... It is possible that the length of a parameter value can become large (indeed quite huge). In this case, it is convenient to store the parameter value in a file and then to use the file name in place of the parameter value. ... For example, assuming the file name contains the text chicyg , then % histo in=@name is equivalent to % histo in=chicyg These @ files can be nested, and multiple @ files can appear on a line (separated by commas). ... The @ file can contain many lines. ...

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• Host Command-Line Interface
• Central Processor Manager CentralProcessor 0.11 documentation
• Tasks

... Default . ... dataset . ... The input combined event list. ... For exposure map generation the BADPIX0n and BADPIX1n pair of tables is also required. ... The output event list, a filtered copy of the input mergedset . ... list of tables . ... If true, an exposure map for each node is added to the output dataset, overwriting any previous versions of the maps. ... If true, parameter expimageset specifies a second output dataset in which the combined exposure map is placed as the primary image. ...

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. Next: Edition of the Up: Typical Run Previous: Creation of the . All of the atomic data listed in 13.2.1. are needed by the program and are to be entered via this table. A template can be found in MID_CLOUD: ABSP.TBL . The quoted parameters are from Morton and Smith (1973) and according to the author the wavelengths are: . vaccum for 2000 ?, air for 2000 ? . Command: . The actual format of this table is described in section Auxiliary Data. Pascal Ballester . Tue Mar 28 16:52:29 MET DST 1995

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• Permanent telescope parameters
• Saving and Loading Session Parameters
• Parameter estimation

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_session_crypto - Apache HTTP Server

... java.lang.Object java.awt.Component java.awt.Container java.awt.Window java.awt.Frame ij.text.TextWindow . ... public class TextWindow . ... Constructor Detail public TextWindow (java.lang.String title, java.lang.String data, int width, int height) . ... public TextWindow (java.lang.String title, java.lang.String headings, java.lang.String data, int width, int height) . ... public TextWindow (java.lang.String path, int width, int height) . ... Method Detail public void append (java.lang.String text)...

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• StackWindow (ImageJ API)
• API Help (ImageJ API)
• WaitForUserDialog (ImageJ API)

... A couple of new tasks have also been added; including, SAACLEAN to the NICMOS package, 'tweakshifts' to the DITHER package and a Python interface to SExtractor. Updated or New Tasks: ===================== 1. NEW TASKS: - 'tweakshifts' added to the DITHER package: This prototype version of 'tweakshifts' provides an automated interface for computing residual shifts between input exposures being combined using MultiDrizzle or PyDrizzle. ... Changes to CALSTIS: - Updated to Version 2.19. ...

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• Python: module shelve
• Index
• Simulation Parameters

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• Stellar parameters from calibrations of spectral types
• Score reports
• OLAS integration test suites

... GUIDE'' (Graphical User Interface for a Data Environment) is an interactive IDL widget-based package that enables users to retrieve selected sets of satellite instrument data and perform various types of graphical analyses on them, without writing a specialized program. GUIDE simplifies the task of laying out multiple plots on a page by (1) using a page-editor to define and laying out multiple ``panels'' which contain the ``plot objects'', and (2) integrating data retrieval functions. ...

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• A Python-based IRAF Task Parameter Editor
• DIRT: The Dust InfraRed Toolbox
• Indexing and Searching Distributed Astronomical Data Archives

... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

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• Structure of the Spectral Package
• Parameters
• *imexamine* - General analysis of image containing many sources

The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...

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• Table of Minor planet lightcurve parameters
• Parameters of lightcurves of minor planets

. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/h' F2
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo E
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es

Stellarium 0.12.3 . ... Classes . ... Renderer . ... StelQGLTextureBackend Class Reference . ... constructFromImage (class StelQGLRenderer *renderer, const QString & path , const TextureParams &params, QImage &image) . Construct a StelQGLTextureBackend from an image. ... constructFromPVR (class StelQGLRenderer *renderer, const QString & path , const TextureParams &params) . ... constructAsynchronous (class StelQGLRenderer *renderer, const QString & path , const TextureParams &params) . ... path . ...

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• Stellarium: SerialPort Class Reference
• Stellarium: StelIndexBuffer Class Reference
• Stellarium: TelescopeClient Class Reference

Next: Presentation of the results Up: World Wide Web version Previous: WWW access . On the main page, a very short description of the program may be found. ... The first link brings the user to a very friendly interface of the main code, where all parameters can be set and the calculations can be started. The second lonk provides a list of papers containing the results of the Scenario Machine calculations beginning from 1983 untill 1996 and a short description of the code. ...

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• The Effect of Relativistic Wind on Accretion Flow Parameters
• Initial parameters of compact stars
• Other parameters of the evolutionary scenario

... The e-mail interface of the CATS is designed like CGI for the call of the basic procedures: select and match from the html-forms and the program is a lexical analyser, distinguishing keywords and parameters from the electronic letter sent to the address `cats@sao.ru'. ... The output of result is forseen in the same formats as in other forms of the access to the CATS. ... out[put] < arg1 arg2... > . ... ra [ < arg1 > ] < arg2 > < arg3 > ... min max [center] . ... window < arg1 arg2 ... > . ...

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• SCORPIO parameters
• проект SCORPIO-2: parameters
• Parameters of the 41 Dra system components

Shell scripts can act like standard UNIX commands and take arguments from the command line. Arguments are passed from the command line into a shell program using the positional parameters $1 through to $9 . Each parameter corresponds to the position of the argument on the command line. ... For example: cat printps # This script converts ASCII files to PostScript # and sends them to the PostScript printer ps1 # It uses a local utility "a2ps" a2ps $* | lpr -Pps1 printps elm.txt vi.ref msg . ...

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• Security Considerations

... spectrum . ffit . ... grids . ... These commands read in a grid of model spectra. ... Values for the parameters are taken from the input models themselves, to avoid mixups. The syntax of the command arguments is precise. model{ . ... If there is only one spectrum to fit, one should set default parameters for the secondary which lie within the model grid, with <L_2/L> being a very small value. ... The output is saved in a file <file.fit> , where <file> was the name of the spectrum being fitted. ...

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• Sfit Control Language: Classified Listing
• Armagh Observatory
• SCL Sfit Genetic Commands

... Bojan Nikolic web pages (r. 329) . ... Since version 0.12, libAIR comes with a simple command line interface to the routines which retrieve the water vapour and the phase correction coefficient. Currently only the very simplest model is supported, in which the all of pressure, temperature and water vapour column are free parameters, and they are inferred from the four observed water vapour radiometer readings. ... Command line interface to libAIR and water vapour column retrieval . ...

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• The Tenth Cambridge (10C) Survey
• OptInt PmWiki : Forms
• OptInt PmWiki : Include Other Pages

This page should contain a form to pass parameter value for a program producing figures illustrating the dependence of optical properties of different scatterers on their parameters. Specify the parameters and press start calculation button to produce a figure. ... Independent variable: x v a/b alpha Re(m)? another? ... Number of curves: 1 2 3 . ... Curve #1: . Particle shape: sphere spheroid another? TE/TM mode: TE TM . Other parameters: x= Re(m)= Im(m)= a/b= alpha= . ...

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• Database of Optical Properties -- Level: database
• Database of Optical Properties -- Level: subsubpage

lsst.coordConv љ unknown . ... coordConv::FK4CoordSys Class Reference . ... FK4CoordSys (double date=1950.0) . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom (double &toDir, double &scaleChange, CoordSys const &fromCoordSys, Coord const &fromCoord, double fromDir, Site const &site, double tai=0) const . ... virtual double coordConv::FK4CoordSys::dateFromTAI . ... virtual double coordConv::FK4CoordSys::taiFromDate . ...

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• lsst.coordConv: coordConv::AppTopoCoordSys Class Reference
• lsst.coordConv: coordConv::ObsCoordSys Class Reference
• lsst.coordConv: coordConv::FK5CoordSys Class Reference

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

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• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• WCS2DR (V1.0) --- Jan00 --- WCS2DR (V1.0)