[daip] MCUBE file size

Eric Perlman eperlman at fit.edu
Wed Jun 22 15:51:42 EDT 2016


Hi Eric,

On 6/22/16 3:42 PM, Eric Greisen wrote:
> On 06/22/2016 01:32 PM, Eric Perlman wrote:
>> Hi Eric,
>>
>> Thanks - and thanks also for putting up with me on this.
>>
>> Just to reiterate what I'm trying to do, I'm trying to assemble cubes to
>> do an RM analysis in DOFARS ... knowing full well that since there are
>> 128 channels of only 16kHz width in each band (C and L) what I will be
>> able to get will be limited.  This was your recommended path.
>>
>> FQUBE seems to run, with these inputs:
>>  >inp fqube
>> AIPS 1: FQUBE:  Convert FREQ/FREQID image cubes into larger FREQID cube
>> AIPS 1: Adverbs     Values                 Comments
>> AIPS 1: ----------------------------------------------------------------
>> AIPS 1: INNAME     'NGC4845_RM'            Input name(name).
>> AIPS 1: INCLASS    'QCL001'                Input name(class).
>> AIPS 1: INSEQ         1                    Input name(seq. #). 0=>high
>> AIPS 1:                                    First sequence # in the set
>> AIPS 1: INDISK        2                    Input disk drive #. 0=>any
>> AIPS 1: IN2SEQ        2                    Last sequence # in set.
>> AIPS 1: IN3SEQ        0                    Sequence # increment.
>> AIPS 1: OUTNAME    'NGC4845_RM'            Output name(name).
>> AIPS 1: OUTCLASS   ' '                     Output name(class).
>> AIPS 1: OUTSEQ        0                    Output name(seq. #).
>> AIPS 1:                                      0 => highest unique
>> AIPS 1: OUTDISK       2                    Output image disk drive #
>> AIPS 1:                                      0 => highest with space
>> AIPS 1: DOALIGN       1                    Alignment control parm
>> AIPS 1: DOKEEP        1                    > 0 keep all planes including
>> AIPS 1:                                    fully blanked missing CG
>>  >
>>
>> this is the header of the file it produced:
>>
>>  >imh
>> LOGFILE FOR USER 1806 GETTING LARGE: USE PRTMSG AND CLRMSG NOW!
>> AIPS 1: Image=NGC4845   (MA)         Filename=NGC4845_RM  .FQUBE .   1
>> AIPS 1: Telescope=VLBA               Receiver=VLBA
>> AIPS 1: Observer=BP191               User #= 1806
>> AIPS 1: Observ. date=08-OCT-2015     Map date=22-JUN-2016
>> AIPS 1: Minimum=-3.76577675E-03      Maximum= 3.81711102E-03 JY/BEAM
>> AIPS 1: ----------------------------------------------------------------
>> AIPS 1: Type    Pixels   Coord value     at Pixel     Coord incr Rotat
>> AIPS 1: RA---SIN  1024    12 58 01.197     512.00 -0.001000 0.00
>> AIPS 1: DEC--SIN  1024    01 34 32.420     513.00 0.001000 0.00
>> AIPS 1: FQID       256   1.0000000E+00       1.00 1.0000000E+00    0.00
>> AIPS 1: STOKES       1   2.0000000E+00       1.00 1.0000000E+00    0.00
>> AIPS 1: FREQ         1   1.3920000E+09       1.00 2.5000000E+05    0.00
>> AIPS 1: ----------------------------------------------------------------
>> AIPS 1: Coordinate equinox 2000.00
>> AIPS 1: Map type=NORMAL              Number of iterations= 100
>> AIPS 1: Conv size= 0.00926 X 0.00371   Position angle=  -2.83
>> AIPS 1: Rest freq   1392.000         Vel type: OPTICAL wrt YOU
>> AIPS 1: Alt ref. value  0.00000E+00  wrt pixel    0.00
>> 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 CC is 128
>>
>> However, it gave warning messages like this:
>>
>> LOCALH> FQUBE1: FQUBCG: COULD NOT FIND FREQ 1.392000E+09 IN OLD CG TABLE
>> LOCALH> FQUBE1: FQUBCG: COULD NOT FIND FREQ 1.392250E+09 IN OLD CG TABLE
>> LOCALH> FQUBE1: FQUBCG: COULD NOT FIND FREQ 1.392500E+09 IN OLD CG TABLE
>> (256 of these)
>> and, as you can see it did not copy over the CC tables from the 2nd
>> image (as that would have meant 256 of those).
>
> Note it says CG not CC - the CG table contains the restoring Clean 
> beam for each channel and is useful if one wants to do further 
> smoothing. But after CONVL the Clean beam is essentially the same in 
> all channels and so the info is meaningless.  Try a PRTAB on the FQ 
> table of the FQUBE output.  You should see a list of the actual 
> frequencies of each plane.  That is all that FARS and RMFIT will need.
>
> Eric Greisen

Good point.  The FQ table does seem to be reasonable:
        1          1                0.00      250000.00 250000.00          1
        2          2           250000.00      250000.00 250000.00          1
        3          3           500000.00      250000.00 250000.00          1
        4          4           750000.00      250000.00 250000.00          1
(and then skipping to 128)
     128        128         31750000.00      250000.00 250000.00          1
      129        129       3460000000.00      250000.00 250000.00          1
      130        130       3460250000.00      250000.00 250000.00          1
      131        131       3460500000.00      250000.00 250000.00          1
      132        132       3460750000.00      250000.00 250000.00          1

These are the correct channels (25 kHz per channel and 128 channels in 
each band).  So are you saying that FARS and RMFIT will run?

Eric

-- 
Eric S. Perlman, Professor 		eperlman at fit.edu
Physics and Space Sciences Department	Phone:  +1 321 674 7741
Florida Institute of Technology	     	Fax:    +1 321 674 7482
150 West University Boulevard		http://my.fit.edu/~eperlman
Melbourne, FL  32901			http://astro.fit.edu/



More information about the Daip mailing list