[daip] Flux calibrator model problems with U-band VLA-only observations?

Amy Mioduszewski amiodusz at nrao.edu
Mon May 19 12:06:38 EDT 2008


Those look O.K..  I think I am actually going to have to look at your data. 
Could you put it somewhere I can ftp it?

Thanks!

Amy

Jeff Mangum wrote:
> Here you go...
> 
> -- Jeff
> 
>  >inp calib
> AIPS 1: CALIB:  Task to determine calibration for data.
> AIPS 1: Adverbs     Values                 Comments
> AIPS 1: ----------------------------------------------------------------
> AIPS 1:                                    Input uv data.
> AIPS 1: INNAME     '20080223'                 UV file name (name)
> AIPS 1: INCLASS    'CH 0'                     UV file name (class)
> AIPS 1: INSEQ         1                       UV file name (seq. #)
> AIPS 1: INDISK        1                       UV file disk drive #
> AIPS 1:                                    Data selection (multisource):
> AIPS 1: CALSOUR    '1331+305'              Calibrator sources
> AIPS 1:            *rest ' '
> AIPS 1: QUAL         -1                    Calibrator qualifier -1=>all
> AIPS 1: CALCODE    ' '                     Calibrator code '    '=>all
> AIPS 1: SELBAND      -1                    Bandwidth to select (kHz)
> AIPS 1: SELFREQ      -1                    Frequency to select (MHz)
> AIPS 1: FREQID        1                    Freq. ID to select.
> AIPS 1: TIMERANG   *all 0                  Time range to use.
> AIPS 1: BCHAN         1                    Lowest channel number 0=>all
> AIPS 1: ECHAN         0                    Highest channel number
> AIPS 1: ANTENNAS   *all 0                  Antennas to select. 0=all
> AIPS 1: DOFIT      *all 0                  Subset of ANTENNAS list for
> AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
> #
> AIPS 1:                                    which solns are desired.
> AIPS 1: ANTUSE     *all 0                  Mean gain is calculated
> AIPS 1:                                    (CPARM(2)>0) using only the
> AIPS 1:                                    listed antennas. See explain.
> AIPS 1: SUBARRAY      0                    Subarray, 0=>all
> AIPS 1: UVRANGE       0           0        Range of uv distance for full
> AIPS 1:                                    weight
> AIPS 1: WTUV          0                    Weight outside UVRANGE 0=0.
> AIPS 1: WEIGHTIT      0                    Modify data weights function
> AIPS 1:                                    Cal. info for input:
> AIPS 1: DOCALIB       0                    > 0 calibrate data & weights
> AIPS 1:                                    > 99 do NOT calibrate weights
> AIPS 1: GAINUSE       0                    CL table to apply.
> AIPS 1: DOPOL        -1                    If >0 correct polarization.
> AIPS 1: BLVER        -1                    BL table to apply.
> AIPS 1: FLAGVER       0                    Flag table version
> AIPS 1: DOBAND       -1                    If >0 apply bandpass cal.
> AIPS 1:                                    Method used depends on value
> AIPS 1:                                    of DOBAND (see HELP file).
> AIPS 1: BPVER        -1                    Bandpass table version
> AIPS 1: SMOOTH     *all 0                  Smoothing function. See
> AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
> #
> AIPS 1:                                    HELP SMOOTH for details.
> AIPS 1:
> AIPS 1:                                    CLEAN map. See HELP.
> AIPS 1: IN2NAME    '3C286_U'                  Cleaned map name (name)
> AIPS 1: IN2CLASS   'MODEL'                    Cleaned map name (class)
> AIPS 1: IN2SEQ        0                       Cleaned map name (seq. #)
> AIPS 1: IN2DISK       1                       Cleaned map disk unit #
> AIPS 1: INVERS        0                    CC file version #.
> AIPS 1: NCOMP      *all 0                  # comps to use for model.
> AIPS 1:                                    1 value per field
> AIPS 1: FLUX          0                    Lowest CC component used.
> AIPS 1: NMAPS         0                    No. Clean map files
> AIPS 1: CMETHOD    ' '                     Modeling method:
> AIPS 1:                                    'DFT','GRID','    '
> AIPS 1: CMODEL     ' '                     Model type: 'COMP','IMAG'
> AIPS 1: SMODEL     *all 0                  Source model, 1=flux,2=x,3=y
> AIPS 1:                                    See HELP SMODEL for models.
> AIPS 1:
> AIPS 1:                                    Output uv data file.
> AIPS 1: OUTNAME    ' '                        UV file name (name)
> AIPS 1: OUTCLASS   ' '                        UV file name (class)
> AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
> #
> AIPS 1: OUTSEQ        0                       UV file name (seq. #)
> AIPS 1: OUTDISK       1                       UV file disk drive #
> AIPS 1:
> AIPS 1:                                    Solution control adverbs:
> AIPS 1: REFANT       22                    Reference antenna
> AIPS 1: SOLINT        0                    Solution interval (min)
> AIPS 1: SOLSUB        0                    Solution subinterval
> AIPS 1: SOLMIN        0                    Min solution interval
> AIPS 1: APARM         4           0        General parameters
> AIPS 1:               0           0           1=min. no. antennas
> AIPS 1:               0           2           2 > 0 => data divided
> AIPS 1:            *rest 0                    3 > 0 => avg. RR,LL
> AIPS 1:                                       5 > 0 => avg. IFs.
> AIPS 1:                                       6=print level, 1=good,
> AIPS 1:                                         2 closure, 3 SNR
> AIPS 1:                                       7=SNR cutoff (0=>5)
> AIPS 1:                                       8=max. ant. # (no AN)
> AIPS 1:                                       9 > 0 => pass failed soln
> AIPS 1:                                      10 < 99 cal output weights
> AIPS 1:                                    Phase-amplitude Parameters:
> AIPS 1: DOFLAG        0                    Flag on closure error?
> AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
> #
> AIPS 1: SOLTYPE    ' '                     Soln type,'  ','L1','GCON',
> AIPS 1:                                       'R', 'L1R', 'GCOR'
> AIPS 1: SOLMODE    'A&P'                   Soln. mode: 'A&P','P','P!A',
> AIPS 1:                                    'GCON',
> AIPS 1: SOLCON        0                    Gain constraint factor.
> AIPS 1: MINAMPER     10                    Amplitude closure error
> AIPS 1:                                    regarded as excessive in %
> AIPS 1: MINPHSER     10                    Phase closure error regarded
> AIPS 1:                                    as excessive in degrees
> AIPS 1: CPARM         0           0        Phase-amp. parameters
> AIPS 1:               1           1           1 = Min el for gain
> AIPS 1:               1        *rest 0             normalization (deg)
> AIPS 1:                                       2 >0 => normalize gain
> AIPS 1:                                       3 avg. amp. closure err
> AIPS 1:                                       4 avg. ph. closure err
> AIPS 1:                                       5 >0 => scalar average
> AIPS 1:                                       6 limit clipping in robust
> AIPS 1:                                       7 limit display of closure
> AIPS 1:                                         errors
> AIPS 1: SNVER         0                    Output SN table, 0=>new table
> AIPS 1: ANTWT      *all 0                  Ant. weights (0=>1.0)
> AIPS 1: ** press RETURN for more, enter Q or next line to quit print **
> #
> AIPS 1: GAINERR    *all 0                  Std. Dev. of antenna gains.
> AIPS 1: BADDISK    *all 0                  Disk no. not to use for
> AIPS 1:                                       scratch files.
>  >
> 
> 
> On 5/16/08 4:42 PM, Amy Mioduszewski wrote:
>> Sorry.  Send me your CALIB inputs.
>>
>> Amy
>>
>> Jeff Mangum wrote:
>>> That is what I mean.  The models that CALRD finds.  It finds the 
>>> 3C286 model just fine.  When I tries to use it, though, CALIB fails.
>>>
>>> -- Jeff
>>>
>>> On 5/16/08 4:34 PM, Amy Mioduszewski wrote:
>>>> Hi Jeff,
>>>>
>>>> What do you mean by "built in models"?  If you want to use the flux 
>>>> calibrator models you have to load them with CALRD.  VLACALIB will 
>>>> load and use models automatically.
>>>>
>>>> Amy
>>>>
>>>> Jeff Mangum wrote:
>>>>> Hello,
>>>>>
>>>>> I have U-band-only VLA observations taken this February that I am 
>>>>> trying to calibrate.  When I try to use CALIB with one of the 
>>>>> built-in models for 3C286, the task simply dies without indicating 
>>>>> what the problem might be.
>>>>>
>>>>> localh> CALIB1: CALIB USING 20080223     . CH 0   .   1 DISK=  1 
>>>>> USID= 277
>>>>> localh> CALIB1: Doing no flagging this time
>>>>> localh> CALIB1: Purports to die of UNNATURAL causes
>>>>>
>>>>> I have tried modifying several input parameters, but cannot get 
>>>>> past this point.  I wonder if the fact that my data only has 14 
>>>>> antennas (only those with U-band receivers) is causing problems?
>>>>>
>>>>> -- Jeff
>>>>>
>>>>> _______________________________________________
>>>>> Daip mailing list
>>>>> Daip at listmgr.cv.nrao.edu
>>>>> http://listmgr.cv.nrao.edu/mailman/listinfo/daip
>>>>>
> 
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