[daip] question about aips tasks

Hiroko Shinnaga shinnaga at submm.caltech.edu
Mon Dec 20 20:09:48 EST 2004


Dear Eric Greisen,

   I found one thing in my previous input
parameters in FILLM which might have some
concern.  "NCOUNT" was 0 there.  So, I tried
"NOUNT 4" and issued "go" (I attached new
input parameters).  In my AIPS message
terminal, it reports all four files
were found to read and the process ended
successsfully.  However, the situation still
keeps the same.  VPLOT shows the same plot.
If you have any suggestions which I could
try, could you please let me know?

   Thank you very much for your help.

Hiroko

//////////////////////////////////////////////
 >inp
AIPS 1: FILLM     Task to read a VLA archive tape
AIPS 1: Adverbs     Values                 Comments
AIPS 1: ----------------------------------------------------------------
AIPS 1: INTAPE        1                    Tape drive number
AIPS 1: INFILE     'MYAREA:AS813.NOV02.XP                           '
AIPS 1:                                    Non-blank: disk file name
AIPS 1: NFILES        0                    Number of files to advance
AIPS 1:                                    Also applies to ON-LINE!
AIPS 1: BAND       '    '                  Freq. band (4,P,L,C,X,U,K,Q)
AIPS 1: QUAL         -1                    Source qualifier -1=>all
AIPS 1: CALCODE    '    '                  Calibrator code
AIPS 1: VLAOBS     '      '                VLA obs. pgm. name ('AZ99')
AIPS 1: VLAMODE    '  '                    VLA obs. mode ('  '=any)
AIPS 1: REFDATE    '        '              Reference date. 'yyyymmdd'
AIPS 1: TIMERANG   *all 0                  Timerange selected
AIPS 1: BCHAN         1                    First spectral channel
AIPS 1: ECHAN         0                    Highest spectral channel
AIPS 1: OUTNAME    '            '          Output UV file name (name)
AIPS 1: OUTSEQ        0                    Output UV file name (seq. #)
AIPS 1: OUTDISK       1                    Output UV file disk unit #.
AIPS 1: DOUVCOMP     -1                    1 (T) => compressed data
AIPS 1: DOALL        -1                    1 (T) => write all data.
AIPS 1: DOCONCAT     -1                    1 (T) => append data to old
AIPS 1:                                    files
AIPS 1: NCOUNT        4                    Number of files to read
AIPS 1: DOWEIGHT      1                    Use nominal sensitivity to
AIPS 1:                                    scale weights?
AIPS 1:                                    = 10, use Memo 108 weights
AIPS 1: DOACOR       -1                    Load autocorrelation data?
AIPS 1: CPARM         0           0        User options.
AIPS 1:               0           0        1 => Avg. time (seconds)
AIPS 1:               0           0        2 => bitmap    (see help)
AIPS 1:               0          0.05           = 16 for planets & Sun
AIPS 1:               0           0        3 => Max. OK IF status
AIPS 1:                                         <=3 => 3
AIPS 1:                                    4 => Control dropping of
AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
#
AIPS 1:                                         shadowed data
AIPS 1:                                         < 0 => no shadow check
AIPS 1:                                         0 => 25 m limit
AIPS 1:                                         > 0 => Shadow limit is
AIPS 1:                                               CPARM(4) in meters
AIPS 1:                                    5 = channel code (see HELP)
AIPS 1:                                    6 => Subarray number-see HELP
AIPS 1:                                    7 => FQ entry tolerance (kHz)
AIPS 1:                                         (see HELP)
AIPS 1:                                    8 => CL table time incr. min
AIPS 1:                                    9 => TY table time incr. min
AIPS 1:                                    10=> Calibrator avg. time
AIPS 1: DPARM      *all 0                  Selection by Frequency
AIPS 1:                                    1+2 => A Frequency (Hz)
AIPS 1:                                    3+4 => B Frequency (Hz)
AIPS 1:                                    5+6 => C Frequency (Hz)
AIPS 1:                                    7+8 => D Frequency (Hz)
AIPS 1:                                    9 => tolerance for A&C
AIPS 1:                                    10 => tolerance for B&D
AIPS 1: BPARM        20           1        Opacity and Gain curve
AIPS 1:               0           0        control (see help)
AIPS 1:               0           0           0           0
AIPS 1:               0           0.75
AIPS 1: IN2FILE    '                                                '
AIPS 1:                                    Antenna gains file
/////////////////////////////


Hiroko Shinnaga wrote:
> Dear Eric Greisen,
> 
>   Thank you very much for your kind and prompt
> response to my questions.
> 
>>  > 1. I found a disagreement between LISTR statements
>>  >    and the plot made with VPLOT for a data set.
>>  >    The situation is as follows.  Although LISTR reports
>>  >    data on some specific object were taken during some
>>  >    specific time periods, the plot created by VPLOT is
>>  >    shifted about 15 min from the LISTR statements. Namely,
>>  >    the observing periods has a time lag roughly about 15
>>  >    minutes between LISTR and VPLOT.  I checked the observing
>>  >    script which was run during the period.  Comparing with
>>  >    the script, it seems that LISTR output looks correct
>>  >    and VPLOT looks not correct.  With UVPLOT, the
>>  >    plot of time vs. phase (or amp) agrees with
>>  >    LISTR results.  So, it seems VPLOT creates wrong plot.
>>  >    I tried to specify time using the BPARM option.  However,
>>  >    the results were the same.  Could you let me know
>>  >    possible reasons why this is happening?  Have you
>>  >    seen this problem before?
>>
>>       No and I do not see it when I try right now.  I would need to
>> see the inputs used to VPLOT.  Note that time is BPARM(1)=12 in VPLOT
>> and =11 in UVPLT.  BPARM(1)=11 is Greenwich time but that should
>> differ by an integer number of hours.
> 
> 
> I set time as IAT hours for both UVPLT and VPLOT.
> These should give us the same pattern for UVPLT and
> VPLOT.  But VPLOT gives me a weird pattern.  I
> carefully checked LISTR 'SCAN' output on the data.
> I should get the pattern shown in UVPLT, not like
> VPLOT.  Here I attach the plots in gif.
> 
> 
>>
>>  >  > 2.  Using the same data set, when I set xinc as 3
>>  >     or 2 on vplot, I couldn't see almost any point on many
>>  >     baselines (such as antenna 1, 8, 11, 17, 18,19,
>>  >     etc).  However, when I set xinc as 1, I could see
>>  >     all the data points including baselines of antenna
>>  >     1 etc, which looked missing using xinc = 2 or 3.
>>  >     Could you let me know possible reasons why this is
>>  >     happening?
>>
>>      If XINC=3 then only every 3rd point is considered for plotting.
>> If the number of baselines selected with the adverbs is a multiple of
>> 3 then you should see lots of points for some baselines and virtually
>> none for others.  Editing and other vagueries usually make XINC
>> reasonable but in small data sets you could easily see the effect you
>> are reporting.  Use XINC=1, modern computers are fast enough.
> 
> 
>   Yes, I will use xinc=1, instead of 2 or 3, because
> the computer is fast enough to handle it.
> 
> 
>>  >  > 3.  Above two issues are  happening only on a specific
>>  >      data set. I created this AIPS data file using
>>  >      multiple(four) tape files with FILLM.  For the
>>  >      other data set that I created from one tape file
>>  >      with FILLM, with the same options, I didn't have
>>  >      the above problems.  Do you think these are related?
>>  >      (Please note that both data sets were taken using
>>  >      fast switching.  I don't know if these are related.
>>  >      But just as a info. )
>>  >  >    I would like to appreciate your response soon,
>>  > if possible.  I have my next VLA run this week
>>  > Thursday.  In case the data itself have some problem,
>>  > I need to investigate my script to avoid these issues.
>>
>> Did you run FILLM 4 times and use DBCON or did you run FILLM once with
>> all 4 files read?  The latter may end up with times offset by 5 days.
>> The former could get interesting too if the four files are from very
>> different dates.  Times are kept in single-precision floating days and
>> would get inaccurate if many days were involved.  But UVPLT and VPLOT
>> should see the same times since the data are handed to both of them
>> from the same subroutines.
>>
> 
> The above might be caused by the way that I used FILLM.
> Let me explain more about this.  Followings are
> the input parameters that I used to read the four
> tape files.
> 
> ///////////////////////////////////////
>  >inp
> AIPS 1: FILLM     Task to read a VLA archive tape
> AIPS 1: Adverbs     Values                 Comments
> AIPS 1: ----------------------------------------------------------------
> AIPS 1: INTAPE        1                    Tape drive number
> AIPS 1: INFILE     'MYAREA:AS813.NOV02.XP                           '
> AIPS 1:                                    Non-blank: disk file name
> AIPS 1: NFILES        0                    Number of files to advance
> AIPS 1:                                    Also applies to ON-LINE!
> AIPS 1: BAND       '    '                  Freq. band (4,P,L,C,X,U,K,Q)
> AIPS 1: QUAL         -1                    Source qualifier -1=>all
> AIPS 1: CALCODE    '    '                  Calibrator code
> AIPS 1: VLAOBS     '      '                VLA obs. pgm. name ('AZ99')
> AIPS 1: VLAMODE    '  '                    VLA obs. mode ('  '=any)
> AIPS 1: REFDATE    '        '              Reference date. 'yyyymmdd'
> AIPS 1: TIMERANG   *all 0                  Timerange selected
> AIPS 1: BCHAN         1                    First spectral channel
> AIPS 1: ECHAN         0                    Highest spectral channel
> AIPS 1: OUTNAME    '            '          Output UV file name (name)
> AIPS 1: OUTSEQ        0                    Output UV file name (seq. #)
> AIPS 1: OUTDISK       1                    Output UV file disk unit #.
> AIPS 1: DOUVCOMP     -1                    1 (T) => compressed data
> AIPS 1: DOALL        -1                    1 (T) => write all data.
> AIPS 1: DOCONCAT     -1                    1 (T) => append data to old
> AIPS 1:                                    files
> AIPS 1: NCOUNT        0                    Number of files to read
> AIPS 1: DOWEIGHT      1                    Use nominal sensitivity to
> AIPS 1:                                    scale weights?
> AIPS 1:                                    = 10, use Memo 108 weights
> AIPS 1: DOACOR       -1                    Load autocorrelation data?
> AIPS 1: CPARM         0           0        User options.
> AIPS 1:               0           0        1 => Avg. time (seconds)
> AIPS 1:               0           0        2 => bitmap    (see help)
> AIPS 1:               0          0.05           = 16 for planets & Sun
> AIPS 1:               0           0        3 => Max. OK IF status
> AIPS 1:                                         <=3 => 3
> AIPS 1:                                    4 => Control dropping of
> AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
> #
> AIPS 1:                                         shadowed data
> AIPS 1:                                         < 0 => no shadow check
> AIPS 1:                                         0 => 25 m limit
> AIPS 1:                                         > 0 => Shadow limit is
> AIPS 1:                                               CPARM(4) in meters
> AIPS 1:                                    5 = channel code (see HELP)
> AIPS 1:                                    6 => Subarray number-see HELP
> AIPS 1:                                    7 => FQ entry tolerance (kHz)
> AIPS 1:                                         (see HELP)
> AIPS 1:                                    8 => CL table time incr. min
> AIPS 1:                                    9 => TY table time incr. min
> AIPS 1:                                    10=> Calibrator avg. time
> AIPS 1: DPARM      *all 0                  Selection by Frequency
> AIPS 1:                                    1+2 => A Frequency (Hz)
> AIPS 1:                                    3+4 => B Frequency (Hz)
> AIPS 1:                                    5+6 => C Frequency (Hz)
> AIPS 1:                                    7+8 => D Frequency (Hz)
> AIPS 1:                                    9 => tolerance for A&C
> AIPS 1:                                    10 => tolerance for B&D
> AIPS 1: BPARM        20           1        Opacity and Gain curve
> AIPS 1:               0           0        control (see help)
> AIPS 1:               0           0           0           0
> AIPS 1:               0           0.75
> AIPS 1: IN2FILE    '                                                '
> AIPS 1:                                    Antenna gains file
> /////////////////////////////////////////////////////////////
> 
> Under the directory MYAREA, I have four tape
> files named as follows.
> 
> AS813.NOV02.XP1
> AS813.NOV02.XP2
> AS813.NOV02.XP3
> AS813.NOV02.XP4
> 
> I issued "go" only once to use FILLM.
> I was told that the above parameter setting
> for infile 'MYAREA:AS813.NOV02.XP" would
> work.  Would you think this is not a right
> way to do?
> 
> 
> 
>> So far as I can tell you should have no problem in your data, but I
>> have no idea what VPLOT appears to be doing or why.
> 
> 
> I really hope that would be the case.
> 
> 
> Hope to hear from you.  Thank you very much for
> your help.
> 
> 
> Hiroko
> 
> 
> 
> 
> ------------------------------------------------------------------------
> 
> 
> ------------------------------------------------------------------------
> 


-- 
Hiroko Shinnaga, Staff Scientist    email: shinnaga at submm.calteh.edu
Caltech Submillimeter Observatory   Phone: 808-935-1909
California Institute of Technology  Fax:   808-961-6273
111 Nowelo St., Hilo, HI 96720 USA  http://puuoo.submm.caltech.edu/~hs




More information about the Daip mailing list