... 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) . ...

To create a tarfile containing several files: tar cvf data.tar *.dat . This creates a tarfile data.tar containing all the files in the current directory which have the filename extension .dat . ... To create a tarfile of a directory: tar cvf project.tar Project Project/README Project/Makefile Project/Makefile Project/main.c Project/screen.c Project/menus.c Project/calculator.c Project/setup/configuration . ... This creates a tarfile book.tar containing the directories text and illustrations . ...

Examples of pipeline processing . ... This page presents examples of "on the fly" processing of FITS astronomical data available on the WEB using the HyperLeda pipeline tools. ... In many cases, raw data are archived and a consisten description of the file (FITS header) allows to process them on the fly. ... This first command makes a "pre-view" display of the image. o=fa:L93111HP1/00147&z=vg . ... The result of a pipeline processing is a FITS file that you can read as a normal disk file. ...

Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties . ... If necessary, data have been determined for the different crystallographic axes. ... In the following we give some examples of the data and their possible applications. Table: Summary of data measured in the Jena laboratory, which are currently available from the JPDOC. compound . ... amorph. ... Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties root 2003-03-06 ...

OptInt PmWiki : Pm Wiki / Local Customizations . ... A Wiki Administrator can make a lot of customizations simply by setting variables in the /local/config.php and defining cascading style sheets in /pub/css/local.css files. Any group or page can also have its own configuration file and configuration css file . ... As a result, the core pmwiki.php script makes extensive use of PmWiki.Variables to determine how markup sequences will be processed and what each individual page will output. ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Modules . ... Description: . ... This module is designed for the use in test suites and large networks which have to deal with different httpd versions and different configurations. ... IfVersion [[!] operator ] version > .. ... httpd version is equal . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

... Default FTS configurations contain in 4 tables in pg_catalog schema, namely, pg_ts_cfg , pg_ts_parser , pg_ts_dict , pg_ts_cfgmap . To facilitate management of FTS objects a set of SQL commands, described in FTS Reference Part I , is available. ... CREATE FULLTEXT CONFIGURATION public.testcfg LIKE russian_utf8 WITH MAP; =# ALTER FULLTEXT CONFIGURATION public.testcfg SET PARSER htmlparser; . ... By default, the first visible schema is the pg_catalog , so that system FTS objects always mask users. ...

Stellarium 0.12.3 . ... Classes . ... Scripting . ... Scripting Engine . ... Script Console . ... Since version 0.10.1, Stellarium includes a scripting feature based on the Qt Scripting Engine . ... Prior to version 0.10.0, Stellarium used a different scripting engine called StratoScript . ... Prior to version 0.10.0, Stellarium had a simple scripting engine, known as StratoScript . ... This script prints "Hello Universe" in the Script Console output window. core.debug( "Hello Universe" ); . ...

... To run the <LAYER> version of the example, select: flower.htm . ... However, if the page had several layers with absolute positions, and you wanted to place another layer in a relative position to one of the existing layers, you could use inline JavaScript to calculate the value for LEFT or TOP . ... In this example, there is really no need to use inline JavaScript to position the last flower layer, since you could just let the TOP value default to its natural value, as in the other flower layers. ...

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. ...

... spectrum . ... SPECTRUM will compute synthetic spectra, line profiles equivalent widths, specific intensities, assuming LTE, from model atmospheres of early-type stars. ... sterne models . file containing model atmosphere in 2006 Sterne format . ... T=25000, log g=4.0, vt=0, 1400-1415A. a) NLTE model atmosphere, spectrum computed with SYNSPECv25 (black). b) LTE model atmosphere, same linelist in converted format, spectrum computed with SPECTRUM (red) using this input file and this linelist . ...

... Use of This Manual . ... Spectral-Line Observing at Arecibo (3.25 Mbyte) + Spectral line Appendices (0.56 Mbyte) ( HTML page ) . ... Data Analysis . ... Continuum Observing at Arecibo (0.36 Mbyte) + Continuum Appendices (0.31 Mbyte) . ... Pulsar Observations at Arecibo (4.03 Mbyte) + Pulsar Appendices (0.70 Mbyte) ( HTML page ) . ... VLBI Observing at Arecibo (0.36 Mbyte) + VLBI Appendices (0.35 Mbyte) . ... Introduction to Computing at Arecibo (0.33 Mbyte) + Computing Appendices (0.32 Mbyte) . ...

... However, init, like almost all programs, uses functions from libraries. ... It comes from the standard C libraries, on a GNU/Linux system, glibc. ... They are libraries of these functions. ... There are two ways programs can use these library functions. ... For example, here are the libraries that bash uses: . ... Use ldd to find out what libraries init uses. ... Write, compile and link a program that uses this library. source code, see Building a Minimal Linux System from Source Code for urls . ...

Underdetermined sets is a new type of data structures (terms) developed in Actor Prolog . ... The point is that an underdetermined set can include some indefinite rest (a tail) like a list in usual Prolog . At the same time, the order of elements of an underdetermined set can be arbitrary one and it does not affect results of unification of underdetermined sets. Moreover, Actor Prolog guarantees that a rest of an underdetermined set never contains elements that are explicitly given in the set. ...

... How to display images in IRAF using the display task. ... The most general IRAF task for displaying image data is the display task, the best choice for a first look at HST imaging data. ... Display the image with the IRAF display task, using the syntax appropriate for the file format (Chapter 2 explains how to specify GEIS groups and FITS extensions): tv> display fname.c0h [2] 1 (GEIS group 2) . ... If you want to display an image with high dynamic range, you may prefer to use logarithmic scaling. ...

... pyqc.tar v2.0 (May 2014) . ... pyQC script structure . ... plot modules . ... instrument-independent module creating 2D images from a single detector (raw frame, master, comparison to reference) . ... instrument-independent module creating a simple 2D image from a raw or product file; does not need additional configuration . ... instrument-independent module creating an overview of all (or of a selected number of) extensions in a raw or product file; does not need additional configuration . ...

I. Installation . ... AMPLE package distributive (created with program InstallShield for Microsoft Visual C++) has been downloaded on FTP server of IAA RAS as archive Ample.zip. ... Note: If the window "file download" appears, select Open... switch button, then press OK button. ... The shortcut for AMPLE will be linked with this folder, and auxiliary files will be created here during AMPLE work. ... When running AMPLE all auxiliary and new configuration files are created in the WORK folder. ...

It is now possible to specify multiple log files, each with a fully customizable format. ... Multiple log files are implemented as part of the mod_log_config module which as of Apache 1.2 is the default log module. Multiple log files be created with either the TransferLog or CustomLog directive. These directives can be repeated to create more than one log file (in previous releases, only one logfile could be given per server configuration). ... Syntax: CustomLog filename "format" . ...

The two archives in this directory contain the same image files. They are more than 4 GB in size, and the download time may be hours, even with a fast broadband connection: WASP-12b_example_images.tar.gz 4.3GB WASP-12b_example_images.zip 4.4GB Linux and Mac OS users should select the tar.gz file because it is over the 4GB limit of the usual unzip software. Use these commands to unpack the files in Linux or OSX: tar xvf WASP-12b_example_images.tar.gz or jar xf WASP-12b_example_images.zip

Sending commands to an instrument or other actor is straightforward. ... This script simply takes a few darks. ... If the command fails then the script will terminate. Early termination will not affect this script because executing the command is the last step, but it can be very useful for longer scripts.) If a user cancels the script while the command is executing, the abort command is sent. ... Users are bound to abort your script and they should be able to do so safely and gracefully. ...