[daip] Help in imagr
Eric Greisen
egreisen at nrao.edu
Tue Dec 9 13:05:17 EST 2008
Oozeer Nadeem wrote:
> Hi again,
>
> imheader
> ***************
>
> AIPS 1: Image=1514-241 (UV) Filename=1514-241 .SPLAT . 1
> AIPS 1: Telescope=GMRT Receiver=GMRT
> AIPS 1: Observer=CRS User #= 121
> AIPS 1: Observ. date=02-AUG-2002 Map date=05-DEC-2008
> AIPS 1: # visibilities 14532 Sort order TB
> AIPS 1: Rand axes: UU-L-SIN VV-L-SIN WW-L-SIN BASELINE TIME1
> AIPS 1: WEIGHT SCALE
> AIPS 1: ----------------------------------------------------------------
> AIPS 1: Type Pixels Coord value at Pixel Coord incr Rotat
> AIPS 1: COMPLEX 1 1.0000000E+00 1.00 1.0000000E+00 0.00
> AIPS 1: STOKES 1 -1.0000000E+00 1.00 -1.0000000E+00 0.00
> AIPS 1: FREQ 110 6.1400000E+08 1.00 -6.2500000E+04 0.00
> AIPS 1: IF 1 1.0000000E+00 1.00 1.0000000E+00 0.00
> AIPS 1: RA 1 15 17 41.995 1.00 3600.000 0.00
> AIPS 1: DEC 1 -24 22 17.793 1.00 3600.000 0.00
> AIPS 1: ----------------------------------------------------------------
> AIPS 1: Coordinate equinox 2000.00
> AIPS 1: Rest freq 0.000 Vel type: RADIO wrt LSR
> AIPS 1: Alt ref. value 0.00000E+00 wrt pixel 1.00
> AIPS 1: Maximum version number of extension files of type FQ is 1
> AIPS 1: Maximum version number of extension files of type HI is 1
> AIPS 1: Maximum version number of extension files of type AN is 1
>
You do realize I hope that the way you are running IMAGR will produce an
image CUBE with 110 spectral channels. Thus 110 separate Cleans must
happen. When you tell IMAGR to stop Cleaning it stops that channel and
goes on to the next. That will take a very long time. If these are not
observations of a spectral line, then you should set BCHAN and ECHAN to
encompass only the good channels (the outermost will not be good after
bandpass correction), then set NCHAV=(ECHAN-BCHAN+1) so that a single
image is made from the NCHAV channels gridded in the proper place for
each channel in the UV plane.
Eric Greisen
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