... CREATE FULLTEXT CONFIGURATION -- create full-text configuration . CREATE FULLTEXT CONFIGURATION cfgname PARSER prsname [ LOCALE localename ] [ AS DEFAULT ]; CREATE FULLTEXT CONFIGURATION cfgname [ { PARSER prsname | ... PARSER . ... LOCALE . ... Create new configuration test with default parser and ru_RU.UTF-8 locale. CREATE FULLTEXT CONFIGURATION test PARSER default LOCALE 'ru_RU.UTF-8'; =# \dF+ test Configuration "public.test" Parser name: "pg_catalog.default" Locale: 'ru_RU.UTF-8' Token | ...

This example shows a difference between CSS's table model for HTML and for other document formats. The first, HTML, example is defined by HTML to be illegal, as it would lead to overlapping cells if HTML's rules for layout are followed. ... The diagram depicts how the two examples, the HTML one and the almost identical non-HTML one, might be rendered. ... The rendering of the non-HTML example is on the right, it follows the CSS rules and thus has no overlapping cells. ...

... Class List . ... include <iostream> #include < casa/Containers/Link.h > main() { Link<int> *hed = new Link<int>(23); hed = new Link<int>(12,0,hed); hed = new Link<int>(19,0,hed); hed = new Link<int>(10,0,hed); while (hed) { Link<int> *cur = hed; hed = hed->unlink(); cout << cur->val() << " " ; delete cur; } cout << endl; } . ... As each new link is being created, the new element goes at the beginning of the list because the previous head of the list, hed , is being passed in as the next list element...

... 173Wall Peacock We catalogue the brightest extragalactic radio sources at 2.7 GHz. ... These data were originally presented in Wall and Peacock, MNRAS, 216, 173. The values in parenthesis include (units, datatype, example). 1 iauname Name of source in IAU convention (char7, example: '0320-37') . ... 3 ra_1950 rad Right ascension of source in radians (B1950) (real, example: 0.876068) . ... 9 alpha Spectral index of source between 2.7 and 5 GHz (real, example: 0.52) . ... Longair, 1975 . ...

... analysis 3-2 . ... apphot 3-15 . apropos 3-2, A-7 . ... basic2d 21-2, 21-4, 21-23 . boxcar 3-12 . ... calstis 20-1, 21-1 , 21-4 . ... chiplot 23-6 . ... compass 3-9 . ... daophot 3-15 . ... describe 3-2 . ... fitting 3-23 . ... gstatistics 3-12, 3-14 . ... imexamine 3-10, 3-11 , 3-12, 3-15, 26-9 . ... implot 3-10, 3-10 , 3-12 . ... imtab 3-21, 3-22 . ... metric 3-9, 3-10, 28-18 . ... msstatistics 3-12, 3-14 . ... plcreate 3-12, 3-15 . ... rimcursor 3-9, 3-10 . ... xy2rd 3-9, 3-10, 28-19 . ...

Comedi Documentation . ... comedi_get_version_code -- Comedi version code . ... int comedi_get_version_code (comedi_t * device); . Returns the Comedi kernel module version code. A valid Comedi device referenced by the parameter device is necessary to communicate with the kernel module. ... This function is of limited usefulness. ... If the application needs to know of the existence of a particular feature, an existence test function should be written and put in the Comedilib source. ...

... JavaScript 1.1 Plugin objects are predefined JavaScript objects that you access through the navigator.plugins array. A Plugin object is a plug-in installed on the client. ... For example, the following code displays the type and description properties of the first Plugin object's first MimeType object. myPlugin=navigator.plugins[0] . ... Description . ... The following code assigns shorthand variables for the predefined LiveAudio properties. var myPluginName = navigator.plugins["LiveAudio"].name . ...

Appendix C. Display Device Names . ... A "display device name" is a string description that uniquely identifies a display device; it follows the format "<type>-<number>", for example: "CRT-0", "CRT-1", "DFP-0", or "TV-0". ... Display device names can be used in the MetaMode, HorizSync, and VertRefresh X config options to indicate which display device a setting should be applied to. ... That is why specifying the display device name is preferable. ... Appendix B. X Config Options . ...

To get an overview of section 1 (one) of the manual: man 1 intro . ... This displays a one line synopsis of each command that has this keyword in its description. To search the online manual for a command with the phrase "copy files": man -k 'copy files' . ... To check what a command does: whatis more more, page (1) - browse or page through a text file . ... To display the manual page for the cp (copy files) command: man cp . ... To print the manual page for the man command: man -t man . ...

... espfilt (espfilt-0.8.2) [xmmsas_20070708_1801-7.1.0] . ... The default min and max channels will be 2500eV and 12000eV respectively. espfilt eventset=''file1 file2 file3'' withsmoothing=yes smooth=25 this command will cause espfilt to loop through the 3 individual files listed, and change the default smoothing from 60 to 25. espfilt eventset=''MOS2S002.fits'' withspecranges=yes specminchan=500 specmaxchan=12000 this command will change the default minimum and maximum energy ranges. ...

The XPA source code directory contains two test programs, stest.c , and ctest.c that can serve as examples for writing XPA servers and clients, respectively. ... The stest program can be executed with no arguments to start an XPA server that contains the access points: xpa, xpa1, c_xpa (containing sub-commands cmd1 and cmd2), and i_xpa. ... xpaset xpa # send to xpa cat xpa.c | xpaset "xpa*" # send to xpa and xpa1 xpaget xpa # receive from xpa xpaget xpa* # receive from xpa and xpa1 etc. ...

... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

... Corrected geomagnetic coordinates | Let us consider as an example two numerical files with names tp.cng This files contain the information about INTERBALL Tail Probe and POLAR magnetic conjugations. ... The predicted magnetic conjugations correspond to the less then 5 deg geocentric angular distance between the footprints. ... dlt - the difference between two satellites corrected geomagnetic local times (on the second line), . ... GLAT (deg) - the satellite geographical latitude, . ...

Package . Class . ... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ... These links take you to the next or previous class, interface, package, or related page. ...

grdhisteq - Histogram equalization for grd files grdhisteq in _ grdfile [ -G out _ grdfile ] [ -C n _ cells ] [ -D ] [ -N [ norm ] ] [ -Q ] [ -V ] grdhisteq allows the user to find the data values which divide a given grdfile into patches of equal area. ... One could use grdhisteq to write to stdout an ASCII list of those data values which divide the range of the data into n _ cells segments, each of which has an equal area in the image. ... C Sets how many cells (or divisions) of data range to make. ...

polimplot -- Plot a polarization vector map . ... inpol = "" [name] . Input linear polarization image (in %) to plot. inpopa = "" [name] . Input image for position angle of linear polarization vectors (degrees). poi_err = "" [boolean] . ... Name of corresponding polarization position angle error image (degrees). ... This task is a flexible tool for plotting a polarization vector map from two images of the polarization and the position angle of the polarization vector. ...

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ClassљList . ClassљIndex . ClassљHierarchy . ... StelNoGuiPluginInterface Class Reference . An example GUI plugin with an empty GUI. More... #include < StelNoGui.hpp > . virtual class StelGuiBase *љ . getStelGuiBase () const . Get the instance of StelGuiBase implmenting the GUI. ... Definition at line 50 of file StelNoGui.hpp . virtual class StelGuiBase * StelNoGuiPluginInterface::getStelGuiBase . const . ...

SAI VO . ... SAI CAS . ... Web Services . Catalog Access Services . ... SAI VO Wiki . ... Program Access . SAI CAS Wiki . SAI Web Services . ... DSS Mirror . ... We provide an implementation of IVOA standard Simple Image Access Protocol interface to our DSS mirror. Service metadata is available here . Currently, we provide the atlas service only, which returns the list of original DSS images intersecting the requested sky area. ... SAI MSU | ...