... GPI Data Pipeline 1.0 documentation . ... Frequently Asked Questions . ... When trying to start the pipeline, I get the error ?xterm: Can?t execvp idl: No such file or directory? ... Credits for the GPI Pipeline Software Development . ... You can either (1) change your $PATH to include the directory with idl, (2) put a symlink pointing to idl in some directory already in your path, or (3) edit your local copy of the gpi-pipeline script to explicitly set the full path to the idl executable. ...

. Your system administrator may have customised the mail program for you. The system wide default values are in the file /usr/lib/Mail.rc . Check which variables are already set before making changes of your own. If you are in command mode, enter the command: set . If you are composing a mail message, enter the command: ~:set . This displays a list of variables that are currently set, and their values.

README for XFree86 on OS/2 : Adding Variables to CONFIG.SYS . ... ETC . Set to an ETC directory. Normally, this is already set to the ETC directory of the TCP/IP code, such as SET ETC=C:\TCPIP\ETC For Warp 4 and later, this may point to the \MPTN\ directory. ... Normally you will set this variable to the same value as the HOSTNAME variable and simply add a :0.0 after it, such as SET DISPLAY=myhost:0.0 Read the X11 man page on the exact meaning of these postfixes and other options. ...

... This appendix describes how to use the JavaScript console to evaluate expressions and display error messages to the user. ... Displaying Error Messages with the Console JavaScript 1.2 and earlier versions. ... You can specify whether to automatically open the console when a JavaScript error occurs or to display a dialog box for each JavaScript error. ... To open a dialog box each time an error occurs, add the following line to prefs.js : user_pref("javascript.classic.error_alerts", true); . ...

Next: MIDAS And the Up: Monitor and Command Previous: Monitor and Command . ... the MIDAS working directory for internal files and (optionally) private procedures: . ... On a Unix system use the option -m < mid_work > to change the default working directory, and -p or -P to run MIDAS in parallel mode љ when you start MIDAS via the command inmidas (see below). ... In NOPARALLEL mode all intermediate MIDAS files in the MIDAS startup directory are deleted when starting MIDAS via inmidas. ...

... Summary: PmWiki group header. ... Summary:Variables used for uploads/attachments:) . ... This array contains forbidden strings for an uploaded file (case insensitive). ... This variable sets additional unix permissions applied to newly uploaded files, and should be 0 (recommended as of 2013). ... This variable sets unix permissions unconditionally applied to newly uploaded files, for example 0604 . ... Sets the prefix for uploaded files to allow attachments to be organized other than by groups. ...

... This is the MS-DOS general help file. ... Type FASTHELP with no arguments to display the text in this file. ... APPEND Allows programs to open data files in specified directories as if they were in the current directory. ... COPY Copies one or more files to another location. ... FC Compares two files or sets of files, and displays the differences between them. ... PATH Displays or sets a search path for executable files. ... SYS Copies MS-DOS system files and command interpreter to a disk you...

... Display of FITS image extensions and binary tables . SAOtng now can display FITS image extensions, FITS binary tables and raw event files. See Loading an Image for more information. ... Display of compressed FITS and WWW FITS files . SAOtng now can display compressed FITS files by automatically decompressing them on the fly. ... SAOtng now will search for image files in directories specified by the IMAGE_PATH environment variable. ... See the SAOtng XPA List for more information. ...

... Common options . All SAS tasks support the following command line options: . ... If the task uses the ODF Access Layer ( oal ) the following command line option is recognized as well: . ... odf odf . ... odf can be the name of an ODF summary file as created by the task odfingest or merely the name of a directory containing one. ... All tasks may have additional parameters in a parameter file, that can be set on the command line (more information can be found in package param ). param = value . ...

... Documentation for the Python objects defined by the project is divided into separate pages for each package, module, and class. The API documentation also includes two pages containing information about the project as a whole: a trees page, and an index page. ... A description of the package. ... A summary of the classes defined by the package. ... The module contents frame contains a list of every submodule, class, type, exception, function, and variable defined by a module or package. ...

OptInt PmWiki : Pm Wiki / Upload Variables . Security Variables | ... The directory where uploads are to be stored. Defaults to uploads/ in the pmwiki directory, but can be set to any location on the server. ... UploadDirQuota = 100*1024; # limit uploads to 100KiB $UploadDirQuota = 1000*1024; # limit uploads to 1000KiB $UploadDirQuota = 1024*1024; # limit uploads to 1MiB $UploadDirQuota = 25*1024*1024; # limit uploads to 25MiB $UploadDirQuota = 2*1024*1024*1024; # limit uploads to 2GiB . ...

... xntpd is an operating system daemon which sets and maintains the system time-of-day in synchronism with Internet standard time servers. xntpd is a complete implementation of the Network Time Protocol (NTP) version 3, as defined by RFC-1305, but also retains compatibility with version 1 and 2 servers as defined by RFC- 1059 and RFC-1119, respectively. xntpd does all computations in 64-bit fixed point arithmetic and requires no floating point support. ... Specify the name and path of the log file. ...

Next: Adding plot classes Up: Plotting Previous: Plotting Contents . Plot variables are identified by a sequence number in , and are defined in terms of data variables in set_plotdata (and the corresponding function set_ploterr . ... The following additional information needs to be entered for each plot variable. Each plot variable's ID is entered in set_plotlabels for the index label it requires so that it is displayed together with the name in the plots. ...

... Next, the screen displays "Press 0 to align or Mode for Menu." Press "0" if you wish to begin Automatic alignment (or Easy Align, depending on your telescope model), or press Mode if you wish to choose a manual alignment method ("Automatic Alignment" displays, and you can press MODE to go through the menu to find other alignments). ... Note: If you press the "?" key while "Ctr Brightest Star" displays, the alignment star that AutoStar has chosen will display. ... Alignment successful" displays. ...

... Tonight's Sky . ... The Magazine . News . Observing . ... Magazine . ... Star Atlas . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Open cluster NGC 2818, spiral galaxy NGC 2964, and spiral galaxy NGC 2976 . ... Astronomy for Kids . ... variable stars . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

This document explains how to install, configure and run Apache 1.3 under Novell NetWare 5.x and above. ... Apache 1.3 is designed to run on NetWare 5.x and above and is installed by default on all NetWare 6 servers. ... You will need to compile apache and copy the files over to the server manually. ... Follow these steps to install Apache on NetWare from the binary download (assuming you will install to sys:/apache): . ... Copy the MIME.TYPES and magic files to SYS:/APACHE/CONF directory . ...

Since XmCCD uses Motif, the libraries and include files must be available. ... By default it will create a directory xmccd-#.# with the command tar -xvzf xmccd-#.#.tar Set your current working directory to xmccd-#.# cd xmccd-#.# ... For "ls -l" you should see something like this -rwsr-xr-x 1 root root 281883 Mar 10 01:08 xmccd Move xmccd to a directory in your search path such as /usr/local/bin mv xmccd /usr/local/bin xmccd will use ds9 for image display if it is present. ...

... CodingљStyle . ... Plugins . ... Building Plugins . ... dynamic plugins are stand-alone dynamic libraries (separate files with .so extension on Linux, .dll in Windows or .dylib on Mac OS X) that are loaded at run-time (on start-up) by Stellarium. This allows dynamic plugins to be distributed separately from Stellarium. static plugins are linked statically at build-time. ... For the rest of this discussion, I will assume you downloaded the source code in the directory /home/me/builds/stellarium . ...

... Up: FITS-Flexible Image Transport System . ... The FITS List Calculator and Bulk Data Processor (FLC) is an IDL program with a graphical user interface developed for processing large groups of Near Infrared Camera and Multi-Object Spectrometer (NICMOS) test data efficiently. ... Figure 1 shows the data structures used to hold lists and images. ... The IDL structures for images are similar to the structures for lists except that the image headers and image data arrays are kept in the structure. ...

THE 75th NAME-LIST OF VARIABLE STARS. ... The 75th Name-List consists of two tables. ... the literature, taken from positional catalogues, including USNO A1.0/A2.0 and GSC, or determined by the authors); the range of variability (sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol ( means that the star , in minimum light, becomes fainter, than the magnitude indicated); and the system of magnitudes used ( P are photographic ...