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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• Structure of the Spectral Package

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The mslist utility is a simple, command-line driven measurement set inspection tool. ... mslist.sh [options] MS_filename > MS_summary.txt 2>&1 . ... data . ... datacolumn=str . ... Choose the data column to display. --field=str . ... mslist.sh --data --antenna = '3&&4' --spw = '0:5~10' --correlation = 'XX,YY' 1641/2015-04-14_071714_ch00000-00511.ms . mslist (Measurement summary and data inspection utility) . ...

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• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• Input Parameters to the Self-Calibration Tasks
• kpvslice: interactive position-velocity slicing

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)
• OYSTER Lab
• A visual tour

... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / Je lon0 / lat0 / scale (Equidistant). Jf lon0 / lat0 / horizon / scale (Gnomonic). ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/grd2xyz.html
• http://xray.sai.msu.ru/~ivan/gmt/man/triangulate.html
• http://xray.sai.msu.ru/~ivan/gmt/man/grdvector.html

... dataset . ... Used only if withrmfset is set to true . ... dataset flat psf . The origin of the detector map: if set to dataset , then the user must specify the name of that dataset, and the table name of the map though detmaparray . If it is set to flat or psf , then the parameters detxoffset , detyoffset , detxbins and detybins define the detector map grid. ... If true , the raw detector map and the bad pixel lists are filtered using the DSS information stored in the spectrum dataset. ...

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• Command-line position entry.

... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... Aperture Coordinate System . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... Position . ...

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• Obsolescent Acquisition Parameters
• VERSION User's Guide

... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...

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• CREATE FULLTEXT DICTIONARY
• GIMP animations: merge-anim example 1
• Zen: GetCovers

... way these widgets work for the user. #include gtk/gtk.h GtkWidget *hscale, *vscale; void cb_pos_menu_select( GtkWidget * item , GtkPositionType pos ) { /* Set the value position on both scale widgets */ gtk_ scale _set_ value _pos (GTK_ SCALE (hscale), pos); gtk_ scale _set_ value _pos (GTK_ SCALE (vscale), pos); } void cb_update_menu_select( GtkWidget * item , GtkUpdateType policy ) { /* Set the update policy for both ...

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• Session Parameters
• Print options
• HyperLEDA documentation: parameter: celpos

... 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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... 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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• Manpage of FITSHDR_EDIT

... To run the <LAYER> version of the example, select: flower.htm . ... However, if the page had several layers with absolute positions, and you wanted to place another layer in a relative position to one of the existing layers, you could use inline JavaScript to calculate the value for LEFT or TOP . ... In this example, there is really no need to use inline JavaScript to position the last flower layer, since you could just let the TOP value default to its natural value, as in the other flower layers. ...

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• Tutorial on Fortran 90, Digital UNIX
• Notation
• Long description for example illustrating positioning with respect to a

Allows you to specify a drift scan: motion at a constant velocity along a great circle. ... The path starts at the new object position (though the telescope actually intersects the path later, see Subtleties ). ... Note that the units are always /sec for both axes. ... The velocity along the path is 0.01 /sec. ... The path is assumed to start when you hit the Slew button (more precisely, when the TCC parses the command). However, it takes the telescope awhile to slew to meet the specified path. ...

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• TUI:Telescope:Slew Window:Options:Axis Wrap
• TUI:Telescope:User Catalogs
• sgs summary

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• A Python-based IRAF Task Parameter Editor
• The SuperCOSMOS Sky Surveys
• ADASS 2002 Conference Proceedings

... A reset button on an HTML form. ... Client-side object . ... JavaScript 1.1: added type property; added onBlur and onFocus event handlers; added blur and focus methods . JavaScript 1.2: added handleEvent method The HTML INPUT tag, with "reset" as the value of the TYPE attribute. ... JavaScript 1.0 blur() None The following example removes focus from the reset button userReset: userReset.blur() This example assumes that the button is defined as <INPUT TYPE="reset" NAME="userReset"> Reset.focus . ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/option.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
• Program parameters

lte-codes . Sterne . ... In 2006, Behara and Jeffery introduced a new file format for the model atmospheres produced by STERNE and used by SPECTRUM and SFIT. ... allow depth-dependent descriptions of composition, and . ... model.lambda_ref <lambda ref > . ... abundance < elem > < abund > . ... structure.abundance < elem > : ( needs N depth ) . ab elem,1 , ab elem,2 , ..., ab elem,Ndepth > . ... structure.tau_ref : ( needs N depth ) . ... structure.opac_ref : ( needs N depth ) . ...

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• Spectrum - control
• sfit help file
• Spectrum v1 - Examples

Stellarium 0.12.3 . ... StelGeometryBuilder Class Reference . ... buildCircle ( StelVertexBuffer < VertexP2 > *vertexBuffer, const float x, const float y, const float radius, const int segments=128) . ... buildCylinder ( StelVertexBuffer < VertexP3T2 > *const vertexBuffer, const float radius, const float height, const int slices, const bool orientInside=false) . ... Build a fisheye-textured sphere. ... Build a flat texture mapped ring with 3D coordinates (for example for planet's rings) More.. ...

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• Stellarium: CLIProcessor Class Reference
• Stellarium: TextParams Struct Reference
• Stellarium: Skybright Class Reference

... 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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... A modern driver for a device will find out the bus-resource configuration without you having to tell it anything. ... In the worst case you must hard-code the bus-resources into the kernel (or a module) and recompile. In the middle are cases such as where you run a program to give the bus-resource info to the driver or put the info in a configuration file. ... You give such bus-resources as a parameter to the kernel or to a loadable module. ... Setserial is often run from a start-up file. ...

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• C Standard Library Functions
• проект SCORPIO-2: parameters
• Writing programs that use comedi and comedilib

The following parameters as a function of the universal time are enclosed in this file. 1. no . ... Universal time date (YYYYMMDD) . ... Universal time (.hhmmss) . ... Geomagnetic local time in the satellite position . ... geomagnetic latitude . ... co-ordinate - . ... system . ... co-ordinate system . ... Solar-ecliptic co-ordinate - . ... Satellite velocity . ...

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• STDA files
• ASCII files description
• Multipoint correlations of the solar wind parameters observed by several