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. ...

The left mouse button controls the creation and manipulation of region markers or cursors. ... Text When a marker type of selected, new markers of that type can be created using the left mouse button. The current default marker type is displayed below the menu. ... Set Default Marker Name (and Color) . ... Reset the fix parameter state of currently existing markers to match the global state set by the -fix command switch or by the Edit Global Fix Params For New Markers option in the Markers menu. ...

... User Guide ] Task: tvflag Purpose: Interactive editing of a UV data set on a TV device. ... The user should make sure, if the display device is capable of creating menus that the menu program has been loaded ``before'' running this routine (eg. xpanel for the XMTV) - see the User's Guide or Cookbook under TV Devices for details. ... The user may edit the data in one of two ways: 1) By entering commands at the keyboard; or 2) by selecting commands from the listed menu items. ... Minimum match is used...

Next: FIT/ROMAFOT Up: Study of the Previous: Study of the . SELECT/ROMAFOT frame [int_tab] [wnd_size] . With this command the user can select a number of well behaving stellar images to determine the Point Spread Function on the frame. ... SELECT/ROMAFOT displays the frame (or part of it) on the image display and allows the user to select the objects. The image display cursor and its control box is used to select the objects . ... If these are unknown the default can be used. ...

... 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. ...

D.Chumbalov and A.Romashchenko. ... Proc. 40th International Symposium in Mathematical Foundations of Computer Science (MFCS), Part 1. ... Preliminary version: Proc. 6th International Computer Science Symposium in Russia (CSR), 2011.) download: arXiv:1102.5538 , slides: pdf . ... Bulletin of the EATCS (The Logic in Computer Science Column by Yuri Gurevich) no. 97 (2009) pp. 126--136. download: pdf . ... Lecture Notes in Computer Science 5162 Springer 2008 pp. 527-538). download: pdf . ...

Next: Calibrating amplitude errors Up: Calibrate data Previous: Calibrate data Contents . ... The results will be entered in the calibrations table (strictly speaking an array of calibration entry structures), and automatically applied to the data. ... L IST List the entries . ... UNDO Remove entries and corresponding calibration . U NCAL Completely remove calibration from the selected data only. ... U NDO U NCAL will remove all calibrations for the selected data and all stars/scans. ...

Set the display of the status bar, tool bar, locator bar, and properties associated with the display of the pointer position in the Locator bar. ... Set fixed point . ... When the fixed point is set, and the display format is (DX, DY), (DIST), or (R, Theta) then give the location relative to the fixed point. ... Set the fixed point to (0.0, 0.0). ... DX, DY] Display the delta in X and Y of the position of the mouse relative to the fixed point, or (0, 0) if no fixed point has been selected. ...

... Interactive photometry can be done on the selected sources. ... The Main Window . Summary of Widgets . Table . delete . Regions colour . ... photometry . ... Source-List Table . ... Delete . ... Source Selection Window . ... old regions . new regions . ... Omdetect Window . ... Imaging Mode Photometry Window . ... Background Determination Controls . ... User regions . ... Delete table . ... Fast Mode Photometry Window . ... Background Regions window . ... Background regions . ...

... select data groups menu . activate fields (radio buttons) to qualify the query . ... select menu option to record query selections, enter a unique report option name and save option . ... select Visit Data menu from data groups menu . ... select LRP menu from data groups menu . activate LRP name "query" radio button and select LRP 02035A from automatically activated dropdown menu . ... select LRP menu from data groups menu and select LRP 02036A from automatically activated dropdown menu . ...

... Logout of current observing session if necessary . ... Select 'Line' from the observing modes . From the ' Choose receiver' widget: Choose ALFA & then 'Select this receiver now' . Dismiss widget . From the 'Observer's interface' select Pointing Control . Within Pointing Control click on ' catalog' . ... Leave this widget open (i.e. don't click 'dismiss') . ... Dismiss the 'New improved IFLO Control' widget. ... From the WAPP ALFA widget click on 'Configure WAPP ALFA' . ...

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

Permitted Context: SELECT . ... The OPTION element can only occur within a SELECT element. ... When the form is submitted, the NAME of the enclosing SELECT element is paired with the OPTION's VALUE attribute to contribute a name/value pair for the selection. ... CLASS . ... The string to be used together with the name attribute of the enclosing select element, when submitting the form. ... SELECTED . ... This attribute is used within menus to define shaped hotzones associated with this option's value. ...

Next: The exercise level Up: Using Ceilidh as a Student Previous: Using Ceilidh as a Student . ... This menu is identical whether it is obtained from the system level of Ceilidh using the sc command, or by entering Ceilidh with a -c argument. ... Course Summary button) If the teacher remembers to keep the information up-to-date, this command gives you a summary of the timetable for your course, with . ... ceilidh -c pr1 . ... If you entered the course level from the system level using first ceilidh . ...

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. ...

... It runs on unix, MacOS and possibly on Windows. ... On MacOS or Windows, double-click TUI. If MacOS complains that the application is unsigned then right-click TUI and select Open. ... If you have never run TUI before, set up your preferences before proceeding (for help on any item, right-click on the control and select Help from the menu that appears): . ... To save your window positions and remember which windows to open at startup, select Save Window Positions from the TUI menu. ...

As an obligatory preparing for the application to participate in the IAO a short report of National Olympiad of the current year with a set of all problems used on the Olympiad has to be presented by the applicating team. ... The final minutes (protocols written in Latin or Cyrillic in form of tables) of the Olympiad (evaluating of solutions of the students participated in the last stage of the Olympiad) should be included as well. ... Historical data of the National Astronomy Olympiad: . ...

home education > resources . ... Education from Mercury . ... Selected Topical Bibliographies . Astronomy Education Bibliography . ... Astronomy . ... Goldman, S. "Prime Time Astronomers: The Astronomers TV Series" in Sky Telescope, May 1991, p. 472. ... Goldman, S. "Astronomy on the Internet" in Sky Telescope, Aug. 1995, p. 20. ... Marschall, L. "Virtual Professional Astronomy" in Sky Telescope, Aug. 1995, p. 92. ... Wallin, J. "Astronomy Education on the Web" in Sky Telescope, Nov. 1997, p. 68. ...

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...