To run a process in the background as a job and carry on working add an (ampersand) at the end of the command line. ... The shell forks a child process to run the command and displays the job number ( [ n ] ) and the PID (Process IDentifier) number. ... If the command is likely to produce error messages you will need to redirect standard error. ... Do not run an interactive command that requires you to type something at the terminal as a background job. ... You will then have to kill its process . ...

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• Managing background jobs

Next: Order Extraction Up: Background Definition Previous: Background estimate by . ... The sky background component can be measured in spectra taken with an extended slit using the two commands DEFINE/SKY and EXTRACT/SKY . ... The command EXTRACT/ECHELLE performs an average extraction of the sky background using these offsets, optionally fiters for cosmics, and provides an extracted spectrum in a format similar to the one resulting from EXTRACT/ECHELLE . ...

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• Background estimate by filtering
• Background Correction
• Backgrounds

... Use the ROSAT broad band background which is a array file at 1/30 the *.qp file resolution, and contains data from PI bins 7-240. input files: xdata$rp110590.qp; xdata$rp110590_bk1.imh . ... xr> ximages xi> imcalc input file ('-' for STDIN) or imcalc commands: - # Interactive mode IMC) IMC) rp90_a.imh = xdata$rp110590.qp[bl=30,pi=7:240] - xdata$rp110590_bkl.imh # Select same size and channels as the background map # and subtract the background IMC) quit # To exit the interactive mode and imcalc . ...

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• Setting the CDE Backdrop - shell script
• Multi-Rsh parallelized rsh program
• The AstroStat Slog background

... The photometry is computed by aperture photometry (phototype=0) with an aperture of 6 image pixels (aperturer=6), an inner background annulus radius of 8 image pixels (innera=8) and an outer background annulus radius of 13 image pixels (outera=13). omphotom imageset=P0123920101OMS006IMAGE_1000.FIT backgroundimageset=P0123920101OMS006IMAGE_1000.FIT oldsrclistset=P0123920101OMS006SWSRLI1000.FIT newsrclistset=test.fits sourceno=1 phototype=1 aperturer=6.0 background=10.0 . ...

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• Extraction and correction of an X-ray light curve for a point-like source
• How to extract MOS spectra of a point-like source and associated matrices
• Extraction of a X-ray light curve for a point-like source

... Commands can be executed even when you are not physically at a terminal, or even logged on the system. ... Because you may not necessarily be on the system when the batch job is executed, the system relies on the command procedure for any information needed to complete the task. ... Since a batch job logs in under your username, your LOGIN.COM file will be executed before the batch command procedure (see "Defining Your Environment" on page 35 for information about setting up your LOGIN.COM file). ...

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• Remote display
• Dark Backgrounds
• Thermal/Sky Backgrounds GPI Data Pipeline 1.0 documentation

Home - News - Download - Documentation - Search - FTP . About NEdit . ... Macros . ... Back ] . ... Add the following to your .nedit file, after the nedit.shellCommands: \ line: RCS>checkout::o:DL: chmod a-w %; co % RCS>checkout/lock:Shift+Ctrl+L:l:DL: co -l % RCS>checkin:Shift+Ctrl+I:i:DSL: xterm -e ci -u % RCS>unlock::u:D: rcs -u % RCS>rcsinfo::r:D: rcsinfo RCS>rcsdiff::d:W: rcsdiff % The rcsinfo program is not part of RCS, but is a Perl script which duplicates the functionality of sccs info . ...

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• Running UNIX Commands from C
• From Power Up To Bash Prompt: Commands
• Sending Signals - kill()

... To aid description, line numbers are given on the left side of each line (these line numbers are not part of the shell script ). 1: #!/bin/csh 2: 3: # Delete any datasets called multi.uv . 4: 5: rm -rf multi.uv 6: 7: fits in= MULTI.UV op=uvin out= multi.uv 8: 9: foreach srcnam ( 1934-638 0823-500 vela ) 10: uvaver vis = multi.uv select=source(${ srcnam }) out=${ srcnam }.uv 11: end 12: 13: mfcal Line 1: C-shell scripts must always start with the rather cryptic #!/bin/csh . ...

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• Host Command-Line Interface
• Pulsar Group PmWiki/Backup and Restore
• SM - General Index

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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• The repainted Farnham dome with the AITC in the background

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : resources hard limits . Keywords: getrlimit setrlimit limit ulimit hard resource limits . ... As for soft/hard limits, ulimit -S vs. ulimit -H ought to do that. Incidentally, if you specify neither, both should get changed at the same time. csh is an excemption; here you need to use limit -h for hard limits. ...

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• HwB: SCSI Information Connector (Offline)
• Appunti Linux: Processi e shell
• SDSSmosaic

Next: The root filesystem Up: Overview of the Directory Previous: Overview of the Directory . This chapter is loosely based on the Linux filesystem standard, FSSTND, version 1.2 (see the bibliography, [ Qui95 ]), which attempts to set a standard for how the directory tree in a Linux system is organized. ... This chapter does not explain all files in detail. ... The major parts are the root, /usr   , /var   , and /home   filesystems (see figure 2.1 ). ... Figure 2.1: Parts of a Unix directory tree. ...

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• Index
• Contents
• HISTORICAL BACKGROUND

... View/Edit: Fix reading text from files with a code page that doesn't have a valid character for all 256 values, especially 1252 which has a few gaps. Make more archiver command work correctly by using shell escapes and path separators in the right direction. Editor search/replace: - Fix a memory leak - Improve efficiency when replacing text in very long lines. ... Support Ctrl-Shift-F3 as alternate viewer to be consistent with Ctrl-Shift-F4 as alternate editor. ...

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• http://crydee.sai.msu.ru/ftproot/pub/comp/os/linux/slackware-2.3/SLAKWARE/AP4/DISKAP4
• Image: Trees in the Vatican. San Pietro is on the background.
• Image: We're getting closer; Mt. Athos is at the background. It is about 2000

Tiled backgrounds for Netscape and Internet Explorer are on everybody's minds. ... Before you even get started on this project, you should make a duplicate of the original file. You'll want to have the original *and* the copy open at the same time. First we're going to offset the duplicate image using the "offset" filter. ... Make sure to select the 'wrap around' option. ... The image now has an ugly seam criss-crossing in the middle, but the edges will match perfectly. ...

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• Hands-on; Those Little Inset Bars
• Hands On; Dropshadows
• CoolType - Lightning

... Um den Editor ohne eine Datei zu starten, EINGABETASTE drБcken. prompt = Zu Фffnende Datei? parameter = %1 } shortcut = ALT+E shortcutcode = 2066 } program = { shortcut = ALT+G shortcutcode = 2082 command = c:\tools\globe\pcglobe title = Globe pause = disabled } program = { shortcut = ALT+V shortcutcode = 2095 command = c:\tools\virus\scan %9 title = Virus pause = enabled dialog = { ...

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• http://www.naic.edu/~astro/School/Talks/handson_gbt2.pdf
• http://www.naic.edu/~astro/School/Talks/large_pdf/handson_gbt2_2.pdf
• CIMA Command File Observing

... Flux density at 1 GHz (/Jy): 19 . ... Notes: This is the remnant of the SN of AD 1006. ... Optical: Filaments to the NW, with broad H component. ... Point sources: The background Schweizer Middleditch star is near the middle of the remnant. ... van den Bergh 1976, ApJ, 208, L17. Optical observations. ADS . ... X-ray spectroscopy. ... Schweizer & Middleditch 1980, ApJ, 241, 1039. ... Optical spectroscopy of the Schweizer Middleditch star. ... Optical spectroscopy. ... 2013, A&A, 552, A9. ...

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• OptInt PmWiki : PmWiki / Backup and Restore
• Astrophysics Group Cosmic Microwave Background (CMB)
• Martin Krause - Publications

Next: NOVIDAS and UVPROC II-Data Archive and Reduction System for Nobeyama Millimeter Array . ... The RATAN-600 radio telescope allows us to carry out simultaneous multi-frequency observations using wide-band radiometers. ... Using these features a flexible astronomical data processing system (FADPS), operating on different UNIX platforms, was created. ... FADPS commands may be executed directly in UNIX, in scripts, or using a special shell for our data processing system in the X-Window system. ...

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• Recreating Einstein Level One Processing Exposure Masks and Background Maps in
• The Future of Data Reduction at UKIRT
• Using XML and Java for Astronomical Instrument Control

National Aeronautics and Space Administration . ... Frank Borman . ... A romance with airplanes that began when he was 15 years old, took Frank Borman to the Air Force and then to NASA. ... Frank Borman retired from the air Force in 1970, but is well remembered as a part of this nation's history, a pioneer in the exploration of space and a veteran of both the Gemini 7, 1965 Space Orbital Rendezvous with Gemini 6 and the first manned lunar orbital mission, Apollo 8, in 1968. ...

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• as15-85-11514
• Astronaut Bio: James A. Lovell
• as15-88-11863

... FRAMES NO FRAMES All Classes . ... Classes in ij.plugin.filter that implement ExtendedPlugInFilter . ... Implements ImageJ's Subtract Background command. class . ... This plugin implements the Euclidean Distance Map (EDM), Watershed, Ultimate Eroded Points and Voronoi commands in the Process/Binary submenu. class . ... This plugin implements ImageJ's Process/Math submenu. class . ... This plugin implements the Mean, Minimum, Maximum, Variance, Median, Remove Outliers and Despeckle commands. class . ...

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• ij (ImageJ API)
• BackgroundSubtracter (ImageJ API)
• ScaleBar (ImageJ API)

.

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• Infall and Omega
• The Creation of Helium
• Astronomy HyperText Book

Next: Gravitational Wave Background from Previous: Galactic Gravitational Wave Background . ... It is intuitively clear that at frequencies above the critical ones for our Galaxy, one will detect rare bright jerks produced by coalescing white dwarfs ? (at a rate of 1 per 100 year) and NS (at a rate of 1 per - year) in our Galaxy, against a background of the extragalactic stochastic GW. ... Firstly we consider GWB from close individual galaxies, and then will discuss overall extragalactic GWB. ...

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• Transparency of the Stochastic Background
• Galactic Gravitational Wave Background
• Gravitational wave background from nearby galaxies

Next: Introduction Up: Optical Interferometer Script Data Previous: Observing list preparation Contents . ... About CHAMELEON . Data and auxilliary files . ... Open the data file . Read configuration information, create tables, and load data . ... Astrometry . ... Basic widget procedures . Open a data file . Access a data file . Browse through an HDS file . Load configuration, tables, and logs . Load point data . Load scan data . ... Loading data . ... A CCESS B ROWSE . ...

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• Reduce the background data
• ESO - Thesis Topic: Foreground emission and Cosmic Microwave background
• utilities package