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1. http://www.eso.org/~qc/dfos/ABbuilder.txt
NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~qc/dfos/ABbuilder.txt -- 8.0 Кб -- 17.02.2006
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2. The File Life Cycle
The File System . This section describes how you can create new files, copy existing files, and delete obsolete files. ... RENAME to change the name of a file. ... Files can be created in several ways: text can be entered from the keyboard via the CREATE command, an editor can create a file, as can a running program, and files can be copied from other directories. ... To delete obsolete files, use the DELETE command followed by a file name or file name template (wildcards). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/system-docs/vms-guide/html/VUG_22.html -- 9.0 Кб -- 01.11.1995
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3. How to create a new tool in CASA Bojan Nikolic web pages (r. 329)
... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/sweng/casanewtool.html -- 19.7 Кб -- 04.04.2016
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4. Recreating Einstein Level One Processing Exposure Masks and Background Maps in
... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/vanstoned.html -- 11.6 Кб -- 03.11.2000
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5. XMM-Newton SAS: Watchout Page
... Due to a change of the structure of the RGS event lists and RGS source list files since SAS 5.1, it is necessary to convert products that where generated with SAS 5.0 to the format required by SAS 5.1 tasks, mainly rgsrmfgen . ... sourceset=PppppppppppRiSeeeSRCLI_0000.FIT Users are reminded that spectra can be extracted only for sources, corresponding to rows in the SCRLIST extension of the source list file which have PROCESS=T . In case of doubt, inspection of the source list file is recommended. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/watchout/5.3/rgs_backward.shtml -- 6.3 Кб -- 22.12.2007
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6. correlator:geodetic [ATNF VLBI Wiki]
... You are here: start €Ё correlator €Ё geodetic . ... correlator:geodetic . ... fourfit . aedit . Creating the files required by aedit . Running aedit . ... The data is required to be submitted in a particular format. ... This contains the geodetic environment variables: export HOPS_STATION_CODE=/nfs/apps/vlbi/lba_locations/hops_station_code.txt export DEF_CONTROL=/nfs/apps/vlbi/lba_locations/fourfit_control.txt export PATH=${PATH}:/nfs/apps/vlbi/hops/x86_64-3.8/bin export HOPS_QUIET='SHH' . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/vlbi/dokuwiki/doku.php/correlator/geodetic -- 16.2 Кб -- 10.04.2016
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7. Creation of Sky Correction Frames
Next: Illumination Corrected Flat Up: Additional Processing Previous: Sky Illumination Corrections . For creation of one or more sky illumination correction frames the command ( SKYCOR/CCD ) is available. ... After this calibration step, the command will smooth the reduced sky frame(s) to create the final sky illumination frame(s). ... After the illumination frame has been created, one can multiply the original flat field by the illumination frame, resulting in an adjusted flat field. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node58.html -- 5.9 Кб -- 23.02.1996
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