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CCG_FLX3x - Combines data lines using the integrated value

Description:
This routine accepts an array consisting of a series of (vectorised) lines of data. It forms the sum of the data values multiplied by its pixel width lines are then summed, i.e a flux. The output integrated values are returned in the array RESULT.

Invocation:
CALL CCG_FLX3x( NPIX, NLINES, STACK, WIDTHS, MINPIX, RESULT, NCON, NBAD, STATUS )

Arguments:

NPIX = INTEGER (Given)
The number of pixels in a line of data.
NLINES = INTEGER (Given)
The number of lines of data in the stack.
STACK( NPIX, NLINES ) = ? (Given)
The array of lines which are to be combined into a single line.
WIDTHS( NPIX, NLINES ) = ? (Given)
The pixel widths in world co-ordinates.
MINPIX = INTEGER (Given)
The minimum number of pixels required to contribute to an output pixel.
RESULT( NPIX ) = ? (Returned)
The output line of data.
NCON( NLINES ) = DOUBLE PRECISION (Returned)
The actual number of contributing pixels from each input line to the output line.
NBAD = INTEGER (Returned)
The number of bad values in the output array created while forming the statistics. It excludes those bad values whose corresponding values along the collapse axis are all bad.
STATUS = INTEGER (Given and Returned)
The global status.

Notes:



next up previous 278
Next: CCG_FM1x - Combines data lines using a fast median
Up: Routine Descriptions
Previous: CCG_FLX1x - Combines data lines using the integrated value

KAPLIBS -- Internal subroutines used within the KAPPA package.
Starlink User Note 238
D.S. Berry
Malcolm J. Currie
9th March 2009
E-mail:ussc@star.rl.ac.uk

Copyright © 2010 Science and Technology Facilities Council