For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

... ksnow and ktrek are simple programs to visualise points whose coordinates are in a table. ... With ktrek you can fly through these data points. ... The optional switch -bg sets the background colour of the display window, otherwise it will have the default window background colour. ... Loading the table takes some time because ksnow and ktrek scale the data. Depth . ksnow and ktrek draw the points on the screen using a perspective projection. ... Update can be used to update the display. ...

The XImtool control panel is the main interface for the XImtool display program, on which SAOtng is based. The SAOtng GUI duplicates the most of the functionality of the control panel in its menu and accel buttons, but the control panel is offered as a window-based alternative to run-of-the-mill menus. ... Tile Frames . ... The text display window gives the field X,Y center, X,Y scale factors, and the X,Y zoom factors. ... Fit Frame makes the display window the same size as the frame buffer. ...

Next: Using Image Memories Up: Image Displays Previous: True Colour or . With the term XWindow display we refer to a bitmapped screen supporting the XWindow environment. ... For example, display screens of different sizes may be created and different number of image channels may be connected to any one display. ... You may create several image displays at the same time on your bitmapped screen even though only one display can be the current active display at any time. ... Using Image Memories . ...

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 Astronomical Data Analysis Software and Systems (ADASS) conference is held each year at a different hosting astronomical institution. The conference provides a forum for scientists and programmers concerned with algorithms, software and software systems employed in the acquisition, reduction, analysis, and dissemination of astronomical data. ... The 26th annual ADASS conference will be held from October 16th to 20th, 2016 at the Stazione Marittima Conference Centre , Trieste, Italy. ...

. You can get more information from the manual page for the Bourne shell (sh). To get information about shell programming with another shell, read the manual page for that shell. For example: man ksh . This will display the manual page for the Korn shell. There are a number of books on the different shells and how to program them. Many will be stocked in the computer section of most major booksellers. Or they may be available through your library.

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. ...

Next: Algorithm Up: Description of program searchdup Previous: Program parameters . Program is started by the command searchdup with no parameters. The graphic user interface appears, with all parameters to their default value. After parameter entry, the button START starts data processing. ... It is possible to stop the program clicking button BREAK! ... It is then possible to change some parameters, or to exit the program, by clicking on the EXIT button. ... 2000-06-30 ...

Appendix E. Dots Per Inch . ... DPI (Dots Per Inch), also known as PPI (Pixels Per Inch), is a property of an X screen that describes the physical size of pixels. Some X applications, such as xterm, can use the DPI of an X screen to determine how large (in pixels) to draw an object in order for that object to be displayed at the desired physical size on the display device. ... The NVIDIA X driver reports the size of the X screen in pixels and in millimeters. ... grep -B1 dot . ...

... Here we will look at line plots. We will go through steps, such as changing linestyles and symbols, you can use to modify your line plots. ... IDL> plot, num, line . ... IDL> plot, num, line, psym = 1 . ... IDL> plot, num, line, linestyle = 1 . ... Line Style . ... IDL> plot, num, line, linestyle=2, thick=3 . ... IDL> plot, num, line, psym = 8, symsize = 2.0 . ... IDL> plot, num, line, charsize=2.0, title='GHRS spectrum . ... IDL> plot, num, line, charsize=2.0, xcharsize=0.8, xtitle='wavelength' . ...

... Data Reduction FAQ > The reduced science spectrum displayed in the Reflex window appears good but when I try to plot it, it is quite different. How can I get it? ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Reflex . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... ESO Annual Reports . ... Seminars at ESO Santiago . ... Seminars at ESO Garching . ... ESO Telescope Bibliography . ... Last Update: 01.04.14 ESO . ...

... MAG _Base ? +--- SELECT/CHANGE DATABASE ? Selection of working database file ? +--- LOOK 1 STATION ? Display and correct data of one selected ? station (remove spikes, fill gaps) +--- VIEW DATA ? Display up to 10 plots of selected ? stations and components +--- TYPE DATA ? Type 1-minute data and other information ? from ...

User has possibility to impose some restriction(s) on the Results of calculation. ... Possible set of restrictions depends on coordinates that were specified for planned run. ... The set of the quantities on which may be imposed restrictions in the next run are highlighted on marking Set restrictions . ... Dist. d(R.A.)/dt . ... Phase . ... To impose restriction on any quantity mark check box at the left of corresponding line and then click on the field where you want to introduce limitative value. ...

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

... Proposed directory for placement: /pub/os2/util/system Your name: Andrey Vasilkin Email address: digi@os2.snc.ru Program contact name: (same) Program contact email: (same) Program URL: (none) Would you like the contact email address included in listings? no Operating System/Version: Additional requirements: Replaces: /pub/os2/util/system/sl100.wpi ...

Stellarium 0.12.3 . ... File Structure . ... core . ... 233   void azimuthalGridDisplayedChanged( const bool ) const ; . 234   void azimuthalGridColorChanged( const Vec3f & newColor) const ; . 235   void equatorGridDisplayedChanged( const bool displayed) const ; . 236   void equatorGridColorChanged( const Vec3f & newColor) const ; . 237   void equatorJ2000GridDisplayedChanged( const bool displayed) const ; . 238   void equatorJ2000GridColorChanged( const Vec3f & newColor) const ; . ...

... Meta Index / Home Page / Fast Mode Photometry Window / Annuli controls When clicked the photometry for the selected source is computed and the computed parameters will be displayed and will replace the values for that source in the source-list. Also, an average magnitude will be computed for all the magnitude determinations made by the user, plus the original one, and displayed in the combobox near the bottom of the window. ... XMM-Newton SOC/SSC -- 2008-07-02 ...

Trail encounter . ... Expected meteor rates . ... The Leonids are the debris of Comet 55P/Tempel-Tuttle. ... The Earth's passage right through the centre of trails is associated with the most spectacular meteor displays (studies show that, as well as how close to the centre of the trail you are, the strength of the display also depends on how far along a trail's length you are). ... The encounter with the 1932 trail will lead to enhanced meteor activity: a nice outburst, but below storm level. ...

FIRST SCREEN . Input files : image with wedges and image with spectrum (fits or tiff format). ... What to do : First of all you must fill in the region which the profiles should be taken from, by pressing "range for profiles" button. ... SECOND SCREEN . ... THIRD SCREEN . ... In the first screen you can change the size of the image by pressing "CHANGE SIZE" button. ... After pressing "Next profile" button, click to the same spectral lines in the same order as you did in the first profile. ...