[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