... 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 | ...

Еще в разделе: (Показать все результаты (>1296) - www.sai.msu.su/ )

• ALTER FULLTEXT CONFIGURATION
• CREATE FULLTEXT MAPPING
• COMMENT ON FULLTEXT

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

Еще в разделе: (Показать все результаты (>12986) - www.atnf.csiro.au/ )

• Central Processor Manager CentralProcessor 0.11 documentation
• Casda Upload Utility CentralProcessor 0.11 documentation
• ccontsubtract CentralProcessor 0.11 documentation

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

Еще в разделе: (Показать все результаты (>9693) - www.arcetri.astro.it/ )

• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/javobj.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/javarray.htm

... Meta Index / Home Page . ... Output Files . ... Input Files . ... Parameters | Errors | ... Comments . ... Different types of detector | ... Initialisation . ... Description | ... A detector map | ... Detector map filtering | ...

Еще в разделе: (Показать все результаты (>17812) - xmm.vilspa.esa.es/ )

• Housekeeping parameters
• Detailed description.

asnphot -- plot magnitude as function of subpixel position asnphot association . ... calnicb style association input file with list of images to be processed and co-added. istar . star to be used for the photometry. ... Calls "qphot" to perform photometry on the same star in each image of an association. ... The task requires that "alignasn" has been run on the association in order to define the stars to be used and in order to measure accurately the shifts between images. digiphot, qphot ...

Еще в разделе: (Показать все результаты (>254) - www.stecf.org/ )

• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• WCS2DR (V1.0) --- Jan00 --- WCS2DR (V1.0)

gmtset - To change individual GMT default parameters gmtset PARAMETER1 value1 PARAMETER2 value2 PARAMETER3 value3 ... gmtset will adjust individual GMT defaults settings in the current directory's .gmtdefaults file. If no such file exists one will be created. ... To change the dpi to 600, set anotation font to Helvetica, and select grid-crosses of size 0.1 inch, try gmtset DOTS_PR_INCH 600 ANOT_FONT Helvetica GRID_CROSS_SIZE 0.1i gmt , gmtdefaults . ...

Еще в разделе: (Показать все результаты (>504) - xray.sai.msu.ru/ )

• Parameters of binary compact star evolution

... Chapter 10: Fine Guidance Sensors (FGS) > 10.1 Introduction to the FGS . ... The Instrument Configurations and Operating Modes described in the following section are used for the Visit and Exposure Specifications. ... Note that many of the Optional Parameters have default values; in such cases, an Optional Parameter entry in the Visit and Exposure Specifications is necessary only if it is desired to override the default value . ... Table 10.1: Supported Instrument Parameters for the FGS . ... FGS . ...

Еще в разделе: (Показать все результаты (>15938) - www.stsci.edu/ )

• Introduction to STIS
• Examples of GHRS Phase II Proposals
• Index

. Next: Example Up: Long-Slit and 1D Previous: Command Summary . For the storage of control parameters and results, the context LONG uses a number of special keywords. They are intialised by the command SET/CONTEXT LONG , their values can at any time be listed by typing SHOW/LONG . The following table provides a brief description of the purpose of the LONG keywords: . љ . Table: Keywords Used in Context LONG . љ . Table: Keywords Used in Context LONG (continued) . Rein Warmels . Mon Jan 22 15:08:15 MET 1996

Еще в разделе: (Показать все результаты (>2684) - www.sao.ru/ )

• Echelle Spectra
• HyperLeda: example of online pipeline processing
• Session Parameters

... 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. ...

Еще в разделе: (Показать все результаты (>1157) - jet.sao.ru/ )

• comedi_get_version_code
• проект SCORPIO-2: parameters
• comedi_get_cmd_generic_timed

... 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) . ...

Еще в разделе: (Показать все результаты (>2307) - star.arm.ac.uk/ )

• lte-codes: sterne model atmospheres

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