... ALTER FULLTEXT .. OWNER -- change the owner of a full-text object . ALTER FULLTEXT { PARSER|DICTIONARY|CONFIGURATION } name OWNER TO newowner ; . ... The new owner of the full-text object. ... Then we change owner of the new dictionary. ... CREATE SCHEMA test; =# CREATE FULLTEXT DICTIONARY test.synonym LIKE pg_catalog."synonym"; =# SHOW search_path; search_path ---------------- "$user",public =# SET search_path TO test,public; =# ALTER FULLTEXT DICTIONARY synonym OWNER TO megera; . ...

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 . ...

... This is done by taking in all input files the extension whose name is specified by the maintable parameter (called 'merged extension' in what follows) and merging the columns into a single output extension of the same name. ... Its contents is taken from the CCDID keyword (and QUADRANT for EPIC PN). ... To propagate other column specific keywords, they must be specified manually via the extensionchecks , mainattributes , maxattributes and minattributes parameters (see above). ...

... 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. ...

... 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) . ...

... 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 . ...

... 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. ...

Some Documentation for the IDL ICRED . ... This is the system which recieves all command inputs. it decodes inputs and selects tasks, parses parameter inputs and also runs the 'go', 'list' and 'help' commands. It does no error checking, for example to see if the parameter inputs are sensible (e.g. it does not check if an x-range has been entered as 'chicken', rather than a more understandable range of say 10,20). 2) the task decoders: icred_<taskname>.pro . ... Other tasks or important commands: . ...

... 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 . ...

... A cookie is a small piece of information stored on the client machine in the cookies.txt file. ... Transparently, with the server-side JavaScript the client object, when using client-cookie maintenance. ... name = value . ... DOMAIN= domainName ] . PATH= pathName ] . ... Set-Cookie: PART_NUMBER=ROCKET_LAUNCHER_0001; path=/ When client requests a URL in path "/" on this server, it sends: . ... Set-Cookie: SHIPPING=FEDEX; path=/foo When client requests a URL in path "/" on this server, it sends: . ...

Stellarium 0.12.3 . ... Classes . ... Renderer . ... ClassљList . ... LogBook Class Reference . ... voidљ . enableLogBook (bool b) . ... virtual boolљ . ... Detect or show the configuration GUI elements for the module. ... virtual voidљ . ... getCallOrder ( StelModuleActionName actionName) const . ... virtual bool LogBook::configureGui . boolљ . ... virtual void LogBook::draw . ... The main StelStyle instance should be passed. virtual void LogBook::init . ... virtual void LogBook::update . ...

... Abstract Determine whether a file exists. ... Brief_I/O VARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- fname I Name of the file in question. ... Examples The following code fragment illustrates the use of exists_c . ... Exceptions 1) If the input name is blank, the error SPICE(BLANKFILENAME) will be signalled. ... Files None. ... Version -CSPICE Version 1.1.0, 08-FEB-1998 (NJB) References to C2F_CreateStr_Sig were removed; code was cleaned up accordingly. ...

... This tool is designed to create formatted and unformatted file-by-file reports from fits headers, or fits files. fitsreport reads from a configuration file all the keys to be displayed: . ... retrieve non-FITS information (file name, path name). ... The tool reads all fits files in the given path, evaluates the configuration file fitsreport_raw.cfg (to be in ${DFO_CONFIG_DIR}) and dumps the output into out. ... This is more evident in the other config file, fitsreport_raw.cfg. ...

... 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) . ...

tranback -- Transform an X,Y position from output to input pixel position using the same conventions as drizzle tranback xout yout . xout = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... If "output" the input image center is mapped to the center of the output grid, rotated about that center and then shifted along the grid of the output image. ...

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" | ...

... In this paper, a project aiming to allow access to data archives by means of a query-by-example mechanism is described. The basic user query would simply be the submission of an input image, either 1-D or 2-D; the system should allow retrieval of archived images similar to an input one on the basis of some ``resemblance parameter". ... A system called QUBE is currently being designed to support the QUery-By-Example paradigm in accessing astronomical data archives. ... the QUBE User Interface. ...

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...

... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...