REQUIRED flag and not the DONE flag, run(ip) is called once with the argument null . ...

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• Translator (ImageJ API)
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... The errors associated with several of the pipeline corrections will not manifest themselves until data from individual visits are compared via the plate overlay process. ... The locations of the individual reference stars on each plate determine how to map the data from that visit onto the common master plate. ... The rms residuals of the fit, referred to as the plate overlay residuals , can be as small as 1 mas or as large as 6 mas. ... POSITION Mode Corrections and Errors . ...

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• Introduction
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Unless you specify otherwise sort treats the one or more space characters between words as field delimiters. You may want to sort files where words are separated by another character such as a colon ( : ). Use the -t option to specify another character to act as the field delimiter. For example -t: . specifies the colon ( : ) character as the delimiter. One specific delimiter followed by another indicates an empty field. ... field2 is taken to be empty. ...

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• Options that can be used to change the sort order
• Change an option value permanently

... A Hidden object is used for passing name/value pairs when a form submits. ... JavaScript 1.0 . JavaScript 1.1: added type property The HTML INPUT tag, with "hidden" as the value of the TYPE attribute. ... Property . ... The form contains a "Display hidden value" button that the user can click to display the value of the Hidden object in an Alert dialog box. ... P><INPUT TYPE="button" VALUE="Display hidden value" NAME="button2" . ... Form name:<INPUT TYPE="hidden" NAME="h1" VALUE="Beluga"> . ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/option.htm
• http://www.arcetri.astro.it/~olmi/GRASP/BLAST-01sep051.tci
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm

... This appartus will drop a mass from different heights. When the mass strikes the ground, some percentage of its original energy will be absorbed by the ground. ... The percentage of the energy which is absorbed by the surface on each "bounce" (EAS) . ... The impact velocity of the object will also be given at each bounce. ... Start= Drop the ball after Energy, Mass and EAS have been set; resume after step or pause has been selected . ... Reset = Reset experiment to intial values . ...

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• The Galaxy Gallery: Messier Objects
• Hubble Ultra Deep Field
• Fundamentals of Mechanics

Compilation of cz (radial velocity) measurements . HyperLeda home | Documentation | ... The catalog (table a110 in the database) presents the compilation of redshift of galaxies, z , z = ( - 0 ) / 0 = ( 0 - ) / where and 0 refer the observed and emitted wavelength, and 0 are the observed and emitted frequency. ... For homogeneity of the HyperLEDA, the radial velocity from "radio" convention has to be transferred to redshift using formula cz = V radio / (1 - V radio /c). ... radio measurement . ...

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• HyperLEDA documentation: HyperLEDA: catalogue of designations (a101)
• EXTRACT HOMOGENIZED DATA FOR A LIST OF OBJECTS
• HyperLEDA documentation: compilation on nature of objects (a115)

... Tonight's Sky . ... Observing . ... Sky this Month . ... Star Atlas . ... stars . ... Observing Podcasts . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... How do neutron stars generate steady magnetic fields? ... How can a neutron star exist if those neutrons are just going to pieces? Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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• Previously understood that magnetic fields were directly related to rotation,
• Magnetic fields, subatomic particles, etc., traveling in different directions
• Iт??ve read about background radiation fields that fill the universe. Is the

XMM­Newton CCF Release Note XMM­CCF­REL­209 OM Grisms Astrometry A. Talavera, A. Breeveld June 13, 2006 1 CCF components Name of CCF VALDATE EVALDATE List of Blocks changed XSCS flag OM ASTROMET 0012 2000­01­01T00:00:00 --- FILTER­GRISM10 NO --- FILTER­GRISM20 NO --- POLYNOM MAP NO --- POLYNOM MAP2 NO 2 Changes When using the OM grisms, the position of the sources in the field of view is translated to the grism image in the position of their corresponding zero orders. ...

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• SciSim Changes v2.0.2
• Generation from In-Orbit Data
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Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

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• Spatial Region Coordinates
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... Next: 7 kslice_3d: slicing data Up: Karma User Manual Previous: 5 Volume Rendering a . The <kpvslice> programme allows you to use a two-dimensional image to define a slice through a three-dimensional data cube. ... The slice is drawn on the total column density or velocity field map, and the corresponding position-velocity diagram will appear in the other window. ... To load the cube, press the Cubes button in the left window and select a cube file. ... The image is displayed in the left window. ...

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• SOURCE
• Package: panel
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... To mark coordinate net in plot, first select Plate in menu bar and then Coordinate net in drop-down menu. ... User has possibility to save plot of sky or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print plot of plate select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print. ... To return to the list of centers click on x button in title bar. ...

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This WWW form allows the user to obtain "postage stamp" FITS or jpeg images or contour plots of selected, small fields from the The VLA Low-Frequency Sky Survey (VLSS, formerly VLSS). ... The specified region of the closest VLSS field is returned as a FITS or jpeg format image or a contour plot. ... The VLSS postage stamp server can return a FITS file with the MIME type of image/x-fits; your browser needs to be told a suitable display program for FITS files. ...

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• Help for FIRST Survey Postage Stamp Server incl contour option
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• NVSS Source Search ($Revision: 1.6 $ - running v2.17)

... There are number of features that can be set by the user in the Sparkle Dialog box. ... The Sparkle plug-in computes the luminosity (level of whiteness) of each pixel in the image (the user can see this when the progress window labeled Generating luminosity array... is displayed). ... The threshold value is currently a slider/text field pair which have a precision of .0001. ... Like the Threshold value, the Flare Intensity has both a slider and a text input field for specifying its value. ...

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• Monitoring Options
• Zen: ts changes
• Lighting plug-in

... At Keck we use the graphical tool sky to plan observations and to control the telescope. ... The user controls the telescope by clicking on stars and an overlayed view of the instrument detectors. ... To point the telescope, the sky user selects a pointing origin with the mouse and then drags and rotates the instrument field until the desired orientation appears on the display. ... To point the telescope, the sky user specifies two points: a sky location and a detector location . ...

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• ADASS 2003 Conference Proceedings
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• Towards Optimal Analysis of HST Crowded Stellar Fields

The Spectrograph is intended for multiobject spectroscopy up to 75 objects within the BTA field of view with medium spectral resolution. ... Fibers are shorter then 0.5 m in length and transmit near 80 % of light in the spectral range 3700-9600 A. Fibers are organized in block unit with the possibility to change together with mask. ... The mask has two additional holes to hold a pair of fibers of 3(26") mm in diameter to project the images of stars needed for adjustment the field and guiding. ...

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• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex1
• Laboratory of spectroscopy and photometry of extragalactic objects :MOUSER
• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex

130705 ephemeris tracking . The pnt command has been added to the aotcl interpreter in vxWorks (used for online datataking). within the online tcl interpreter pnt ? ... Load ephemeris file with pnt ephm ld . Track the ephemeris file . Ephemeris tracking was added to the pnt command on 05jul13. ... The new command includes loading an ephemeris file and then tracking using this file. ... The user then starts the ephemeris tracking by issuing the pnt track command: . ... cR current ra,dec . ...

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• Appendix E. Dots Per Inch
• Chapter 11. Specifying OpenGL Environment Variable Settings
• pulsars