... inclusive or left to right For example, to create a mask consisting of a large circle with a smaller box removed, one can use the and and not operators: CIRCLE(11,11,15) !BOX(11,11,3,6) and the resulting mask is: 1234567890123456789012345678901234567890 ---------------------------------------- 1:1111111111111111111111.. 2:1111111111111111111111.. 3:11111111111111111111111.. 4:111111111111111111111111.. ... 6:1111111111111111111111111.. ... 1111111111111.. ... 22:111111111111111111111.. ...

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• The Markers Menu
• Spatial Region Coordinates
• Differences Between Funtools and IRAF Regions

... The previous example, Chapter 12, "Expanding Colored Squares Example," illustrates how to expand and contract the clipping region of a layer without changing the wrapping width of the layer. This example illustrates how to capture mouse events so that the user can make a layer's wrapping width wider or narrower by dragging the mouse. ... how to capture mouse events for a layer . how to change the wrapping width of a layer by using the load() function . ... Capturing Events for the Layer . ...

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comments sql gen Rick Whitman November 27, 1996 Usage The tool is invoked by entering comments sql gen on the command line followed by one argument which is a file specification for the updated load file you want to process. ... Changing any of the mode keywords will invalidate the SQL that is produced by this tool. ... The sql file will be executed to load the values into the database. ffl The database will be queried to get the comments associated with the reference file loaded by unex­hrs­init.lod. ...

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• http://www.stsci.edu/hst/observatory/crds/documents/comments_sql_gen.pdf
• http://www.stsci.edu/hst/HST_overview/documents/multidrizzle/ch44.html
• http://www.stsci.edu/instruments/observatory/cdbs/image/recreate_load_file.ps

. 1. Move the cursor to the start of the text block you want to define. 2. Type M-space (the META character followed by a space). This sets a 'mark' at the start of the 'region'. 3. Move the cursor to the end of the text block you want to define as the 'region'. This sets the 'point' at the end of the 'region'. You do not have to type anything to set this 'point', the 'point' is the location of the cursor.

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The Status popup displays useful information about the state of sets, regions, and graphs. ... When the number of sets is less than 30, this button is not needed, use the scroll bars to view the status of the sets that are not shown in the display. ... Operations in the Status popup are performed by clicking on the operation, then clicking on one or more set numbers shown in the display. ... Clicking on Copy followed by clicking on a set number in the scrolled window will select the set to copy from. ...

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• http://xray.sai.msu.ru/~polar/xmgr/regions.html

... This is not important for drift observations but poses a problem for any observing mode in which the telescope is moving while taking data, since the ALFA beams then will be rotating on the sky. ... The new mode is called ' sky angle tracking ' and is available for all existing observing modes. ... The next figure shows the distance between the beams in declination as a function of hour angle when the telescope is tracking a source with Dec=+10 from rise to set with a sky angle of 19 degrees. ...

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• CIMA Configuration Files
• p12mProg: 12m control program
• software_downloads

XmCCD Copyright 2007-2013 John Kielkopf ======================================= Development Log =============== March 9, 2002 Version 1.0.0 * Support for SBIG cameras using the first public SBIG library * Basic panel for operation with ds9 +--------------------------+ May 22, 2002 Version 1.1.0 * Updated to use libudrv 4.35 +--------------------------+ May 24, 2004 Version 1.2.0 * USB support +--------------------------+ March 1, 2005 ...

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• http://www.astro.louisville.edu/software/sbig/xmccd-5.1/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.2/CHANGELOG

... Magnetospheric boundary layer is a region close to the magnetopause in which magnetosheath plasma has strong influence. ... A new boundary called the free-flow boundary has been suggested to exists between the exterior cusp and the magnetosheath (this is the boundary that is often plotted as a dashed line in schematic figures of the magnetosphere). Boundary layer is a very special region, not only because of the presence of magnetosheath plasma, but also because of the still uncertain topology. ...

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• Magnetosheath [Oulu]
• Dayside aurora [Oulu]
• Ionospheric troughs [Oulu]

... The SAS task especget has been designed to allow extraction of source+background and background spectra, redistribution matrices, and effective area vectors from an EPIC event list with a single command. especget can be launched from the main xmmselect window, in which case an extraction region size optimization algorithm is also ran, which maximizes the signal-to-noise of the net source spectrum. ... When you are happy with your definition, click the button 1D region in the xmmselect window. ...

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• update time
• Defining the spatial area with a region file

... Please note that throughout this exercise you need some patience since the PEARL procedures use the Direct Fourier Transform which is quite slow for the size of map we are trying to work with! . ... Initial chisq= 24.980139 . SVD: will edit 0 singular values! ... Click Update to add the selected number of CLEAN component to the current model (which was empty at the start), self-calibrate the phases, subtract the CLEAN components from the data, and re-display the updated residual and final maps. ...

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• The Very Large Telescope Project
• PWVmonitor.html
• GOODS

Stellarium 0.12.3 . ... Classes . ... Renderer . ... HelloStelModule Class Reference . ... virtual voidљ . ... Update the module with respect to the time. ... Return the value defining the order of call for the given action For example if stars.callOrder[ActionDraw] == 10 and constellation.callOrder[ActionDraw] == 11, the stars module will be drawn before the constellations. ... virtual void HelloStelModule::draw . ... virtual void HelloStelModule::init . ... virtual void HelloStelModule::update . ...

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• Stellarium: SimpleDrawLine Class Reference
• Stellarium: EmptySphericalRegion Class Reference
• Stellarium: TextUserInterface Class Reference

At Arcetri a Radio Astronomy observative and instrumental group is active. ... A catalog of all known maser sources north of -30 degrees is kept updated and is made available to anyone interested. ... The group is involved in the design phase for the Atacama Large Miillimeter Array , a (sub)millimeter interferometer with a large collecting area (about 10000 m2). ... H2O Maser Catalog . ... ADLB Autocorrelation spectrometer . ... Our involvement in the Atacama Large Millimiter Array ( ALMA ) project . ...

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• Arcetri Star-Formation Group Publications
• Procedures for Observations
• CHIANTI: A Database for Astrophysical Emission Line Spectroscopy

... Оборудование (Модераторы: LifeIsGood , Hornet ) > . Firmware Loader and Update для SynScan . ... Оборудование и телескопы . ... Оффлайн . Сообщений: 725 . Благодарностей: 0 . DOB10 Pyrex, FirstScope 90 EQ, SW EQ-6 Pro SynScan . 23 Октябрь 2006, 09:50:50 ? ... Последнее редактирование: 23 Октябрь 2006, 14:20:33 от veifert ? ... Сообщений: 292 . ... Ответ #1 : 25 Октябрь 2006, 09:03:17 ? ... Сообщений: 2125 . ... Сообщений: 5170 . Благодарностей: 148 . ...

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... The clock correction system described here refers the Parkes clock to UTC(NIST) and to UTC as defined by the BIPM. The data to make these corrections in TEMPO are stored in two files: . ... To checkout the repository, do the following on any ATNF machine: cd $CVSHOME cvs co soft_atnf/atas/clkcorr Ensure that the executables are up-to-date: cd $CVSHOME/soft_atnf/atas/clkcorr make Then follow the procedure outlined below to generate the clock correction files required by TEMPO: . ...

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• casacore: images/Regions/WCLELMask.h Source File
• casacore: lattices/Lattices/LCRegionSingle.h Source File
• kpvslice: interactive position-velocity slicing

... Home About Meade Product Information Dealer Locator Customer Support Investor Relations Dealer Support Employment Opportunities Site Map . Meade Instruments Corp. ... Meade Autostar Supplementary Software Downloads . ... To upgrade your Autostar first click on the link below to download the Autostar Update (ASU) Client Application for Windows. ... The most recent versions of AutoStar Update automatically check for the newest versions of the AutoStar Updater and download it if necessary. ...

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• Meade Instruments Corporation - Meade Autostar Update
• Meade Instruments Corp. - Software Downloads
• Meade Instruments Corporation - Operating Instructions #505 Connector Cable Set

... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...

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... Updates to HST Standard-Star Fluxes . ... These data are in an STScI data base named CRCALSPEC and have been divided into two categories to help the user understand the origin and accuracy of these flux distributions. ... 1990, ApJS, 73, 413) and Oke (1990, AJ, 99, 1621) spectra are available. Oke (1990) used the DoubleSpectrograph on the 5-m Hale Telescope to obtain these spectra for HST calibration; and these data are identified in the HST data bases by the keyword OBSMODE=OKE DBSP. ...

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• Guider Image Controller Overview
• Zerostep Procedure
• TUI:Scripts:Scripting Tutorial:Refinements

... AVERAGE/TABLE frame table xy_col outcol [size] . ... BACKGROUND/ECHELLE in out [radx,rady,step] [degree] [smooth] [method] . ... BACKGROUND/SMOOTH input output [radx,rady] [niter] [visu] . ... performs order definition and wavelength calibration . ... DISPLAY/ECHELLE image [g_flag] . ... Extract echelle orders and produces a frame in space pixel-order . ... LOAD/ECHELLE . display echelle orders (and optionally background) positions . ... Plots the overlap region between adjacent orders n and n+1 . ...

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• The use of IRAS data to define H II regions
• Common Range Functions
• mod_proxy_balancer - Apache HTTP Server

... The orbits as follows are considered: INTERBALL Tail Probe (IB_TAIL) & Auroral Probe (IB_AUR), GEOTAIL (NASA/ISAS), and POLAR (NASA). ... The situation investigation aim is to select the following favourable spatial positions (FSP) : . ... FSP3 : That part of the FSP1 & FSP2 time intervals, which corresponds to the magnetic conjugations of the any couple of the considered spacecraft. ... The polar diagram plot . ... The geocentric distance (GCD) of the 4 spacecraft as a function of the time. ...

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• INTERBALL IB_TAIL September 1999 during operation scheduling
• INTERBALL AURORAL PROBE May 1997
• INTERBALL AURORAL PROBE April 1997

Here are all the plug-ins I have written. ... NOTE: Most of these plug-ins have been updated for the developers-only version of the GIMP, release 0.60. ... Until a new official GIMP version is released, the fix is to insert these two lines at the start of gimp.h : #define RGBA_IMAGE 4 #define GRAYA_IMAGE 5 For Texinfo documentation, look at the bottom of this page. ... Updated for GIMP 0.60. ... Quartic suggests that you try this: engrave an image, blur it slightly, and use it as a bump map. ...

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• APOD: Galileo Views Ganymede
• Zen: GinTestUpdate
• Porting Hints