rv2fits - Convert from an RV format to an ACIS level 1 format.
rv2fits --ccdid integer --input rvfilename --ouput level1fitsfilename
[ --date-end end_date_of_observation (default value is today's date) ] [ --date-obs begin_date_of_observation (default value is today's date) ] [ --detname | -D detector_name (the default is acis) ] [ --filter | -f the_filter_used (the default value is NONE) ] [ --grating | -g the_grating_used (the default value is NONE) ] [ --help | -h ] [ --mission | -m the_name_of_the_mission (the default value is CHANDRA) ] [ --readmode | -r FITS_READMODE_keyword (the default value is TIMED) ] [ --splitthreshold | -s the_split_threshold (the default value is 13) ] [ --src_spec FITS_SRC_SPEC_keyword (the default value is MONO ) ] [ --telescope | -t name_of_the_telescope (the default value is CHANDRA) ] [ --time-end end_time_of_observation (the default value is 12:59:59) ] [ --time-obs begin_time_of_observation (the default value is 00:00:01) ] [ --usage | -u ] [ --version | -v ]
The program converts an RV format to an ACIS FITS level 1 format.
Options may be abbreviated. Options which take values may be separated from their values either by white space.
The options are :
rv2fits --ccdid 2 --input foo.rv --output foo.fits
rv2fits --date-end 2002-05-21 --ccdid 2 --input foo.rv --output foo.fits
rv2fits --dateobs 2002-05-21 --ccdid 2 --input foo.rv --output foo.fits
rv2fits --filter junk --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits -f junk --ccdid 2 --input foo.rv --output foo.fits
rv2fits --grating junk --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits -g junk --ccdid 2 --input foo.rv --output foo.fits
rv2fits --help
or
rv2fits -h
rv2fits --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits --ccdid 2 -i foo.rv -o foo.fits
rv2fits --mission axaf --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits -m axaf --ccdid 2 -i foo.rv -o foo.fits
rv2fits --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits --ccdid 2 -i foo.rv -o foo.fits
rv2fits --readmode NOTTIMED --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits -r NOTTIMED --ccdid 2 -i foo.rv -o foo.fits
rv2fits --splitthreshold 14 --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits -s 14 --ccdid 2 --input foo.rv --output foo.fits
rv2fits --src_spec QUADRAPHONIC --ccdid 2 --input foo.rv --output foo.fits
rv2fits --telescope axaf --ccdid 2 --input foo.rv --output foo.fits
or
rv2fits -t axaf --ccdid 2 -i foo.rv -o foo.fits
rv2fits --time-end 12:00:00 --ccdid 2 --input foo.rv --output foo.fits
rv2fits --timeobs 1:00:00 --ccdid 2 --input foo.rv --output foo.fits
rv2fits --usage
For example:
rv2fits --version
or
rv2fits -v