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http://xmm.vilspa.esa.es/sas/7.0.0/doc/evlistcomb/node3.html.

1. Description
... This is done by taking in all input files the extension whose name is specified by the maintable parameter (called 'merged extension' in what follows) and merging the columns into a single output extension of the same name. ... Its contents is taken from the CCDID keyword (and QUADRANT for EPIC PN). ... To propagate other column specific keywords, they must be specified manually via the extensionchecks , mainattributes , maxattributes and minattributes parameters (see above). ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/evlistcomb/node3.html -- 10.7 Кб -- 09.07.2007
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2. Loading the Telescope and Instrument Specifications
... For reducing data from ESO instrumentation it is assumed that the FITS headers conform the standards set by the document ``ESO Archive, Data Interface Requirements''. ... As an example, in the ESO case the exposure type is stored in the ESO hierarchical FITS keyword `HIERARCH ESO GEN EXPO TYPE'. ... To fill the CCD keywords with the telescope and instrument setup parameters, like name of the telescope, CCD used, read-out noise, frame size, etc. the command LOAD/CCD can be used. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node39.html -- 5.6 Кб -- 23.02.1996
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3. 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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4. Parameters Specific to the VLA
... This section gives a brief description of each of the parameters available to SCHED that are specifically for VLA observations or are especially useful for VLA observations. ... Should be provided for non-VLBI observations. ... This used to be required in order to obtain calibration data for the VLBI observations. ... FREQ: and DOPPLER Warning -- these parameters cannot be used for non-VLBI observations at the VLA since they are only used to adjust the baseband converter frequencies. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Parameters_Specific_VLA.html -- 11.8 Кб -- 10.04.2016
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