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SC2FILTERMAP
- Filter a 2-d map
- Description:
- This routine takes the FFT of a 2D map, applies a Fourier-space filter,
and then transforms back to real-space before writing out. Currently
the only available filter is a whitening filter which is measured
using a supplied reference image.
- Parameters:
-
-
FILT_EDGEHIGH = _REAL (Write)
-
High-pass filter frequency (1/arcsec)
-
FILT_EDGELOW = _REAL (Write)
-
Low-pass filter frequency (1/arcsec)
-
IN = NDF (Read)
-
Input files to be transformed.
-
MSG_FILTER = _CHAR (Read)
-
Control the verbosity of the application. Values can be
NONE (no messages), QUIET (minimal messages), NORMAL,
VERBOSE, DEBUG or ALL. [NORMAL]
-
OUT = NDF (Write)
-
Output transformed files.
-
OUTFILTER = NDF (Write)
-
Optional NDF for the filter.
-
WHITEN = _LOGICAL (Read)
-
If selected, measure azimuthally-averaged angular power
spectrum in WHITEREFMAP, fit a model A/F
B
W, and apply
its complement to the FFT of the data (normalized to
W). AZAVSPEC is set implicitly. [FALSE]
-
WHITEREFMAP = NDF (Read)
-
Reference map in which to measure whitening filter. [FALSE]
-
ZEROBAD = _LOGICAL (Read)
-
Zero any bad values in the data before taking FFT. [TRUE]
- Notes:
- Transforming data loses the VARIANCE and QUALITY components.
-
Related Applications
- SMURF: SC2MAPFFT
Next: SC2MAPFFT - Fourier Transform 2D maps
Up: Specifications of SMURF Applications
Previous: SC2FFT - Fourier Transform SCUBA-2 time-series data
SMURF -- the Sub-Millimetre User Reduction Facility
Starlink User Note 258
Edward Chapin, Andrew G. Gibb, Tim Jenness, David S. Berry, Douglas Scott & Remo Tilanus
14th February 2013
E-mail:starlink@jiscmail.ac.uk
Copyright © 2012 University of British Columbia \& the Science \& Technology Facilities Council