mpi_kmeans(1) [debian man page]

MPI_KMEANS(1)						      General Commands Manual						     MPI_KMEANS(1)

NAME

       mpi_kmeans - K-Means clustering tool

SYNOPSIS

       mpi_kmeans [options]

DESCRIPTION

       mpi_kmeans  is a program that uses k-means clustering to produce a list of cluster centers. The resulting data can be used by mpi_assign(1)
       to assign points to those cluster centers.

OPTIONS

       A summary of options is included below.

   Generic Options:
       --help Produce help message

   Input/Output Options:
       --data file
	      Training file, one datum per line (default: "data.txt")

       --output file
	      Output file, one cluster center per line (default: "output.txt")

   K-Means Options:
       --k num
	      Number of clusters to generate (default: 100)

       --restarts num
	      Number of k-means restarts (default: 0 = single run)

       --maxiter num
	      Maximum number of k-means iterations (default: 0 = infinity)

EXAMPLES

	      mpi_kmeans --k 2 --data example.txt --output clusters.txt

SEE ALSO

       mpi_assign(1)

AUTHOR

       mpi_kmeans was written by Peter Gehler <peter.gehler@tuebingen.mpg.de>.

       This manual page was written by Christian Kastner <debian@kvr.at>, for the Debian project (and may be used by others).

								  April 11, 2011						     MPI_KMEANS(1)

WCSREMAP(1)							   User Commands						       WCSREMAP(1)

NAME

       wcsremap - AME

SYNOPSIS

       remap [-vf][-a rot][[-b][-j] ra dec][-i bits][-l num] file1.fit file2.fit ... filen.fit

DESCRIPTION

       Remap FITS or IRAF images into single FITS image using WCS

	      or  :  remap  [-vf][-a  rot][[-b][-j] ra dec][-i bits][-l num] @filelist -a: Output rotation angle in degrees (default 0) -b ra dec:
	      Output center in B1950 (FK4) RA and Dec -e long lat: Output center in ecliptic longitude and latitude -f file:  Use  WCS	from  this
	      file as output WCS -g long lat: Output center in galactic longitude and latitude -i num: Number of bits per output pixel (default is
	      input) -j ra dec: center in J2000 (FK5) RA and Dec -l num: Log every num rows of output image -m mode:  c  closest  pixel  (more	to
	      come)  -n  num:  integer	pixel  value  for blank pixel -o name: Name for output image -p secpix: Output plate scale in arcsec/pixel
	      (default =input) -s: Set BZERO and BSCALE in output file from input file -t: Number of samples per linear output	pixel  -u:  Delete
	      distortion  keywords from output file -v: Verbose -w type: Output WCS type (input is default) -x x y: Output image reference X and Y
	      coordinates (default is center) -y nx ny: Output image dimensions (default is first input image)

wcsremap 3.8.4							     June 2012							       WCSREMAP(1)