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w_fits

FUNCTION
	Main script to invoke the FOT reading program wfotfits
	call into action programs (stage-1) for extracting,
	monitoring and processing SAX-WFC FOTs in order to 
	prepare the data for detecter correlation and X-ray 
	sources detection (stage-2).


USAGE

	w_fits -f prefix [-specifier [argument]] ..... [-specifier [argument]]

        Where a specifier can be a switch or option followed by an argument. 
	Common practice is taking for the FOTID the
	Observation Period number preceded by 'OP' 

	Before being able to use the w_proc at least the
	following shell environment variables must be set:

		WFC_TOP		e.g. /home/xrayman/wfc
		WFC_ETC		e.g. $WFC_TOP/etc
		WFC_BIN		e.g. $WFC_TOP/bin
		path 		e.g. ( $WFC_ETC $WFC_BIN $path )
		
	As in some instances use is made of ftools utilities 
	also the following environment variable must be set
		
		FTOOLDIR	e.g. /home/library/ftools
			
	To store the parameter files In addition a directory in
	your home directory must exist with the following name:
		
		$HOME/pfiles/release
			
	The names of these directories may be site dependent, 
	so when in doubt ask your local ftools manager.
			
	It is advisable to create a single shell source file
	for setting these variables plus others to be used 
	with stage-2 processing.


DESCRIPTION 
	From the recieved FOT data is extracted checked on
	anomalies and copied into FITS formatted files.
	The producing of the files is done by invoking 
	program 'wfotfits' with the proper parameters.
	Checking of required directory structures is performed
	and the user is warned if missing.
	
	The following filetypes are/can be produced of all but 
	the last are in FITS format:
	
	       FOT
		|
		V
	    --------
	    wfotfits 
	    --------
		|
		|--> *__att0.fits [attitude data]
		|--> *__eph0.fits [ephemerides data]
		|--> *__utc0.fits [OBT-UTC table]
		|--> *__obs0.fits [observations table] 
		|--> *w#hit0.fits [IT diagnostic ITHKD000]
		|--> *w#@hi0.fits [instrument housekeeping HKD000]
		|--> *w#@hs0.fits [science housekeeping ENG000]
		|--> *w#@rn0.fits [normal rate data DIR001]
		|--> *w#@rh0.fits [high rate data DIR002]
		|--> *w#@ba0.fits [background analysis data DIR003]
		|--> *w#@dr0.fits [reduced diagnostic data DIR004] 
		|--> *w#@de0.fits [extended diagnostic data DIR005]
		|--> *w#@ib0.fits [packetblocks info]
		|--> *w#@rn0.gti  [GTI file]
		|--> *w#@rh0.gti  [GTI file]
		|--> *w#obs0.txt  (observation times survey text]
		-
		
	where 'w#' denotes the camarea ('w1' or 'w2'), '@' denotes
	the type of observation ('p' for pointing, 's' for slewing)
	and '0.' the level of processing.  This will be reflected
	in keyword 'VERSION' of the
	
	The "EXCONF'(experiment configuration) data is stored in the
	extension header of the instrument housekeeping (*hi0.fits) file
	
	The script allows the insertion or replacement of auxiliary
	files according to te following conventions.  A file can be
	explicitly assigned by using swith '-att' or by pre-setting
	the corresponding environment variable.  
	It is also possible to have a directory searched automatically
	for a file.  This is done by pre-setting environment variable 
	'WFC_FOTREPDIR'.  
	Then for '-f prefix' a files are searched with the name 
	  $WFC_FOTREPDIR/Wprefix_ATT/attitude*.dat or
	  $WFC_FOTREPDIR/Wprefix_EPH/ephemeris*.dat or 
	  $WFC_FOTREPDIR/Wprefix_OBT/obt_utc*.dat
	If found that file will be the replacement file.
	


OPTION SPECIFIERS

    The order of actions or options is not fixed.  An option can be
    either a switch or a keyword followed by one or more arguments.
    At least one of the following actions must be selected: 
 
-h	
	Display a concise help on the available switches and recognized
	environment settings.  It will not show the switches of possible 
	subsequently invoked programs however.

-f [string]
	The argument specifies the FOT identifier.  TFor resulting files
	this will become the prefix of all names.  Only when processing 
	directly from tape with the '-fot' action can this switch be omitted,  
	in which case the FOTID is taken from the FOT directory.  But also
	in this case it will be overruled by giving the -f FOT_ID switch.
	
-t [string]
	Specify (top-)directory where input (link)files are located.
	By default the current directory is taken.  This default
	can be overruled by setting environment variable $WFC_OBS
 	  Only in case of '-fot' action this will be the destination 
	directory where the FOT files from tape will be placed to be 
	used as input for level 0 (-fits) processing.
	It will overrle the value of enveironment variable FOT_TOP.
	
-d [string]
	Force result files under destination top-dir.
	By default this will be the input directory.
	Already existing result files will be overwritten.

-vv [integer]
	Argument value regulates the output verbosity volume.  When 0 a 
	minimal (silent) output will occur.  The default is 1 where it 
	will show the programs that were active and some info on files 
	produced.  A larger value will produce more diagnostic info.
	This switch will be passed on to subsequently invoked scripts.
	
-w1
-w2
	Only process the data of one (-w1 or -w2) camera.  
	(not relevant for '-fot' and -fits' actions)
	
-save
	Force intermediate files to be saved.  By default the 
	lower level files will be discarded.
	
-n  [integer]
-n1 [integer]
-n2 [integer]
	Indicates the number (-n) or number range (-n1 and -n2) 
	of observations to be processed.  By default n1 = 1 and 
	n2 = 999.

-c1 [string]
-c2 [string]
        The name of the input FITS file that contains the 
	coefficients to calculate the physical values of 
	temperatures and voltages from digitally coded 
	analog value.   By default they are $WFC_CAL/wfc1.det
	and $WFC_CAL/wfc1.det respectively.  The defaults can
	be fixed by setting environment variables W_INSCAL1
	and W_INSCAL2 respectively.

-blockio
	Allow writing and reading data files in fast block I/O.  
	This may introduce a non-standerd FITS format that cannot
	be used across different computer systems and will not work 
	with systems using VAX byte order.  Presently by default 
	the blockio option is disabled for OSF1 unix systems and 
	enabled for all other systems like HPUX.

-swap
-noswap
	Specify whether the data is organized according to VAX
	definition and bytes of words and double-words must be
	swapped.  This will be normally the case if FOT's were
	produced by the Science Data Centre.
	Presently by default the swap option is disabled for OSF1 
	unix systems and enabled for all other systems like HPUX.

-att [string]
-eph [string]
-obt [string]
	Specify the name of an alternative file containing attitude,
	ephemeris or OBT_UTC data.  It will replace the one that is in 
	the FOT.  If not present in the FOT it will be inserted at the
	porper place in the original FOT.
	  It is possible to specify the alternative file by setting
	the respective environment variables W_ATTFILE, W_EPHFILE,
	or W_OBTFILE.

-frt [string]
	Argument specifies root-name of disk created fotfiles 
	By default takes the specified FOTID plus '_'
	NOT RECOMMENDED TO CHANGE THE DEFAULT

-fxt [string]	
	Argument specifies extension of disk located fotfiles (default .fot)
	NOT RECOMMENDED TO CHANGE THE DEFAULT


RECOGNIZED ENVIRONMENT VARIABLES
  
    In addition default values for switches and installed settings 
    can be overruled by the following  shell environment variables.

	WFC_TOP The top directory of the WFC software distribution 
		No default as it is site dependent
 
	WFC_ETC Place where scripts and general selection files are located
		if not present default to $WFC_TOP/etc

	WFC_BIN Place where the program executable binaries are located 
		if not present default to $WFC_TOP/bin

	WFC_CAL Place where calibration and instrument definition files.
		if not present default to $WFC_TOP/cal
		(see also switches '-c1' and '-c2')
		
	WFC_FITSORIG  String to be used for the ORIGIN keyword in produced
		Fitsfiles (default: `hostname` )
		
	FOT_TOP	The directory where the FOT files are resided.
		This is the input directory for all actions except for  
		the '-fot' option where it will be the directory in 
		which the FOT files are loaded. (default: `pwd` )
  
	W_INSCAL1
		if not present default to $WFC_CAL/wfc1.det
		(see also switch '-c1')
		
	W_INSCAL2
		if not present default to $WFC_CAL/wfc2.det 
		(see also switch '-c2')
		
	W_EPHFILE
		if not present default to "-"
		(see also switch '-eph')
		
	W_ATTFILE
		if not present default to "-"
		(see also switch '-att')
		
	W_OBTFILE
		if not present default to "-"
		(see also switch '-obt')

	
EXAMPLES:

Process a FOT from tape completely with standard options, put resulting 
files in the current directory and save the output in a logfile 

  >  w_fits -fot -f OP1234 -t FOTDIR > logfile

To re-process all observation of camera 2 only and store the results 
in a different destination directory

  >  w_proc -f OP1234 -w2 -clean -t FOTDIR -d /DESTDIR



NOTES

    - For narmal use it is recommended to invoke this script 
	by use of script w_proc

    - The destination directory will be created if not present.
    
    - In case a FOT resides on disk its filenaming is not of the 
	form 'prefix__nnnn.fot' a renaming or namelink is needed
	by script w_vaxlink available in $WFC_ETC.

    - The detector calibration files are created during
	the installment of Stage-2 software package.

    - Unspecified options exist fot handling cases of incomplete
	or corrupt FOTs.  They are not advised for use in general
	operations.
	  

SEE ALSO
	w_vaxlink, w_stageI, w_proc, wfotfits



Mark Savenije
Sat Jan 18 15:04:49 MET 1997