... 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 | ...

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• ALTER FULLTEXT CONFIGURATION
• DROP FULLTEXT CONFIGURATION
• DROP FULLTEXT MAPPING

... badpixfind searches for pixels identified as containing no useful data, and uses this information to produce an output file. ... A bad pixel map (or mask) can also be produced. An important point regarding the bad pixels is that there are essentially three separate (though not exclusive) sets of bad pixels that must be dealt with. ... The user is able to specify maximum and minimum allowed values (via the parameters lothresh and hithresh ) to screen for hot and dead pixels. ...

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• Parameters

... 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 . ...

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• Introduction to STIS
• Introduction to the ACS
• Introduction to WFC3

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• mod_macro - Apache HTTP Server
• mod_session_crypto - Apache HTTP Server
• Determination of the Detector Parameters

... Input via keyin format is of the form keyword = value . ... The input keywords are not case sensitive. Most of the values required by SCHED, except for file names in case sensitive systems like unix, are also not case sensitive. keywords are, in all cases, limited to 8 characters in length. ... Keyin values can be mathematical statements in parenthesis; for example, dur = 15 rep = (4*5) This example shows the most likely way in which this capability might be used in SCHED input files. ...

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• makecube CentralProcessor 0.11 documentation
• Central Processor Manager CentralProcessor 0.11 documentation
• User Parameters - Preparation of the Science field data CentralProcessor 0.11

... L-Wide . ... Receiver History . ... Available Filters: . ... Use with e.g. filter 5) NOTE 2 1120-1220 3 1230-1470 4 1550-1820 5 1100-1800 6 1360-1470 7 1320 hipass NOTE 8 1180-1280 9 1280 hipass (ext Output unit. ... Consequently, the calibration for data collected using the hipass 1320 and the hipass 1370 filters only will be mis-calibrated (i.e. by using the opposite polarisation calibration data). ... It is now possible to select any bandpass filter that is not in the 1320 hipass band. ...

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• CIMA Configuration Files
• Arecibo Observatory: 800-MHz Receiver
• WAPP File Format Page

... 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) . ...

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• Homepage of "Jorick Vink"
• lte-codes: sterne model atmospheres

... 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. ...

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• pyQC: script structure
• dfosVNCserver
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

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• Initial Distributions of Binary Parameters
• Initial binary parameters

Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...

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• A Computer-Based Technique for Automatic Description and Classification of
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• Automatic Detection of Linear Features in Astronomical Images

Next: The Reduction Session Up: Echelle Reduction Previous: Standard orientation . ... The command SHOW/ECHELLE displays only those parameters which must be set according to the options and methods chosen for the reduction. ... Current parameters are saved with the command SAVE/ECHELLE name , where name is the session name. ... Current parameter values are set to the default value with the command INIT/ECHELLE , or set to the values of a previously saved session with INIT/ECHELLE name . ...

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• Mean astrophysical parameters from LEDA
• Session parameters
• Parameters

The MOD and IOPT parameters value depend of the external magnetic field model (MOD), used during magnetic mapping and IOPT version (IOPT = Kp + 1), see the table: . MOD . External model . IOPT range . ... N.A.Tsyganenko, Planet. Space Sci., ... N.A. Tsyganenko, A magnetospheric magnetic fields model with a warped Tail current sheet: Planet. Space SCI., ...

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

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

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• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: TextParams Struct Reference
• Stellarium: RingParams Struct Reference

... Exploring the physics of Type Ia supernovae through spectral analysis . ... Their progenitor scenario as well as the details of the explosion mechanism remain a mystery. ... It produces a supernova spectrum for a given luminosity, photospheric velocity, time since explosion and several elemental abundances. Tweaking these parameters to produce a spectrum that fits an observed spectrum is a complex, as of yet, manual task. ... The search space is large and complex. ...

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• COALA - Sanjoy Nandi

seeing -- Create a simulated ground-based star image based on a model of atmospheric turbulence seeing output xdim ydim gamma fwhmx fwhmy . output = "" [image] . The name for the output image to be created. xdim = 512 [integer] . The X dimension for the output image. ydim = 512 [integer] . The Y dimension dor the output image. gamma = 1.6666 [real] . ... For a discussion of the significance of this please see the discussion below and the references given. fwhmx = 5.0 [real] . ...

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• ASNPHOT (Nov98) --- nictools --- ASNPHOT (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

... Description . ... The SCORPIO-2 project: . ... The multi-mode spectrograph SCORPIO-2 was developed using the experience of observations at the 6-m telescope BTA with the SCORPIO focal reducer . ... The focal reducer consists of several units ('floors') mounted in the common case in the following order (from the telescope focal plane): . ... The focal reducer is connected with the platform-adapter which used for guiding by offset stars and for illumination the spectrograph by calibration lamps. ...

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• проект SCORPIO-2: parameters
• comedi_get_cmd_generic_timed
• comedi_from_phys

... 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. ...

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• SAI OCL Catalog Structure
• SAI OCL Catalog Description

... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/Type...

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

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• Brief description of GRS
• INTERBALL-TAIL KP
• INTERBALL-TAIL KP list

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. ...

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