Displays the current status of NICFPS spectrograph and allows you to change the configuration. ... Once the instrument builders have more time with the instrument we plan to refine the controls. ... Select TUI:Save Window Positions to remember the state of this checkbutton. ... The contextual menu on each control can return that control to the current setting of the instrument. ... the current set of filters. ... Current : reset all configuration widgets to the current state of the instrument. ...

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• TUI:Instruments:Echelle:Echelle window

The WFPC2 camera configuration and filter set require a substantial number of apertures for full utilization of its capabilities. All possible aperture and filter combinations are given in Table 3.14 . Each camera has an associated 'optimum' aperture close to the geometric center of its field-of-view (FOV). ... The aperture designations are WF2, WF3, WF4, and PC1 for the individual cameras and WFALL for the three-WFC combination. ... CCD . ... Optimum center WF2 . ... Optimum center WF3 . ...

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• ACS Instrument Handbook
• Space Telescope Imaging Spectrograph Instrument Handbook
• ACS Instrument Handbook for Cycle 20

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

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... Circles are used to depict the source positions. ... A optional ID label can also be displayed alongside the circle, corresponding to the row num- ber of that source in the input source list. ... These circles are in fact DS9-type regions, which can be written out to a le for future use (for example, when running a later DS9 session) by setting withregionfile to true, and specifying the desired le name via the regionfile parameter. ... This is a text le containing region descriptions for each source...

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• http://xmm.vilspa.esa.es/sas/7.1.0/doc/srcdisplay.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/srcdisplay.ps.gz
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/srcdisplay.ps.gz

If the image header contains World Coordinate System information, SAOtng will display WCS positions as the mouse is moved across the image. The format for the display is controlled by the Coords Menu (or using the right mouse button on the screen WCS display). ... WCS information is displayed on the lower part of the image. ... The coordinates are returned in the current format, (e.g. if your image supports WCS information, you can get RA/Dec output). ...

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• General usage.
• *tvimcontour* - Overlay contours and/or source positions on the display
• QPOE Files

... Charge Coupled Devices (CCD) are currently by far the most widely used type of detector in astronomy. ... After a brief introduction to the VLT Control System, the VLT CCD Detectors Control Software is presented. The VLT Control System is a distributed system consisting of a set of UNIX Workstations, dedicated to high level operations, such as coordination of sub-system activities and interface to the users, and VME-based Local Control Units (LCU), dedicated to the control of sub-systems hardware. ...

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• WinTICS-24 Version 2.0 and PFITS-An Integrated Telescope/CCD Control Interface
• POW: A Tcl/Tk Plotting and Image Display Interface Tool for GUIs
• Novel Use of a Simulator for the Calibrations of Scientific Instruments

Contents] [Prev page] [Next page] [Index] . Navigator 4 from Netscape, which is part of the Communicator product suite, includes three new areas of functionality that taken together give you Dynamic HTML. The three components of Dynamic HTML are style sheets, content positioning, and downloadable fonts. Used together, these three components give you greater control over the appearance, layout, and behavior of your web pages. ... Introducing Downloadable Fonts . ...

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• User interface
• Adding Variables to CONFIG.SYS

... Next, the screen displays "Press 0 to align or Mode for Menu." Press "0" if you wish to begin Automatic alignment (or Easy Align, depending on your telescope model), or press Mode if you wish to choose a manual alignment method ("Automatic Alignment" displays, and you can press MODE to go through the menu to find other alignments). ... Note: If you press the "?" key while "Ctr Brightest Star" displays, the alignment star that AutoStar has chosen will display. ... Alignment successful" displays. ...

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• Meade Instruments Corporation - #497 Autostar Computer Controller for ETX-90EC,
• LX200 and LX600 Sensor Control Board (Left Forkarm)
• LX200 and LX600 Sensor Control Board (Left Forkarm) - Parts - Products

... User Guide ] Task: tvall Purpose: Interact with a previously displayed image Categories: visual display TVALL is a WERONG/MIRIAD task which allows interactive modification of the TV lookup tables, etc. ... A menu for operations to be performed will appear on the TV screen. ... Blink between two channels (The mouse y-coordinate determines the blink rate. ... Hit any button to stop blinking). Fiddle the lookup tables (The transfer function is governed by the mouse position. ...

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• VLBI Wiki | Main / P483ObservingNotes
• Interactive Flagging - BLFLAG
• Event-driven Tasks and Graphical User Interfaces

Next: FIT/ROMAFOT Up: The Interactive Path Previous: FIND/ROMAFOT . ... To examine the catalogue table created by the command FIND/ROMAFOT one should use the command ``M'' followed by the sequential position of the object. ... A subframe with the selected star at the center is presented to the user. ... During the examination of the objects passed by FIND/ROMAFOT it often happens that several stars are asked to fit together in the same window and some of these are in the catalogue table. ...

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• Statusbars
• mod_info - Apache HTTP Server
• Text Entries

... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...

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• Power GrabberTM
• FPG Power Grabber

XmTel ----- XmTel is a Motif-based telescope control program based on INDI, the Instrument-Neutral Distributed Interface. ... See the files LICENSE and COPYRIGHT for the details. ... About Epoch ----------- XmTel assumes that the telescope is set to "Epoch of Date", which means that it is using ideal celestial coordinates precisely aligned today. ... XmTel assumes that target coordinates entered from the keyboard are in the Epoch that the telescope coordinates are currently displayed in. ...

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• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-5.1/DOCUMENTATION
• http://www.astro.louisville.edu/software/xmtel/xmtel-7.1/DOCUMENTATION
• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-3.1/docs/nexstar/GetRA-DEC.txt

... Apache HTTP Server Version 2.2 . ... Location /server-info> . ... You may wish to use mod_authz_host inside the <Location> directive to limit access to your server configuration information: . ... In particular, this module can leak sensitive information from the configuration directives of other Apache modules such as system paths, usernames/passwords, database names, etc. ... For example, http://your.host.example.com/server-info?config will show all configuration directives. ?<module-name> . ...

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• Displaying Errors with the JavaScript Console
• HwB: ASCII Table (Offline)
• FIRPO News

... The package stsdas.graphics needs to be loaded (to run imdisp_pos for getting # the NDC's of the display image) # set imtype="fits" # print " " print " *** Start of impol SPECIAL instrument demo *** " print " [stecf.impol and stsdas.graphics need to be loaded] " print " " # # (First delete any model reflection nebulae left over from previous demos) # print " Deleting any old demo files " imdel reflneb1*.fits verify=yes # # An input (intensity) image is required. ...

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• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
• ST-ECF IRAF package

... The package stsdas.graphics needs to be loaded (to run imdisp_pos for getting # the NDC's of the display image) # set imtype="fits" # print " " print " *** Start of impol SPECIAL instrument demo *** " print " [stecf.impol and stsdas.graphics need to be loaded] " print " " # # (First delete any model reflection nebulae left over from previous demos) # print " Deleting any old demo files " imdel reflneb1*.fits verify=yes # # An input (intensity) image is required. ...

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• http://www.eso.org/observing/etc/doc/hgraph.html
• A visual tour
• pyQC: overview

OptInt PmWiki : Pm Wiki / Page List Templates . ... template first:) . ... template last ...:) sections to specify output for the first or last page in the list or a group. ... template]] (:template defaults order=name:) (:template first:) Pages ordered by group (:template first {=$Group}:) Pages in group [[{=$Group}/]] (:template each:) * [[{=$FullName}]] (:template last {=$Group}:) {=$Group} contains {$$GroupPageCount} pages. (:template last:) {$$PageCount} pages total. [[#templateend]] . ...

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• OptInt PmWiki : Url Approvals
• NVSS Image ftp service Documentation Help for NVSS Image ftp service
• OptInt PmWiki : FDR Todo Lists

There are 5 main areas in the display, the menu bar at the top, the locator bar just below, the toolbar along the lefthand side of the display, the status bar at the bottom, and the drawing area where graphics are drawn. ... The toolbar runs along the lefthand side of the display, and provides functions to manipulate the axes scaling of active graphs, by scrolling and mouse powered zooms. ... Click on Draw to freshenup the drawing area with the current set of graphs, parameters and active sets. ...

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• http://xray.sai.msu.ru/~polar/xmgr/status.html
• http://xray.sai.msu.ru/~polar/xmgr/view.html
• The Focal Plane Instruments

... 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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• Journal "Peremennye Zvezdy"
• Trailing Planets
• Астронет > Trailing Planets

... The aostatus display is an X application and can be run from most any sun or linux box at the ao. The destination X server needs to have TrueType fonts installed. ... Linux displays need to configure themselves for TrueType fonts. ... The sun fonts come already installed. ... All that is needed is the following xset command: xset fp+ /usr/openwin/lib/X11/fonts/TrueType Then to run aostatus on the openindows display: /home/aoui/display/solaris/aostatus . ... Here is a screenshot of aostatus. ...

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• ON/OFF (Position Switching)
• Observer's Display
• Appendix C. Display Device Names

Stellarium 0.12.3 . ... Classes . ... LabelMgr Class Reference . ... intљ . labelObject (const QString &text, const QString &objectName, bool visible=true, float fontSize=14, const QString &fontColor="#999999", const QString &side="E", double labelDistance=-1.0, const QString &style="TextOnly") . ... labelScreen (const QString &text, int x, int y, bool visible=true, float fontSize=14, const QString &fontColor="#999999") . ... setLabelText (int id, const QString &newText) . ... virtual voidљ . ...

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• Stellarium: TelescopeTCP Class Reference
• Stellarium: Nebula Class Reference
• Stellarium: StelSkyPolygon Class Reference