[daip] AIPS - Help
Eric Greisen
egreisen at nrao.edu
Sat Oct 1 16:58:06 EDT 2005
Murad Hamidouche writes:
> Yeah it is a multi-source, I tried 'CLIPM' it worked now but I had to run
> it a couple times to flag all the data I wanted, i.e. > 2 Jy (so I went up
> to FG 5).
Good - be sure to specify FLAGVER correctly to get the highest.
>
> > What is the image? IMAGR would make an ra-dec image on disk and an
> > image of the dirty beam as well. Then you run KNTR to make a plot
> > file and LWPLA to make a POstScript file. These are all explained in
> > Chapter 6 of the CookBook.
> >
> 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
> AIPS 1: Maximum version number of extension files of type NX is 1
> AIPS 1: Maximum version number of extension files of type SU is 1
> AIPS 1: Maximum version number of extension files of type FQ is 1
> AIPS 1: Maximum version number of extension files of type CL is 4
> AIPS 1: Maximum version number of extension files of type TY is 1
> AIPS 1: Maximum version number of extension files of type WX is 1
> AIPS 1: Maximum version number of extension files of type OF is 1
> AIPS 1: Maximum version number of extension files of type FG is 5
> AIPS 1: Maximum version number of extension files of type SN is 2
> AIPS 1: Keyword = 'CORRMODE' value = ' '
> AIPS 1: Keyword = 'VLAIFS ' value = 'ABCD '
>
>
> I applied 'SPLIT' to make a single source, the 'SPLIT' run
> correctly but the header of the output looks weird to me there're some
> tables missing, but didn't get any warning or error message. This its
> header looks:
>
> AIPS 1: Image=04588+29 (UV) Filename=04588+29506 .SPLIT . 1
> AIPS 1: Telescope=VLA Receiver=VLA
> AIPS 1: Observer=AH871 User #= 2
> AIPS 1: Observ. date=17-APR-2005 Map date=29-SEP-2005
> AIPS 1: # visibilities 829162 Sort order TB
> AIPS 1: Rand axes: UU-L-SIN VV-L-SIN WW-L-SIN BASELINE TIME1
> AIPS 1: ----------------------------------------------------------------
> AIPS 1: Type Pixels Coord value at Pixel Coord incr Rotat
> AIPS 1: COMPLEX 3 1.0000000E+00 1.00 1.0000000E+00 0.00
> AIPS 1: STOKES 4 -1.0000000E+00 1.00 -1.0000000E+00 0.00
> AIPS 1: FREQ 1 4.3314900E+10 1.00 5.0000000E+07 0.00
> AIPS 1: IF 2 1.0000000E+00 1.00 1.0000000E+00 0.00
> AIPS 1: RA 1 04 58 46.266 1.00 3600.000 0.00
> AIPS 1: DEC 1 29 50 36.999 1.00 3600.000 0.00
> AIPS 1: ----------------------------------------------------------------
> AIPS 1: Coordinate equinox 2000.00
> AIPS 1: Rest freq 0.000 Vel type: OPTICAL wrt YOU
> 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
> AIPS 1: Maximum version number of extension files of type WX is 1
> AIPS 1: Maximum version number of extension files of type OF is 1
The FG CL SN tables and others have now been applied and so they are
deleted. This looks fine to me.
> And when I try IMAGR on this single-source file it doesn't work ?
What STOKES value do you use? The above should be just fine.
Eric Greisen
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